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1. Fractional Variability—A Tool to Study Blazar Variability

Author

Bernd Schleicher, Axel Arbet-Engels, Dominik Baack, Matteo Balbo, Adrian Biland, Michael Blank, Thomas Bretz, Kai Bruegge, Michael Bulinski, Jens Buss, Manuel Doerr, Daniela Dorner, Dominik Elsaesser, Sergej Grischagin, Dorothee Hildebrand, Lena Linhoff, Karl Mannheim, Sebastian Achim Mueller, Dominik Neise, Andrii Neronov, Maximilian Noethe, Aleksander Paravac, Wolfgang Rhode, Florian Schulz, Kevin Sedlaczek, Amit Shukla, Vitalii Sliusar, Elan von Willert, and Roland Walter

Subjects
blazars, variability, fractional variability, active galactic nuclei, Astronomy, QB1-991
Abstract

Active Galactic Nuclei emit radiation over the whole electromagnetic spectrum up to TeV energies. Blazars are one subtype with their jets pointing towards the observer. One of their typical features is extreme variability on timescales, from minutes to years. The fractional variability is an often used parameter for investigating the degree of variability of a light curve. Different detection methods and sensitivities of the instruments result in differently binned data and light curves with gaps. As they can influence the physics interpretation of the broadband variability, the effects of these differences on the fractional variability need to be studied. In this paper, we study the systematic effects of completeness in time coverage and the sampling rate. Using public data from instruments monitoring blazars in various energy ranges, we study the variability of the bright TeV blazars Mrk 421 and Mrk 501 over the electromagnetic spectrum, taking into account the systematic effects, and compare our findings with previous results. Especially in the TeV range, the fractional variability is higher than in previous studies, which can be explained by the much longer (seven years compared to few weeks) and more complete data sample.

Published
2019
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2. Flux States of Active Galactic Nuclei

Author

Daniela Dorner, Axel Arbet-Engels, Dominik Baack, Matteo Balbo, Adrian Biland, Michael Blank, Thomas Bretz, Kai Bruegge, Michael Bulinski, Jens Buss, Manuel Doerr, Dominik Elsaesser, Dorothee Hildebrand, Lena Linhoff, Karl Mannheim, Sebastian Achim Mueller, Dominik Neise, Andrii Neronov, Maximilian Noethe, Aleksander Paravac, Wolfgang Rhode, Bernd Schleicher, Florian Schulz, Kevin Sedlaczek, Amit Shukla, Vitalii Sliusar, Elan von Willert, Roland Walter, and FACT Collaboration

Subjects
active galactic nuclei, blazars, monitoring, TeV energies, FACT, flux states, flux distributions, duty cycle, Astronomy, QB1-991
Abstract

Blazars are known to show variability on time scales from minutes to years covering a wide range of flux states. Studying the flux distribution of a source allows for various insights. The shape of the flux distribution can provide information on the nature of the underlying variability processes. The level of a possible quiescent state can be derived from the main part of the distribution that can be described by a Gaussian distribution. Dividing the flux states into quiescent and active, the duty cycle of a source can be calculated. Finally, this allows alerting the multi-wavelength and multi-messenger community in case a source is in an active state. To get consistent and conclusive results from flux distributions, unbiased long-term observations are crucial. Only like this is a complete picture of the variability and flux states, e.g., an all-time quiescent state, possible. In seven years of monitoring of bright TeV blazars, the first G-APD Cherenkov telescope (FACT) has collected a total of more than 11,700 hours of physics data with 1500 hours to 3000 hours per source for Mrk 421, Mrk 501, 1ES 1959+650, and 1ES 2344+51.

Published
2019
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3. Unbiased Long-Term Monitoring at TeV Energies

Author

María Magdalena González, Daniela Dorner, Thomas Bretz, and José Andrés García-González

Subjects
monitoring, very high energies (VHE), TeV energies, Astronomy, QB1-991
Abstract

For the understanding of the variable, transient and non-thermal universe, unbiased long-term monitoring is crucial. To constrain the emission mechanisms at the highest energies, it is important to characterize the very high energy emission and its correlation with observations at other wavelengths. At very high energies, only a limited number of instruments is available. This article reviews the current status of monitoring of the extra-galactic sky at TeV energies.

Published
2019
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4. Long-Term Monitoring of Bright Blazars in the Multi-GeV to TeV Range with FACT

Author

Fabian Temme, Jan Adam, Max L. Ahnen, Dominik Baack, Matteo Balbo, Matthias Bergmann, Adrian Biland, Michael Blank, Thomas Bretz, Kai A. Brügge, Jens Buss, Anton Dmytriiev, Daniela Dorner, Sabrina Einecke, Christina Hempfling, Dorothee Hildebrand, Gareth Hughes, Lena Linhoff, Karl Mannheim, Sebastian Müller, Dominik Neise, Andrii Neronov, Max Nöthe, Aleksander Paravac, Felicitas Pauss, Wolfgang Rhode, Amit Shukla, Julia Thaele, and Roland Walter

Subjects
Imaging Air Cherenkov Telescope, First G-APD Cherenkov Telescope, very high energy gamma rays, long-term monitoring, silicon photo multiplier, Astronomy, QB1-991
Abstract

Blazars like Markarian 421 or Markarian 501 are active galactic nuclei (AGN), with their jets orientated towards the observer. They are among the brightest objects in the very high energy (VHE) gamma ray regime (>100 GeV). Their emitted gamma-ray fluxes are extremely variable, with changing activity levels on timescales between minutes, months, and even years. Several questions are part of the current research, such as the question of the emission regions or the engine of the AGN and the particle acceleration. A dedicated longterm monitoring program is necessary to investigate the properties of blazars in detail. A densely sampled and unbiased light curve allows for observation of both high and low states of the sources, and the combination with multi-wavelength observation could contribute to the answer of several questions mentioned above. FACT (First G-APD Cherenkov Telescope) is the first operational telescope using silicon photomultiplier (SiPM, also known as Geigermode—Avalanche Photo Diode, G-APD) as photon detectors. SiPM have a very homogenous and stable longterm performance, and allow operation even during full moon without any filter, leading to a maximal duty cycle for an Imaging Air Cherenkov Telescope (IACT). Hence, FACT is an ideal device for such a longterm monitoring of bright blazars. A small set of sources (e.g., Markarian 421, Markarian 501, 1ES 1959+650, and 1ES 2344+51.4) is currently being monitored. In this contribution, the FACT telescope and the concept of longterm monitoring of bright blazars will be introduced. The results of the monitoring program will be shown, and the advantages of densely sampled and unbiased light curves will be discussed.

Published
2017
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5. Simulations of the M@ <scp>TE</scp> Telescope

Author

Josué Cuzco, Ibrahim Torres, Rodrigo Sacahuí, María M. González, Rubén Alfaro, Yunior Pérez, José Serna, Thomas Bretz, and Daniela Dorner

Subjects
Space and Planetary Science, Astronomy and Astrophysics
Published
2023

6. Probing hadronic interactions using the latest data measured by the Pierre Auger Observatory

Author

Caterina Trimarelli, Pedro Abreu, Marco Aglietta, Ingomar Allekotte, Kévin Almeida Cheminant, Alejandro Almela, Jaime Alvarez-Muniz, Juan Ammerman Yebra, Gioacchino Alex Anastasi, Luis A. Anchordoqui, Belén Andrada, Sofia Andringa, Carla Aramo, Paulo Ricardo Araújo Ferreira, Enrico Arnone, Juan Carlos Arteaga Velazquez, Hernán Gonzalo Asorey, Pedro Assis, Gualberto Avila, Emanuele Avocone, Alina Mihaela Badescu, Alena Bakalova, Alexandru Balaceanu, Felicia Barbato, Jose A. Bellido, Corinne Berat, Mario Edoardo Bertaina, Gopal Bhatta, Peter L. Biermann, Virginia Binet, Kathrin Bismark, Teresa Bister, Jonathan Biteau, Jiri Blazek, Carla Bleve, Johannes Blümer, Martina Bohacova, Denise Boncioli, Carla Bonifazi, Luan Bonneau Arbeletche, Nataliia Borodai, Jeffrey Brack, Thomas Bretz, P. Gabriel Brichetto Orchera, Florian Lukas Briechle, Peter Buchholz, Antonio Bueno, Stijn Buitink, Mario Buscemi, Max Büsken, Anthony Bwembya, Karen S. Caballero-Mora, Lorenzo Caccianiga, Ioana Caracas, Rossella Caruso, Antonella Castellina, Fernando Catalani, Gabriella Cataldi, Lorenzo Cazon, Marcos Cerda, Jose Augusto Chinellato, Jiří Chudoba, Ladislav Chytka, Roger W Clay, Agustín Cobos Cerutti, Roberta Colalillo, Alan Coleman, Maria Rita Coluccia, Rúben Conceição, Antonio Condorelli, Giovanni Consolati, Fernando Contreras, Fabio Convenga, Diego Correia dos Santos, Corbin Covault, Markus Cristinziani, Sergio Dasso, Kai Daumiller, Bruce R. Dawson, Jarryd A. Day, Rogerio M. de Almeida, Joaquin de Jesus, Sijbrand J. de Jong, João de Mello Neto, Ivan De Mitri, Jaime de Oliveira, Danelise de Oliveira Franco, Francesco de Palma, Vitor de Souza, Emanuele De Vito, Antonino Del Popolo, Olivier Deligny, Luca Deval, Armando di Matteo, Madalina Dobre, Carola Dobrigkeit, Juan Carlos D'Olivo, Luis Miguel Domingues Mendes, Rita Cassia dos Anjos, Maria Teresa Dova, Jan Ebr, Mohamed Eman, Ralph Engel, Italo Epicoco, Martin Erdmann, Carlos O. Escobar, Alberto Etchegoyen, Heino Falcke, John Farmer, Glennys R. Farrar, Anderson Campos Fauth, Norberto Fazzini, Fridtjof Feldbusch, Francesco Fenu, Brian Fick, Juan Manuel Figueira, Andrej Filipcic, Thomas Fitoussi, Tomáš Fodran, Toshihiro Fujii, Alan Fuster, Cristina Galea, Claudio Galelli, Beatriz García, Hartmut Gemmeke, Flavia Gesualdi, Alexandru Gherghel-Lascu, Piera Luisa Ghia, Ugo GIACCARI, Marco Giammarchi, Jonas Glombitza, Fabian Gobbi, Fernando Gollan, Geraldina Golup, Mariano Gómez Berisso, Primo F. Gómez Vitale, Juan Pablo Gongora, Juan Manuel González, Nicolas Martin Gonzalez, Isabel Goos, Dariusz Gora, Alessio Gorgi, Marvin Gottowik, Trent D. Grubb, Fausto Guarino, Germano Guedes, Eleonora Guido, Steffen Traugott Hahn, Petr Hamal, Matías Rolf Hampel, Patricia María Hansen, Diego Harari, Violet M. Harvey, Andreas Haungs, Thomas Hebbeker, Dieter Heck, Carlos Hojvat, Jörg R. Hörandel, Pavel Horvath, Miroslav Hrabovsky, Tim Huege, Antonio Insolia, Paula Gina Isar, Petr Janecek, Jeffrey A. Johnsen, Jakub Jurysek, Alex Kääpä, Karl-Heinz Kampert, Bianca Keilhauer, Abha Khakurdikar, Varada Varma Kizakke Covilakam, Hans Klages, Matthias Kleifges, Jonny Kleinfeller, Felix Knapp, Norbert Kunka, Bruno L. Lago, Niklas Langner, Marcelo Augusto Leigui de Oliveira, Vladimir Lenok, Antoine Letessier-Selvon, Isabelle Lhenry-Yvon, Domenico Lo Presti, Luis LOPES, Rebeca López, Lu Lu, Quentin Luce, Jon Paul Lundquist, Allan Machado Payeras, Giovanni Mancarella, Dusan Mandat, Bradley C. Manning, Julien Manshanden, Paul Mantsch, Sullivan Marafico, Federico Maria Mariani, Analisa Mariazzi, Ioana Maris, Giovanni Marsella, Daniele Martello, Sara Martinelli, Oscar Martínez Bravo, Miguel Alexandre Martins, Massimo Mastrodicasa, Hermann-Josef Mathes, James Matthews, Giorgio Matthiae, Eric William Mayotte, Sonja Mayotte, Peter Mazur, Gustavo Medina-Tanco, Diego Melo, Alexander Menshikov, Stanislav Michal, Maria Isabel Micheletti, Lino Miramonti, Silvia Mollerach, François Montanet, Leonel Morejon, Carlo Morello, Ana L. Müller, Katharine Mulrey, Roberto Mussa, Marco Stein Muzio, Wilson M. Namasaka, Alina Nasr-Esfahani, Lukas Nellen, Gabriela Nicora, Mihai Niculescu-Oglinzanu, Marcus Niechciol, Dave Nitz, Ian Norwood, Dalibor Nosek, Vladimír Novotný, Libor Nozka, Achille Nucita, Luis A. Nunez, Cainã Oliveira, Miroslav Palatka, Juan Pallotta, Gonzalo Parente, Alejandra Parra, Jannis Pawlowsky, Miroslav Pech, Jan Pękala, Rodrigo Pelayo, Edyvania Emily Pereira Martins, Johnnier Perez Armand, Carmina Pérez Bertolli, Lorenzo Perrone, Sergio Petrera, Camilla Petrucci, Tanguy Pierog, Mário Pimenta, Manuel Platino, Bjarni Pont, Mart Pothast, Paolo Privitera, Michael Prouza, Andrew Puyleart, Sven Querchfeld, Julian Rautenberg, Diego Ravignani, Maximilian Reininghaus, Jan Ridky, Felix Riehn, Markus Risse, Vincenzo Rizi, Washington Rodrigues de Carvalho, Jorge Rubén Rodriguez Rojo, Matías J. Roncoroni, Simone Rossoni, Markus Roth, Esteban Roulet, Adrian Rovero, Philip Ruehl, Alexandra Saftoiu, Mohit Saharan, Francesco Salamida, Humberto Ibarguen Salazar, Gaetano Salina, Jose Sanabria Gomez, Federico Andrés Sánchez, Edivaldo Moura Santos, Eva Santos, Fred Sarazin, Raul Sarmento, Ricardo Sato, Pierpaolo Savina, Christoph M. Schäfer, Viviana Scherini, Harald Schieler, Martin Schimassek, Michael Schimp, Felix Schlüter, David Schmidt, Olaf Scholten, Harm Schoorlemmer, Petr Schovanek, Frank G. Schröder, Josina Schulte, Tobias Schulz, Sergio J Sciutto, Marina Scornavacche, Alberto Segreto, Srijan Sehgal, Shima Ujjani Shivashankara, Guenter Sigl, Gaia Silli, Octavian Sima, Raluca Smau, Radomir Smida, Paul Sommers, Jorge F. Soriano, Ruben Squartini, Maximilian Stadelmaier, Denis Stanca, Samo Stanič, Jaroslaw Stasielak, Patrick Stassi, Maximilian Straub, Alexander Streich, Mauricio Suárez-Durán, Tristan Sudholz, Tiina Suomijarvi, A. Daniel Supanitsky, Zbigniew Szadkowski, Alex Tapia, Carla Taricco, Charles Timmermans, Olena Tkachenko, Petr Tobiska, Carlos J. Todero Peixoto, Bernardo Tomé, Zoé Torrès, Andres Travaini, Petr Travnicek, Matias Jorge Tueros, Ralf Ulrich, Michael Unger, Lukáš Vaclavek, Martin Vacula, Jose F. Valdés Galicia, Laura Valore, Enrique Varela, Adriana Vásquez-Ramírez, Darko Veberic, Cynthia Ventura, Indira D. Vergara Quispe, Valerio Verzi, Jakub Vicha, Jacco Vink, Serguei Vorobiov, Hernan Wahlberg, Clara Keiko Oliveira Watanabe, Alan Watson, Andreas Weindl, Lawrence Wiencke, Henryk Wilczyński, David Wittkowski, Brian Wundheiler, Alexey Yushkov, Orazio Zapparrata, Enrique Zas, Danilo Zavrtanik, Marko Zavrtanik, and Lukas Zehrer

Published
2022

7. Rapid X-ray Variability in Mkn 421 during a Multiwavelength Campaign

Author

Alex G Markowitz, Krzysztof Nalewajko, Gopal Bhatta, Gulab C Dewangan, Sunil Chandra, Daniela Dorner, Bernd Schleicher, Urszula Pajdosz-Śmierciak, Łukasz Stawarz, Staszek Zola, Michał Ostrowski, Daniele Carosati, Saikruba Krishnan, Rumen Bachev, Erika Benítez, Kosmas Gazeas, David Hiriart, Shao-Ming Hu, Valeri Larionov, Alessandro Marchini, Katsura Matsumoto, A A Nikiforova, Tapio Pursimo, Claudia M Raiteri, Daniel E Reichart, Diego Rodriguez, Evgeni Semkov, Anton Strigachev, Yuki Sugiura, Massimo Villata, James R Webb, Axel Arbet-Engels, Dominik Baack, Matteo Balbo, Adrian Biland, Thomas Bretz, Jens Buss, Laura Eisenberger, Dominik Elsaesser, Dorothee Hildebrand, Roman Iotov, Adelina Kalenski, Karl Mannheim, Alison Mitchell, Dominik Neise, Maximilian Noethe, Aleksander Paravac, Wolfgang Rhode, Vitalii Sliusar, and Roland Walter

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), Astrophysics::High Energy Astrophysical Phenomena, black hole physics, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Mkn 421 [BL Lacertae objects], Astrophysics - Astrophysics of Galaxies, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), active [galaxies], Astrophysics - High Energy Astrophysical Phenomena, Astrophysics::Galaxy Astrophysics, acceleration of particles
Abstract

The study of short-term variability properties in AGN jets has the potential to shed light on their particle acceleration and emission mechanisms. We report results from a four-day coordinated multi-wavelength campaign on the highly-peaked blazar (HBL) Mkn 421 in 2019 January. We obtained X-ray data from AstroSAT, BVRI photometry with the Whole Earth Blazar Telescope (WEBT), and TeV data from FACT to explore short-term multi-wavelength variability in this HBL. The X-ray continuum is rapidly variable on time-scales of tens of ks. Fractional variability amplitude increases with energy across the synchrotron hump, consistent with previous studies; we interpret this observation in the context of a model with multiple cells whose emission spectra contain cutoffs that follow a power-law distribution. We also performed time-averaged and time-resolved (time-scales of 6 ks) spectral fits; a broken power-law model fits all spectra well; time-resolved spectral fitting reveals the usual hardening when brightening behaviour. Intra-X-ray cross correlations yield evidence for the 0.6-0.8 keV band to likely lead the other bands by an average of 4.6 +- 2.6 ks, but only during the first half of the observation. The source displayed minimal night-to-night variability at all wavebands thus precluding significant interband correlations during our campaign. The broadband SED is modeled well with a standard one-zone leptonic model, yielding jet parameters consistent with those obtained from previous SEDs of this source., This article has been accepted for publication in The Monthly Notices of the Royal Astronomical Society (2022), and is published in Volume 513, Issue 2, pp.1662-1679. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. 19 pages; 12 figures

Published
2022

8. Searching for VHE gamma-ray emission associated with IceCube neutrino alerts using FACT, H.E.S.S., MAGIC, and VERITAS

Author

Konstancja, Satalecka, Acciari, Victor A., Stefano, Ansoldi, Lucio Angelo Antonelli, Axel Arbet Engels, Manuel, Artero, Katsuaki, Asano, Dominik, Baack, Ana, Babic, Andr('(e))s, Baquero, Ulisses Barres de Almeida, Juan Abel Barrio, Ivana, Batkovi('(c)), Josefa Becerra Gonzalez, Wlodek, Bednarek, Lorenzo, Bellizzi, Elisa, Bernardini, Maria-Isabel, Bernardos, Alessio, Berti, Jürgen, Besenrieder, Wrijupan, Bhattacharyya, Ciro, Bigongiari, Adrian, Biland, Oscar, Blanch, Hendrik, Bökenkamp, Giacomo, Bonnoli, Zeljka, Bosnjak, Giovanni, Busetto, Roberto, Carosi, Giovanni, Ceribella, Matteo, Cerruti, Yating, Chai, Ashot, Chilingarian, Stefan, Cikota, Sidika Merve Colak, Eduardo, Colombo, Jose Luis Contreras, Juan, Cortina, Stefano, Covino, Giacomo D( extquotesingle)Amico, Valerio D( extquotesingle)Elia, Paolo Da Vela, Francesco, Dazzi, Alessandro De Angelis, Barbara De Lotto, Manuel, Delfino, Jordi, Delgado, Carlos Delgado Mendez, Davide, Depaoli, Federico Di Pierro, Leonardo Di Venere, Elia Do Souto Espi(~(n))eira, Dijana Dominis Prester, Alice, Donini, Daniela, Dorner, Michele, Doro, Dominik, Elsaesser, Vandad Fallah Ramazani, Alicia, Fattorini, Maria Victoria Fonseca, Lluis, Font, Christian, Fruck, Satoshi, Fukami, Yasushi, Fukazawa, Garc('(i))a L('(o))pez, Ramon J., Markus, Garczarczyk, Sargis, Gasparyan, Markus, Gaug, Giglietto, Nicola, Francesco, Giordano, Pawel, Gliwny, Nikola, Godinovic, David, Green, Jarred Gershon Green, Daniela, Hadasch, Alexander, Hahn, Lea, Heckmann, Javier, Herrera, John, Hoang, Dario, Hrupec, Moritz, Hütten, Tomohiro, Inada, Kazuma, Ishio, Yuki, Iwamura, Irene Jim('(e))nez Mart('(i))nez, Jenni, Jormanainen, L('(e))a, Jouvin, Marie, Karjalainen, Daniel, Kerszberg, Yukiho, Kobayashi, Hidetoshi, Kubo, Junko, Kushida, Alessandra, Lamastra, Damir, Lelas, Francesco, Leone, Elina, Lindfors, Lena, Linhoff, Saverio, Lombardi, Francesco, Longo, Ruben, Lopez-Coto, Marcos, L('(o))pez-Moya, Alicia, L('(o))pez-Oramas, Loporchio, Serena, Bernardo Machado de Oliveira Fraga, Camilla, Maggio, Pratik, Majumdar, Martin, Makariev, Manuela, Mallamaci, Galina, Maneva, Marina, Manganaro, Karl, Mannheim, Laura, Maraschi, Mos(`(e)), Mariotti, Manel, Martinez, Daniel, Mazin, Stefano, Menchiari, Simone, Mender, Sa( (s))a Mi('(c))anovi('(c)), Davide, Miceli, Tjark, Miener, Jose Miguel Miranda, Razmik, Mirzoyan, Edgar, Molina, Abelardo, Moralejo, Daniel, Morcuende, Victoria, Moreno, Elena, Moretti, Takeshi, Nakamori, Lara, Nava, Vitaly, Neustroev, Cosimo, Nigro, Kari, Nilsson, Kyoshi, Nishijima, Koji, Noda, Seiya, Nozaki, Yoshiki, Ohtani, Tomohiko, Oka, Jorge, Otero-Santos, Simona, Paiano, Michele, Palatiello, David, Paneque, Riccardo, Paoletti, Paredes, Josep M., Lovro, Pavleti('(c)), Pablo, Pe(~(n))il, Massimo, Persic, Marine, Pihet, Pier Giorgio Prada Moroni, Elisa, Prandini, Chaitanya, Priyadarshi, Ivica, Puljak, Wolfgang, Rhode, Marc, Rib('(o)), Javier, Rico, Chiara, Righi, Andrea, Rugliancich, Narek, Sahakyan, Takayuki, Saito, Shunsuke, Sakurai, Francesco Gabriele Saturni, Bernd, Schleicher, Kevin, Schmidt, Thomas, Schweizer, Julian, Sitarek, Iva, ( (S))nidari('(c)), Dorota, Sobczy('(n))ska, Alessia, Spolon, Antonio, Stamerra, Jelena Stri( (s))kovi('(c)), Derek, Strom, Marcel, Strzys, Yusuke, Suda, Tihomir, Suri('(c)), Mitsunari, Takahashi, Ryuji, Takeishi, Fabrizio, Tavecchio, Petar, Temnikov, Tomislav, Terzic, Masahiro, Teshima, Luca, Tosti, Stefano, Truzzi, Antonio, Tutone, Santiago, Ubach, Juliane van Scherpenberg, Gaia, Vanzo, Monica VAZQUEZ ACOSTA, Sofia, Ventura, Vassil, Verguilov, Carlo Francesco Vigorito, Vincenzo, Vitale, Ievgen, Vovk, Martin, Will, Carolin, Wunderlich, Tokonatsu, Yamamoto, Darko, Zari('(c)), Matteo, Balbo, Thomas, Bretz, Jens, Buss, Laura, Eisenberger, Dorothee, Hildebrand, Roman, Iotov, Adelina, Kalenski, Dominik, Neise, Maximilian, Noethe, Aleksander, Paravac, Vitalii, Sliusar, Roland, Walter, Rasha, Abbasi, Markus, Ackermann, Jenni, Adams, Juanan, Aguilar, Ahlers, M., Maryon, Ahrens, Cyril Martin Alispach, Antonio Augusto Alves Junior, Najia Moureen Binte Amin, Rui, An, Karen, Andeen, Tyler, Anderson, Gisela, Anton, Carlos, Arguelles, Yosuke, Ashida, Spencer, Axani, Xinhua, Bai, Aswathi Balagopal, V., Anastasia Maria Barbano, Barwick, S. W., Benjamin, Bastian, Vedant, Basu, Sebastian, Baur, Bay, R. C., Beatty, J. J., Becker, K. -H., Julia Becker Tjus, Chiara, Bellenghi, Segev, Benzvi, Berley, D., Besson, D. Z., Gary, Binder, Daniel, Bindig, Blaufuss, E., Summer, Blot, Matthias, Boddenberg, Federico, Bontempo, Jurgen, Borowka, Boser, S., Olga, Botner, Jakob, Bottcher, Etienne, Bourbeau, Federica, Bradascio, Braun, J., Stephanie, Bron, Jannes, Brostean-Kaiser, Sally-Ann, Browne, Alexander, Burgman, Ryan, Burley, Raffaela, Busse, Michael, Campana, Erin, Carnie-Bronca, Chujie, Chen, Dmitry, Chirkin, Koun, Choi, Bryanlee, Clark, Kenneth, Clark, Lew, Classen, Alan, Coleman, Gabriel, Collin, Conrad, J. M., Paul, Coppin, Pablo, Correa, Cowen, D. F., Cross, R., Christian, Dappen, Pranav, Dave, Catherine DE CLERCQ, James, Delaunay, Hans, Dembinski, Kunal, Deoskar, Sam De Ridder, Abhishek, Desai, Paolo, Desiati, Krijn de Vries, Gwenhaël de Wasseige, Meike De With, Tyce, Deyoung, Sukeerthi, Dharani, Alejandro, Diaz, Juan Carlos Diaz-Velez, Markus, Dittmer, Hrvoje, Dujmovic, Matt, Dunkman, Michael, Duvernois, Emily, Dvorak, Thomas, Ehrhardt, Philipp, Eller, Ralph, Engel, Hannah, Erpenbeck, John, Evans, Evenson, P. A., Kwok Lung Fan, Fazely, A. R., Sebastian, Fiedlschuster, Aaron, Fienberg, Kirill, Filimonov, Chad, Finley, Leander, Fischer, Derek, B Fox, Anna, Franckowiak, Elizabeth, Friedman, Alexander, Fritz, Philipp, Furst, Gaisser, T. K., Jay, Gallagher, Erik, Ganster, Alfonso, Garcia, Simone, Garrappa, Gerhardt, L., Ava, Ghadimi, Christian, Glaser, Theo, Glauch, Thorsten, Glusenkamp, Goldschmidt, A., Javier, Gonzalez, Sreetama, Goswami, Darren, Grant, Timoth('(e))e, Gr('(e))goire, Spencer, Griswold, Mehmet, Gunduz, Christoph, Günther, Christian, Haack, Allan, Hallgren, Halliday, R., Halve, L., Halzen, F., Martin Ha Minh, Kael, Hanson, John, Hardin, Harnisch, Alexander A., Andreas, Haungs, Simon, Hauser, Dustin, Hebecker, Helbing, K., Felix, Henningsen, Hettinger, Emma C., Stephanie, Hickford, Joshua, Hignight, Colton, Hill, Hill, G. C., Kara, Hoffman, Ruth, Hoffmann, Tobias, Hoinka, Benjamin, Hokanson-Fasig, Hoshina, K., Feifei, Huang, Matthias, Huber, Thomas, Huber, Klas, Hultqvist, Mirco, Hunnefeld, Raamis, Hussain, Seongjin, In, Nad(`(e))ge, Iovine, Aya, Ishihara, Matti, Jansson, George, Japaridze, Minjin, Jeong, Ben, Jones, Donghwa, Kang, Woosik, Kang, Xinyue, Kang, Alexander, Kappes, David, Kappesser, Timo, Karg, Martina, Karl, Karle, A., Katz, U., Kauer, M., Moritz, Kellermann, Kelley, J. L., Ali, Kheirandish, Ken( extquotesingle)ichi Kin, Thomas, Kintscher, Joanna, Kiryluk, Spencer, Klein, Ramesh, Koirala, Hermann, Kolanoski, Tomas, Kontrimas, Lutz, Kopke, Claudio, Kopper, Sandro, Kopper, Koskinen, D. J., Paras, Koundal, Michael, Kovacevich, Marek, Kowalski, Tetiana, Kozynets, Emma, Kun, Naoko, Kurahashi, Neha, Lad, Cristina Lagunas Gualda, Justin, Lanfranchi, Michael, J Larson, Frederik Hermann Lauber, Jeffrey, Lazar, Jiwoong, Lee, Kayla, Leonard, Agnieszka, Leszczy('(n))ska, Yijia, Li, Massimiliano, Lincetto, Qinrui, Liu, Maria, Liubarska, Elisa, Lohfink, Cristian Jesus Lozano Mariscal, Lu, Lu, Francesco, Lucarelli, Andrew, Ludwig, William, Luszczak, Yang, Lyu, Wing Yan Ma, James, Madsen, Kendall, Mahn, Yuya, Makino, Sarah, Mancina, Ioana Codrina Maris, Maruyama, Reina H., Mase, K., Thomas, Mcelroy, Frank, Mcnally, James Vincent Mead, Meagher, K., Andres, Medina, Maximilian, Meier, Stephan, Meighen-Berger, Jessie, Micallef, Daniela, Mockler, Teresa, Montaruli, Roger, Moore, Morse, R., Marjon, Moulai, Richard, Naab, Ryo, Nagai, Uwe, Naumann, Jannis, Necker, Le Viet Nguyen, Hans, Niederhausen, Mehr, Nisa, Sarah, Nowicki, Dave, Nygren, Anna Obertacke Pollmann, Marie, Oehler, Olivas, A., Erin O( extquotesingle)Sullivan, Hershal, Pandya, Daria, Pankova, Nahee, Park, Grant, Parker, Ek Narayan Paudel, Larissa, Paul, Carlos Perez de los Heros, Lilly, Peters, Saskia, Philippen, Damian, Pieloth, Sarah, Pieper, Martin, Pittermann, Pizzuto, A., Plum, M., Yuiry, Popovych, Alessio, Porcelli, Maria Prado Rodriguez, Buford Price, P., Brandom, Pries, Gerald, Przybylski, Christoph, Raab, Amirreza, Raissi, Mohamed, Rameez, Rawlins, K., Immacolata Carmen Rea, Abdul, Rehman, Ren('(e)), Reimann, Giovanni, Renzi, Elisa, Resconi, Simeon, Reusch, Mike, Richman, Benedikt, Riedel, Ella, Roberts, Sally, Robertson, Gerrit, Roellinghoff, Martin, Rongen, Carsten, Rott, Tim, Ruhe, Dirk, Ryckbosch, Devyn Rysewyk Cantu, Ibrahim, Safa, Julian, Saffer, Sebastian Sanchez Herrera, Alexander, Sandrock, Joakim, Sandroos, Marcos, Santander, Subir, Sarkar, Sourav, Sarkar, Maximilian Karl Scharf, Merlin, Schaufel, Harald, Schieler, Sebastian, Schindler, Schlunder, P., Torsten, Schmidt, Austin, Schneider, Judith, Schneider, Schröder, Frank G., Lisa Johanna Schumacher, Georg, Schwefer, Steve, Sclafani, Seckel, D., Surujhdeo, Seunarine, Ankur, Sharma, Shefali, Shefali, Manuel, Silva, Barbara, Skrzypek, Ben, Smithers, Robert, Snihur, Jan, Soedingrekso, Dennis, Soldin, Christian, Spannfellner, Glenn, Spiczak, Christian, Spiering, Juliana, Stachurska, Michael, Stamatikos, Stanev, T., Robert, Stein, Joeran, Stettner, Steuer, A., Stezelberger, T., Timo, Sturwald, Thomas, Stuttard, Sullivan, G. W., Taboada, I., Frederik, Tenholt, Samvel, Ter-Antonyan, Tilav, S., Franziska, Tischbein, Kirsten, Tollefson, Christoph, Tönnis, Simona, Toscano, Delia, Tosi, Alexander, Trettin, Maria, Tselengidou, Chunfai, Tung, Andrea, Turcati, Roxanne, Turcotte, Colin, Turley, Jean Pierre Twagirayezu, Bunheng, Ty, Martin Unland Elorrieta, Nora, Valtonen-Mattila, Justin, Vandenbroucke, Nick van Eijndhoven, David, Vannerom, Jakob van Santen, Stef, Verpoest, Matthias, Vraeghe, Walck, C., Timothyblake, Watson, Chris, Weaver, Philip, Weigel, Andreas, Weindl, Matthew, Weiss, Jan, Weldert, Chris, Wendt, Johannes, Werthebach, Mark, Weyrauch, Nathan, Whitehorn, Wiebusch, C. H., Dawn, Williams, Martin, Wolf, Kurt, Woschnagg, Gerrit, Wrede, Johan, Wulff, Xianwu, Xu, Yiqian, Xu, Juan Pablo Yanez, Yoshida, S., Shiqi, Yu, Tianlu, Yuan, Zelong, Zhang, Weidong, Jin, Hassan, Abdalla, Felix, Aharonian, Faical, Ait-Benkhali, Oguzhan, Anguener, Cornelia, Arcaro, Celine, Armand, Tom, Armstrong, Halim, Ashkar, Michael, Backes, Vardan, Baghmanyan, Victor Barbosa Martins, Anna, Barnacka, Monica, Barnard, Rowan, Batzofin, Yvonne, Becherini, David, Berge, Konrad, Bernlöhr, Baiyang, Bi, Markus, Boettcher, Catherine, Boisson, Julien, Bolmont, Mathieu de Bony, Mischa, Breuhaus, Robert, Brose, Francois, Brun, Tomasz, Bulik, Thomas, Bylund, Floriane, Cangemi, Sami, Caroff, Sabrina, Casanova, Jaqueline, Catalano, Pauline, Chambery, Tej Bahadur Chand, Andrew, Chen, Garret, Cotter, Malgorzata, Curlo, Jean Damascene Mbarubucyeye, Isak Delberth Davids, James, Davies, Justine, Devin, Arache, Djannati-Ataï, Anton, Dmytriiev, Axel, Donath, Victor, Doroshenko, Lente, Dreyer, Louis Du Plessis, Connor, Duffy, Kathrin, Egberts, Sabrina, Einecke, Gabriel, Emery, Jean-Pierre, Ernenwein, Steven, Fegan, Kirsty, Feijen, Armand, Fiasson, Gaëtan Fichet de Clairfontaine, Gerard, Fontaine, Lott, Frans, Matthias, Fuessling, Stefan, Funk, Stefano, Gabici, Yves, Gallant, Shahede, Ghafourizade, Gianluca, Giavitto, Luca, Giunti, Dorit, Glawion, Jean-Francois, Glicenstein, Marie-H('(e))l(`(e))ne, Grondin, Sumari, Hattingh, Maria, Haupt, German, Hermann, Jim, Hinton, Werner, Hofmann, Clemens, Hoischen, Tim, Holch, Markus, Holler, Dieter, Horns, Zhiqiu, Huang, David, Huber, Mario, Hörbe, Marek, Jamrozy, Felix, Jankowsky, Vikas, Joshi, Ira, Jung, Eli, Kasai, Krzysztof, Katarzynski, Ul(`(i)), Katz, Dmitry, Khangulyan, Bruno, Khelifi, Stefan, Klepser, Wlodek, Kluzniak, Nukri, Komin, Ruslan, Konno, Karl, Kosack, Dmitriy, Kostunin, Michael, Kreter, Ga( (s))per Kukec Mezek, Anu, Kundu, Giovanni, Lamanna, S('(e))bastien Le Stum, Anne, Lemiere, Marianne, Lemoine-Goumard, Jean-Philippe, Lenain, Fabian, Leuschner, Christelle, Levy, Thomas, Lohse, Anna, Luashvili, Iryna, Lypova, Jonathan, Mackey, Jhilik, Majumdar, Denys, Malyshev, Dmitry, Malyshev, Vincent, Marandon, Paolo, Marchegiani, Alexandre, Marcowith, Arnaud, Mares, Guillem Marti( extquotesingle)i-Devesa, Ramin, Marx, Gilles, Maurin, Pieter, Meintjes, Manuel, Meyer, Alison, Mitchell, Rafal, Moderski, Lars, Mohrmann, Alessandro, Montanari, Chris, Moore, Paul, Morris, Emmanuel, Moulin, Jacques, Muller, Thomas, Murach, Kaori, Nakashima, Mathieu Naurois (de), Amid, Nayerhoda, Hambeleleni, Ndiyavala, Jacek, Niemiec, Angel, Noel, Paul O( extquotesingle)Brien, Laenita Lorraine Oberholzer, Stefan, Ohm, Laura, Olivera-Nieto, Emma Ona-Wilhelmi (de), Michal, Ostrowski, Sebastian, Panny, Michael, Panter, Dan, Parsons, Giada, Peron, Santiago, Pita, Vincent, Poireau, Dmitry, Prokhorov, Heike, Prokoph, Gerd, Puehlhofer, Michael, Punch, Andreas, Quirrenbach, Patrick, Reichherzer, Anita, Reimer, Olaf, Reimer, Quentin, Remy, Matthieu, Renaud, Brian, Reville, Frank, Rieger, Carlo, Romoli, Gavin, Rowell, Bronislaw, Rudak, Hector Rueda Ricarte, Edna Ruiz Velasco, Vardan, Sahakian, Simon, Sailer, Heiko, Salzmann, David, Sanchez, Andrea, Santangelo, Manami, Sasaki, Johannes, Schaefer, Hester, Schutte, Ullrich, Schwanke, Fabian, Schüssler, Mohanraj, Senniappan, Albert, Seyffert, Shapopi, Jimmy N. S., Kleopas, Shiningayamwe, Rachel, Simoni, Atreyee, Sinha, Helene, Sol, Hugh, Spackman, Andreas, Specovius, Samuel Timothy Spencer, Marion, Spir-Jacob, Lukasz, Stawarz, Riaan, Steenkamp, Christian, Stegmann, Simon, Steinmassl, Constantin, Steppa, Lei, Sun, Tadayuki, Takahashi, Takaaki, Tanaka, Thomas, Tavernier, Andrew, Taylor, Regis, Terrier, Hannes, Thiersen, Charles, Thorpe-Morgan, Martin, Tluczykont, Lenka, Tomankova, Michelle, Tsirou, Naomi, Tsuji, Richard, Tuffs, Yasunobu, Uchiyama, Johann van der Walt, Christopher van Eldik, Carlo van Rensburg, Brian van Soelen, George, Vasileiadis, Johannes, Veh, Christo, Venter, Pascal, Vincent, Jacco, Vink, Völk, Heinrich J., Stefan, Wagner, Jason John Watson, Felix, Werner, Richard, White, Alicja, Wierzcholska, Yu Wun Wong, Hend, Yassin, Anke, Yusafzai, Michael, Zacharias, Roberta, Zanin, Davit, Zargaryan, Andrzej, Zdziarski, Andreas, Zech, Sylvia, Zhu, Andreas, Zmija, Samuel, Zouari, Natalia, Zywucka, The FACT Collaboration, The H.E.S.S. Collaboration, The IceCube Collaboration, The MAGIC Collaboration, The VERITAS Collaboration, and Współautorami artykułu są członkowie Magic Collaboration, IceCube Collaboration, FACT Collaboration, H.E.S.S. Collaboration, VERITAS Collaboration w liczbie 808

Subjects
Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Point source, Astrophysics::High Energy Astrophysical Phenomena, Gamma ray, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, IACT, Astrophysics, law.invention, High Energy Physics - Experiment, Telescope, High Energy Physics - Experiment (hep-ex), law, HESS - Abteilung Hinton, ddc:530, High Energy Physics::Experiment, MAGIC (telescope), Neutrino, Blazar, Astrophysics - High Energy Astrophysical Phenomena, Cherenkov radiation
Abstract

The realtime follow-up of neutrino events is a promising approach to search for astrophysical neutrino sources. It has so far provided compelling evidence for a neutrino point source: the flaring gamma-ray blazar TXS 0506+056 observed in coincidence with the high-energy neutrino IceCube-170922A detected by IceCube. The detection of very-high-energy gamma rays (VHE, $\mathrm{E} > 100\,\mathrm{GeV}$) from this source helped establish the coincidence and constrained the modeling of the blazar emission at the time of the IceCube event. The four major imaging atmospheric Cherenkov telescope arrays (IACTs) - FACT, H.E.S.S., MAGIC, and VERITAS - operate an active follow-up program of target-of-opportunity observations of neutrino alerts sent by IceCube. This program has two main components. One are the observations of known gamma-ray sources around which a cluster of candidate neutrino events has been identified by IceCube (Gamma-ray Follow-Up, GFU). Second one is the follow-up of single high-energy neutrino candidate events of potential astrophysical origin such as IceCube-170922A. GFU has been recently upgraded by IceCube in collaboration with the IACT groups. We present here recent results from the IACT follow-up programs of IceCube neutrino alerts and a description of the upgraded IceCube GFU system., Presented at the 37th International Cosmic Ray Conference (ICRC 2021). See arXiv:2107.06966 for all IceCube contributions. See arXiv:2108.05257 for all H.E.S.S. contributions

Published
2022

9. Cosmic ray mass composition study using a Random Forest applied to data from the IceAct telescopes

Author

Larissa Paul, Karen Andeen, Matthias Plum, Thomas Bretz, John Hewitt, Adrian Zink, and for the IceCube Collaboration

Subjects
Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Physics::Atmospheric and Oceanic Physics
Abstract

The IceAct telescopes are prototype Imaging Air Cherenkov telescopes (IACTs)situated at the IceCube Neutrino Observatory at the geographic South Pole. The IceAct telescopes measure the electromagnetic air shower component of cosmic rays in the atmosphere, which iscomplementary to the muonic componentmeasuredby the IceCubein-ice detector and the particle footprint measured at the surface by IceTop. For this Monte Carlo study a random forest is used to analyze the mass composition of the cosmic rays spectrum using the three independent measurements of the cosmic ray air showers provided by the different detector components.

Published
2022
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10. FACT - Database-based Analysis and Spectrum Calculations

Author

Laura Eisenberger, Alison Mitchell, Adelina Kalenski, Adrian Biland, Roland Walter, Dominik Baack, Roman Iotov, Maximilian Noethe, Dominik Neise, Daniela Dorner, Dorothee Hildebrand, Jens Buss, Dominik Elsaesser, Thomas Bretz, Vitalii Sliusar, Wolfgang Rhode, Karl Mannheim, Axel Arbet-Engels, Aleksander Paravac, Matteo Balbo, and Bernd Schleicher

Subjects
Database, Computer science, business.industry, Event (computing), Photodetector, computer.software_genre, law.invention, Telescope, Software, Duty cycle, law, Observatory, Latency (engineering), business, computer, Cherenkov radiation
Abstract

The First G-APD Cherenkov Telescope (FACT) is located at the Observatory Roque de los Muchachos on the Canary island La Palma. It uses the imaging air Cherenkov technique to detect gamma rays. With the help of silicon based photosensors in the camera, FACT is an ideal instrument to monitor a small sample of sources with a good time coverage. The automatic operation of the telescope allows an increase of the duty cycle of the instrument. An SQL database is part of the automatic analysis chain, where data on an event basis are stored. This way of storing the data has a several advantages. It can provide easy web-access to all data with no need of creating different user accounts for the analysers and without using special software. The data selection is done via simple queries to the database. This allows very flexible and powerful queries with, for example, user-defined time binning or background suppression. By using observed and simulated events, the complete analysis chain can be done, including the calculation of the measured energy spectrum. This could also be implemented to the Quick-Look Analysis to provide spectral information during the night with a low latency., PoS: Proceedings of Science, 395, ISSN:1824-8039, 37th International Cosmic Ray Conference (ICRC 2021)

Published
2022
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11. Periodicity Analysis of Mrk 501 and Mrk 421 in Gamma Rays

Author

Dominik Neise, Torsten Enßlin, Axel Arbet-Engels, Volodymyr Marchenko, Adrian Biland, Adelina Kalenski, Thomas Bretz, Bernd Schleicher, Laura Eisenberger, Dominik Elsaesser, Matteo Balbo, Daniela Dorner, Wolfgang Rhode, Phillip Arras, Roland Walter, Vincent Eberle, Fabian Theissen, Vitalii Sliusar, Karl Mannheim, Natalia Zywucka, Alison Mitchell, Andrija Kostić, Dorothee Hildebrand, Aleksander Paravac, Mariusz Tarnopolski, Michael Kreter, Manuel Boettcher, Dominik Baack, Roman Iotov, Maximilian Noethe, and Jens Buss

Subjects
Physics, Active galactic nucleus, Astrophysics::High Energy Astrophysical Phenomena, Gamma ray, Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Light curve, law.invention, Telescope, Binary black hole, law, Quasiperiodic function, Blazar, Cherenkov radiation, Astrophysics::Galaxy Astrophysics
Abstract

Blazars, a subclass of active galactic nuclei (AGNs), are highly variable objects. Quasiperiodic oscillations (QPOs), which might originate from a binary black hole located at the AGN core,have been found in some blazar light curves. For the blazars Mrk 421 and Mrk 501, we test the possible QPO behavior using a variety of methods (generalized Lomb-Scargle periodogram,continuous-time autoregressive moving average models, wavelet scalograms, and A−T plane), studying systematic effects in detail. We use gamma-ray light curves from FACT, a ground-based imaging air Cherenkov telescope. We report herein on a 3 sigma significant QPO in Mrk 421., PoS: Proceedings of Science, 395, ISSN:1824-8039, 37th International Cosmic Ray Conference (ICRC 2021)

Published
2022

12. Extraction of the Muon Signals Recorded with the Surface Detector of the Pierre Auger Observatory Using Recurrent Neural Networks

Author

Jose Chinellato, Marvin Gottowik, Dariusz Gora, Eric Mayotte, A. Gorgi, M. Gómez Berisso, Alan Coleman, S. J. Saffi, Ioana Caracas, R. C. Shellard, R.J. Barreira Luz, Miroslav Pech, M. Pothast, Pavel Horvath, A. Letessier-Selvon, Mario Buscemi, G. De Mauro, A. Tapia, Jörg R. Hörandel, I. Lhenry-Yvon, P. Ruehl, L. Valore, H. Gemmeke, Lorenzo Cazon, C. Pérez Bertolli, M. Suárez-Durán, M. Unger, E. M. Santos, Sullivan Marafico, Clara Keiko Oliveira Watanabe, Serguei Vorobiov, Marco Giammarchi, Jon Paul Lundquist, A. Menshikov, R. Alves Batista, Bruce R. Dawson, F. Pedreira, Sofia Andringa, Julien Manshanden, Andres Travaini, E. Varela, J.D. Sanabria Gomez, Roberto Mussa, Frank G. Schröder, P.O. Mazur, Marina Scornavacche, Jonathan Biteau, F. Salamida, A. Yushkov, Paul Sommers, Maximilian Reininghaus, Raul Sarmento, Felix Schlüter, Fabian Gobbi, Ioana Codrina Maris, Violet M. Harvey, D. Harari, Martina Bohacova, G. P. Guedes, Toshihiro Fujii, Jakub Juryšek, John Farmer, D. Nitz, G. Cataldi, V. Scherini, J. Rautenberg, M. Risse, Jonathan Blazek, Q. Luce, Juan Pablo Gongora, Alena Bakalova, K. Choi, Esteban Roulet, D. Melo, M. Schimp, H. J. Mathes, A. Puyleart, Stanislav Michal, Corinne Berat, M. Giller, Orazio Zapparrata, B. C. Manning, Marcio Aparecido Muller, Maria-Teresa Dova, Markus Roth, R. Sato, Lourenco Lopes, P. Abreu, D. Ravignani, G. Golup, N. Kunka, T. Bister, Maria Rita Coluccia, G. C. Hill, Maximilian Stadelmaier, J. F. Valdés Galicia, I. De Mitri, N. Fazzini, Petr Hamal, Ana Martina Botti, Francesco Fenu, Steffen Hahn, Juan Carlos D'Olivo, T. Pierog, Antonio Condorelli, Alina Mihaela Badescu, Cristina Galea, Jonas Glombitza, F. C. T. Barbato, M. Prouza, Justin M. Albury, P. L. Ghia, L. R. Wiencke, S. Schröder, Niklas Langner, Italo Epicoco, G. Parente, Fabrizia Canfora, Jose J. Gonzalez, Dusan Mandat, Ralph Engel, J. Ridky, J. Rodriguez Rojo, Fridtjof Feldbusch, Enrique Zas, Lorenzo Caccianiga, L. Zehrer, Thomas Hebbeker, M. A. Leigui de Oliveira, Sergio Dasso, Tristan Sudholz, M. I. Micheletti, J. Chudoba, F. Riehn, Carola Dobrigkeit, M. Muzio, V. Novotny, A.L. Garcia Vegas, C. M. Schäfer, Marcel Köpke, M. Platino, François Montanet, A. Insolia, M. Kleifges, D. Zavrtanik, Fernando Contreras, Valerio Verzi, B. Tome, Martín Miguel Freire, Rossella Caruso, B. L. Lago, A. Lucero, Fernando Catalani, Bjarni Pont, E.E. Pereira Martins, J. de Oliveira, J. Pȩkala, Alejandro Almela, Jaime Alvarez-Muñiz, Alexandru Gherghel-Lascu, Brian Fick, Josina Schulte, V. Pirronello, C. J.W.P. Timmermans, Martin Vacula, Julian Kemp, Philipp Papenbreer, Rúben Conceição, M. E. Bertaina, Alan Watson, M. Perlin, Mihai Niculescu-Oglinzanu, L. Bonneau Arbeletche, G. Marsella, Petr Travnicek, Paula Gina Isar, Peter Hansen, W. M. Namasaka, M. Mastrodicasa, Carla Bleve, Rodrigo Guedes Lang, David Wittkowski, Lukáš Vaclavek, Belén Andrada, A. C. Rovero, Eleonora Guido, G. Mancarella, Jesús Peña-Rodríguez, B. Keilhauer, G. Salina, Olivier Deligny, Trent D. Grubb, F. Guarino, John Matthews, Peter Buchholz, Heino Falcke, Alexandru Balaceanu, Vladimir Lenok, P. Tobiska, L. Perrone, Alex Kääpä, Magdalena Cerdá, Juan Manuel Figueira, Roberta Colalillo, Carla Aramo, Matías J. Roncoroni, S. J. Sciutto, R.C. dos Anjos, A. G. Mariazzi, Adriana Vásquez-Ramírez, Vincenzo Rizi, Julien Souchard, D. Martello, J. Vicha, Hernán Asorey, A. Di Matteo, Juan Miguel Carceller, Silvia Mollerach, Flavia Gesualdi, Tomáš Fodran, Alina Nasr-Esfahani, M. Palatka, Xavier Bertou, Marco Aglietta, O. Martínez Bravo, B. Wundheiler, A. Zepeda, Miroslav Hrabovský, Pedro Assis, H. Martinez, A. Etchegoyen, Jeffrey A. Johnsen, L. Lu, H. Schieler, Ugo Giaccari, N. González, A. Segreto, J. F. Soriano, Günter Sigl, Antonella Castellina, A. Haungs, P. Stassi, Radomir Smida, A. Machado Payeras, Thomas Bretz, Gaia Silli, A. Filipčič, Kai Daumiller, F. Sanchez, Petr Janecek, Corbin Covault, F. Sarazin, Srijan Sehgal, Matías Rolf Hampel, Fernando Gollan, S. Petrera, Marc Weber, F. de Palma, P. Mantsch, Lino Miramonti, V. de Souza, D. de Oliveira Franco, G. Matthiae, Z. Szadkowski, Christian Sarmiento-Cano, P. Savina, W. Rodrigues de Carvalho, Antonio Bueno, G. Farrar, T. Huege, Jeffrey Brack, Olaf Scholten, Humberto Ibarguen Salazar, R. M. de Almeida, Gualberto Avila, Octavian Sima, Nataliia Borodai, Miguel Mostafa, A. Fuster, Samo Stanič, D. Lo Presti, D. Correia dos Santos, Isabel Goos, D. Heck, Rodrigo Pelayo, S. J. De Jong, L. Nellen, L. Anchordoqui, A. Taboada, Stijn Buitink, Katie Mulrey, M. del Río, Jarryd A. Day, A. Saftoiu, P.F. Gómez Vitale, C. Morello, A.C. Cobos Cerutti, T. Suomijärvi, D. Nosek, E. Santos, J. Pallotta, J. R. T. de Mello Neto, A. Weindl, Peter L. Biermann, David Schmidt, Paolo Privitera, Hernan Wahlberg, Darko Veberič, A. Parra, M. Schimassek, C. Hojvat, Jan Ebr, Jacco Vink, H.O. Klages, M. Trini, A. A. Nucita, J. Kleinfeller, Carlos Escobar, Kevin-Druis Merenda, A.D. Supanitsky, P.G. Brichetto Orchera, I. Allekotte, A. C. Fauth, Carla Bonifazi, Jose A. Bellido, Fabio Convenga, I.D. Vergara Quispe, J. Stasielak, K.-H. Becker, M. Pimenta, Denise Boncioli, P.R. Araújo Ferreira, Tobias Winchen, Florian Lukas Briechle, A. Aab, K. H. Kampert, J. C. Arteaga Velázquez, J. Perez Armand, Carla Taricco, C. Trimarelli, Matias Tueros, Claudio Galelli, B. García, R. López, Karen S. Caballero-Mora, Luis A. Nunez, Marcus Niechciol, Martin Erdmann, J. de Jesús, A. Streich, Gioacchino Alex Anastasi, M. Wirtz, Roger W Clay, S. Querchfeld, Olena Tkachenko, J. Šupík, Carlo Ventura, Ladislav Chytka, J. Hulsman, R. Squartini, Alfred Müller, G. Medina-Tanco, M. Zavrtanik, E. De Vito, Giovanni Consolati, C. J. Todero Peixoto, Petr Schovanek, Denis Stanca, H. Wilczyński, Ralf Ulrich, L. Nožka, Physics, Aab, A., Abreu, P., Aglietta, M., Albury, J. M., Allekotte, I., Almela, A., Alvarez-Muniz, J., Batista, R. A., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Ferreira, P. R. A., Velazquez, J. C. A., Asorey, H., Assis, P., Avila, G., Badescu, A. M., Bakalova, A., Balaceanu, A., Barbato, F., Luz, R. J. B., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Bister, T., Biteau, J., Blazek, J., Bleve, C., Bohacova, M., Boncioli, D., Bonifazi, C., Arbeletche, L. B., Borodai, N., Botti, A. M., Brack, J., Bretz, T., Orchera, P. G. B., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero-Mora, K. S., Caccianiga, L., Canfora, F., Caracas, I., Carceller, J. M., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Cerda, M., Chinellato, J. A., Choi, K., Chudoba, J., Chytka, L., Clay, R. W., Cerutti, A. C. C., Colalillo, R., Coleman, A., Coluccia, M. R., Conceicao, R., Condorelli, A., Consolati, G., Contreras, F., Convenga, F., dos Santos, D. C., Covault, C. E., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., de Almeida, R. M., de Jesus, J., de Jong, S. J., de Mauro, G., de Mello Neto, J. R. T., de Mitri, I., de Oliveira, J., de Oliveira Franco, D., de Palma, F., de Souza, V., de Vito, E., del Rio, M., Deligny, O., Di Matteo, A., Dobrigkeit, C., D'Olivo, J. C., dos Anjos, R. C., Dova, M. T., Ebr, J., Engel, R., Epicoco, I., Erdmann, M., Escobar, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Fick, B., Figueira, J. M., Filipcic, A., Fodran, T., Freire, M. M., Fujii, T., Fuster, A., Galea, C., Galelli, C., Garcia, B., Vegas, A. L. G., Gemmeke, H., Gesualdi, F., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., Glombitza, J., Gobbi, F., Gollan, F., Golup, G., Berisso, M. G., Vitale, P. F. G., Gongora, J. P., Gonzalez, J. M., Gonzalez, N., Goos, I., Gora, D., Gorgi, A., Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Hahn, S., Hamal, P., Hampel, M. R., Hansen, P., Harari, D., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Hill, G. C., Hojvat, C., Horandel, J. R., Horvath, P., Hrabovsky, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Janecek, P., Johnsen, J. A., Jurysek, J., Kaapa, A., Kampert, K. H., Keilhauer, B., Kemp, J., Klages, H. O., Kleifges, M., Kleinfeller, J., Kopke, M., Kunka, N., Lago, B. L., Lang, R. G., Langner, N., de Oliveira, M. A. L., Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Lo Presti, D., Lopes, L., Lopez, R., Lu, L., Luce, Q., Lucero, A., Lundquist, J. P., Payeras, A. M., Mancarella, G., Mandat, D., Manning, B. C., Manshanden, J., Mantsch, P., Marafico, S., Mariazzi, A. G., Maris, I. C., Marsella, G., Martello, D., Martinez, H., Bravo, O. M., Mastrodicasa, M., Mathes, H. J., Matthews, J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina-Tanco, G., Melo, D., Menshikov, A., Merenda, K. -D., Michal, S., Micheletti, M. I., Miramonti, L., Mollerach, S., Montanet, F., Morello, C., Mostafa, M., Muller, A. L., Muller, M. A., Mulrey, K., Mussa, R., Muzio, M., Namasaka, W. M., Nasr-Esfahani, A., Nellen, L., Niculescu-Oglinzanu, M., Niechciol, M., Nitz, D., Nosek, D., Novotny, V., Nozka, L., Nucita, A., Nunez, L. A., Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Pech, M., Pedreira, F., Pekala, J., Pelayo, R., Pena-Rodriguez, J., Martins, E. E. P., Armand, J. P., Bertolli, C. P., Perlin, M., Perrone, L., Petrera, S., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Pont, B., Pothast, M., Privitera, P., Prouza, M., Puyleart, A., Querchfeld, S., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Rizi, V., de Carvalho, W. R., Rojo, J. R., Roncoroni, M. J., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Salina, G., Gomez, J. D. S., Sanchez, F., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Savina, P., Schafer, C. M., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schluter, F., Schmidt, D., Scholten, O., Schovanek, P., Schroder, F. G., Schroder, S., Schulte, J., Sciutto, S. J., Scornavacche, M., Segreto, A., Sehgal, S., Shellard, R. C., Sigl, G., Silli, G., Sima, O., Smida, R., Sommers, P., Soriano, J. F., Souchard, J., Squartini, R., Stadelmaier, M., Stanca, D., Stanic, S., Stasielak, J., Stassi, P., Streich, A., Suarez-Duran, M., Sudholz, T., Suomijarvi, T., Supanitsky, A. D., Supik, J., Szadkowski, Z., Taboada, A., Tapia, A., Taricco, C., Timmermans, C., Tkachenko, O., Tobiska, P., Peixoto, C. J. T., Tome, B., Travaini, A., Travnicek, P., Trimarelli, C., Trini, M., Tueros, M., Ulrich, R., Unger, M., Vaclavek, L., Vacula, M., Galicia, J. F. V., Valore, L., Varela, E., Varma, V., Vasquez-Ramirez, A., Veberic, D., Ventura, C., Quispe, I. D. V., Verzi, V., Vicha, J., Vink, J., Vorobiov, S., Wahlberg, H., Watanabe, C., Watson, A. A., Weber, M., Weindl, A., Wiencke, L., Wilczynski, H., Winchen, T., Wirtz, M., Wittkowski, D., Wundheiler, B., Yushkov, A., Zapparrata, O., Zas, E., Zavrtanik, D., Zavrtanik, M., Zehrer, L., Zepeda, A., Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Pierre Auger, Research unit Astroparticle Physics, Alvarez-Mu??iz, J., Alves Batista, R., Ara??jo Ferreira, P. R., Arteaga Vel??zquez, J. C., Barreira Luz, R. J., Boh????ov??, M., Bonneau Arbeletche, L., Brichetto Orchera, P. G., Cobos Cerutti, A. C., Concei????o, R., Correia dos Santos, D., de Jes??s, J., De Mauro, G., De Mitri, I., De Vito, E., del R??o, M., Filip??i??, A., Garc??a, B., Garcia Vegas, A. L., G??mez Berisso, M., G??mez Vitale, P. F., Gonz??lez, J. M., Gonz??lez, N., G??ra, D., H??randel, J. R., Hrabovsk??, M., K????p??, A., K??pke, M., Leigui de Oliveira, M. A., L??pez, R., Machado Payeras, A., Mari??, I. C., Mart??nez Bravo, O., Mostaf??, M., M??ller, A. L., No??ka, L., N????ez, L. A., P??kala, J., Pe??a-Rodriguez, J., Pereira Martins, E. E., Perez Armand, J., P??rez Bertolli, C., Rodrigues de Carvalho, W., Rodriguez Rojo, J., Sanabria Gomez, J. D., S??nchez, F., Sch??fer, C. M., Schl??ter, F., Schov??nek, P., Schr??der, F. G., Schr??der, S., m??da, R., Stani??, S., Su??rez-Dur??n, M., Suomij??rvi, T., up??k, J., Todero Peixoto, C. J., Tom??, B., Vald??s Galicia, J. F., Varma K. C., V., V??squez-Ram??rez, A., Veberi??, D., Vergara Quispe, I. D., Wilczy??ski, H., High Energy Astrophys. & Astropart. Phys (API, FNWI), Aab A., Abreu P., Aglietta M., Albury J.M., Allekotte I., Almela A., Alvarez-Muniz J., Batista R.A., Anastasi G.A., Anchordoqui L., Andrada B., Andringa S., Aramo C., Ferreira P.R.A., Velazquez J.C.A., Asorey H., Assis P., Avila G., Badescu A.M., Bakalova A., Balaceanu A., Barbato F., Luz R.J.B., Becker K.H., Bellido J.A., Berat C., Bertaina M.E., Bertou X., Biermann P.L., Bister T., Biteau J., Blazek J., Bleve C., Bohacova M., Boncioli D., Bonifazi C., Arbeletche L.B., Borodai N., Botti A.M., Brack J., Bretz T., Orchera P.G.B., Briechle F.L., Buchholz P., Bueno A., Buitink S., Buscemi M., Caballero-Mora K.S., Caccianiga L., Canfora F., Caracas I., Carceller J.M., Caruso R., Castellina A., Catalani F., Cataldi G., Cazon L., Cerda M., Chinellato J.A., Choi K., Chudoba J., Chytka L., Clay R.W., Cerutti A.C.C., Colalillo R., Coleman A., Coluccia M.R., Conceicao R., Condorelli A., Consolati G., Contreras F., Convenga F., dos Santos D.C., Covault C.E., Dasso S., Daumiller K., Dawson B.R., Day J.A., de Almeida R.M., de Jesus J., de Jong S.J., de Mauro G., de Mello Neto J.R.T., de Mitri I., de Oliveira J., de Oliveira Franco D., de Palma F., de Souza V., de Vito E., del Rio M., Deligny O., Di Matteo A., Dobrigkeit C., D'Olivo J.C., dos Anjos R.C., Dova M.T., Ebr J., Engel R., Epicoco I., Erdmann M., Escobar C.O., Etchegoyen A., Falcke H., Farmer J., Farrar G., Fauth A.C., Fazzini N., Feldbusch F., Fenu F., Fick B., Figueira J.M., Filipcic A., Fodran T., Freire M.M., Fujii T., Fuster A., Galea C., Galelli C., Garcia B., Vegas A.L.G., Gemmeke H., Gesualdi F., Gherghel-Lascu A., Ghia P.L., Giaccari U., Giammarchi M., Giller M., Glombitza J., Gobbi F., Gollan F., Golup G., Berisso M.G., Vitale P.F.G., Gongora J.P., Gonzalez J.M., Gonzalez N., Goos I., Gora D., Gorgi A., Gottowik M., Grubb T.D., Guarino F., Guedes G.P., Guido E., Hahn S., Hamal P., Hampel M.R., Hansen P., Harari D., Harvey V.M., Haungs A., Hebbeker T., Heck D., Hill G.C., Hojvat C., Horandel J.R., Horvath P., Hrabovsky M., Huege T., Hulsman J., Insolia A., Isar P.G., Janecek P., Johnsen J.A., Jurysek J., Kaapa A., Kampert K.H., Keilhauer B., Kemp J., Klages H.O., Kleifges M., Kleinfeller J., Kopke M., Kunka N., Lago B.L., Lang R.G., Langner N., de Oliveira M.A.L., Lenok V., Letessier-Selvon A., Lhenry-Yvon I., Lo Presti D., Lopes L., Lopez R., Lu L., Luce Q., Lucero A., Lundquist J.P., Payeras A.M., Mancarella G., Mandat D., Manning B.C., Manshanden J., Mantsch P., Marafico S., Mariazzi A.G., Maris I.C., Marsella G., Martello D., Martinez H., Bravo O.M., Mastrodicasa M., Mathes H.J., Matthews J., Matthiae G., Mayotte E., Mazur P.O., Medina-Tanco G., Melo D., Menshikov A., Merenda K.-D., Michal S., Micheletti M.I., Miramonti L., Mollerach S., Montanet F., Morello C., Mostafa M., Muller A.L., Muller M.A., Mulrey K., Mussa R., Muzio M., Namasaka W.M., Nasr-Esfahani A., Nellen L., Niculescu-Oglinzanu M., Niechciol M., Nitz D., Nosek D., Novotny V., Nozka L., Nucita A., Nunez L.A., Palatka M., Pallotta J., Papenbreer P., Parente G., Parra A., Pech M., Pedreira F., Pekala J., Pelayo R., Pena-Rodriguez J., Martins E.E.P., Armand J.P., Bertolli C.P., Perlin M., Perrone L., Petrera S., Pierog T., Pimenta M., Pirronello V., Platino M., Pont B., Pothast M., Privitera P., Prouza M., Puyleart A., Querchfeld S., Rautenberg J., Ravignani D., Reininghaus M., Ridky J., Riehn F., Risse M., Rizi V., de Carvalho W.R., Rojo J.R., Roncoroni M.J., Roth M., Roulet E., Rovero A.C., Ruehl P., Saffi S.J., Saftoiu A., Salamida F., Salazar H., Salina G., Gomez J.D.S., Sanchez F., Santos E.M., Santos E., Sarazin F., Sarmento R., Sarmiento-Cano C., Sato R., Savina P., Schafer C.M., Scherini V., Schieler H., Schimassek M., Schimp M., Schluter F., Schmidt D., Scholten O., Schovanek P., Schroder F.G., Schroder S., Schulte J., Sciutto S.J., Scornavacche M., Segreto A., Sehgal S., Shellard R.C., Sigl G., Silli G., Sima O., Smida R., Sommers P., Soriano J.F., Souchard J., Squartini R., Stadelmaier M., Stanca D., Stanic S., Stasielak J., Stassi P., Streich A., Suarez-Duran M., Sudholz T., Suomijarvi T., Supanitsky A.D., Supik J., Szadkowski Z., Taboada A., Tapia A., Taricco C., Timmermans C., Tkachenko O., Tobiska P., Peixoto C.J.T., Tome B., Travaini A., Travnicek P., Trimarelli C., Trini M., Tueros M., Ulrich R., Unger M., Vaclavek L., Vacula M., Galicia J.F.V., Valore L., Varela E., Varma V., Vasquez-Ramirez A., Veberic D., Ventura C., Quispe I.D.V., Verzi V., Vicha J., Vink J., Vorobiov S., Wahlberg H., Watanabe C., Watson A.A., Weber M., Weindl A., Wiencke L., Wilczynski H., Winchen T., Wirtz M., Wittkowski D., Wundheiler B., Yushkov A., Zapparrata O., Zas E., Zavrtanik D., Zavrtanik M., Zehrer L., and Zepeda A.

Subjects
Photon, Physics::Instrumentation and Detectors, Astronomy, Electron, 01 natural sciences, High Energy Physics - Experiment, Auger, High Energy Physics - Experiment (hep-ex), mass [cosmic radiation], surface [detector], Observatory, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], photon: cosmic radiation, Instrumentation, Mathematical Physics, Physics, AGASA, Settore FIS/01 - Fisica Sperimentale, Detector, cosmic radiation [photon], Astrophysics::Instrumentation and Methods for Astrophysics, Monte Carlo [numerical calculations], electromagnetic [showers], observatory, cosmic radiation [electron], Analysis and statistical methods, numerical calculations: Monte Carlo, Analysis and statistical method, performance, positron: cosmic radiation, atmosphere [showers], Cherenkov detector, data analysis method, Calibration and fitting methods, Cherenkov detectors, Cluster finding, Large detector systems for particle and astroparticle physics, Pattern recognition, Cherenkov counter: water, air, neural network, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, cosmic radiation [positron], cosmic radiation: mass, Calibration and fitting method, Nuclear physics, statistical analysis, 0103 physical sciences, showers: electromagnetic, ddc:530, ddc:610, High Energy Physics, 010306 general physics, Zenith, Pierre Auger Observatory, cosmic radiation [muon], Muon, showers: atmosphere, 010308 nuclear & particles physics, detector: surface, hep-ex, water [Cherenkov counter], electron: cosmic radiation, Recurrent neural network, muon: cosmic radiation, Large detector systems for particle and astroparticle physic, Experimental High Energy Physics, High Energy Physics::Experiment, RAIOS CÓSMICOS, experimental results
Abstract

The Pierre Auger Observatory, at present the largest cosmic-ray observatory ever built, is instrumented with a ground array of 1600 water-Cherenkov detectors, known as the Surface Detector (SD). The SD samples the secondary particle content (mostly photons, electrons, positrons and muons) of extensive air showers initiated by cosmic rays with energies ranging from $10^{17}~$eV up to more than $10^{20}~$eV. Measuring the independent contribution of the muon component to the total registered signal is crucial to enhance the capability of the Observatory to estimate the mass of the cosmic rays on an event-by-event basis. However, with the current design of the SD, it is difficult to straightforwardly separate the contributions of muons to the SD time traces from those of photons, electrons and positrons. In this paper, we present a method aimed at extracting the muon component of the time traces registered with each individual detector of the SD using Recurrent Neural Networks. We derive the performances of the method by training the neural network on simulations, in which the muon and the electromagnetic components of the traces are known. We conclude this work showing the performance of this method on experimental data of the Pierre Auger Observatory. We find that our predictions agree with the parameterizations obtained by the AGASA collaboration to describe the lateral distributions of the electromagnetic and muonic components of extensive air showers., Comment: Published version, 23 pages, 15 figures

Published
2022

13. FACT - Highlights from more than Eight Years of Unbiased TeV Monitoring

Author

Adelina Kalenski, Aleksander Paravac, Thomas Bretz, Matteo Balbo, Adrian Biland, Bernd Schleicher, Dominik Elsaesser, Roland Walter, Alison Mitchell, Daniela Dorner, Dorothee Hildebrand, Laura Eisenberger, Karl Mannheim, Jens Buss, Wolfgang Rhode, Dominik Baack, Roman Iotov, Maximilian Noethe, Axel Arbet-Engels, Dominik Neise, and Vitalii Sliusar

Subjects
Telescope, Duty cycle, law, Spectral density, Astronomy, Context (language use), MAGIC (telescope), Blazar, Light curve, Cherenkov radiation, law.invention
Abstract

The First G-APD Cherenkov Telescope (FACT) has been monitoring blazars at TeV energies for more than eight years. Using solid state photo sensors and performing robotic operations results in a maximized duty cycle of the instrument and minimized observational gaps, providing an unprecedented data sample of more than 14700~hours of physics data. With an unbiased observing strategy, a small sample of sources is monitored. Results of an automatic quick-look analysis are published with low latency on an open-access website. Since 2014, close to 150 alerts including 11 astronomer's telegrams have been issued triggering target-of-opportunity observations and a variety of multi-wavelength studies. In 2016, FACT alerted MAGIC to a high state of 1ES 2344+51.4. The combined observations revealed a renewed extreme behaviour of the source. Thanks to target-of-opportunity observations and preplanned campaigns, several rich datasets with combined observations with INTEGRAL, XMM-Newton and AstroSAT are available for Mrk 421. Furthermore, dedicated campaigns each observing season provide multi-wavelength light curves and spectral energy distributions for the brightest blazars. The unprecedented, unbiased TeV data sample also provides the unique chance to study the duty cycle and the long-term spectral and temporal behaviour of the sources, including the search for periodic signals. Studying the long-term variability of Mrk 421 and Mrk 501 in the multi-wavelength context, correlations of different wavelengths are investigated searching for delays. In this presentation, selected highlights from more than eights years of monitoring will be summarized, including results from deep multi-instrument campaigns and long-term studies., PoS: Proceedings of Science, 395, ISSN:1824-8039, 37th International Cosmic Ray Conference (ICRC 2021)

Published
2022
Full Text
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14. Investigation of the correlation patterns and the Compton dominance variability of Mrk 421 in 2017

Author

Katsuaki Asano, I. Jiménez, A. Fuentes, C. M. Raiteri, D. Dominis Prester, E. Molina, E. Colombo, Y. V. Troitskaya, Nikola Godinovic, Sidika Merve Colak, Jenni Jormanainen, Yuki Iwamura, Alessandra Lamastra, Lab Saha, Antoniya Valcheva, Sunay Ibryamov, Elena G. Larionova, B. De Lotto, Evgeni Ovcharov, D. Zarić, Kazuma Ishio, David A. Green, M. Villata, D. Horan, Givi N. Kimeridze, Alexander Hahn, S. Nozaki, M. Perri, Michael D. Joner, D. Neise, S. Loporchio, R. J. García López, Marcello Giroletti, Victor A. Acciari, V. Fallah Ramazani, Tomohiko Oka, Daniela Dorner, Narek Sahakyan, J. Kushida, M. Kopp, Lorenzo Bellizzi, Noah Biederbeck, Joseph Moody, M. Gaug, L. Schneider, A. López-Oramas, Daniel Morcuende, N. Rizzi, Jose Luis Contreras, G. Vanzo, Rodolfo Carosi, L. Maraschi, Andrés Baquero, M. I. Carnerero, R. Iotov, Mosè Mariotti, A. Paravac, John Hoang, Ashwani Pandey, Z. R. Weaver, Francesco Longo, F. D'Ammando, S. Paiano, Elina Lindfors, Moritz Hütten, J. Herrera, Koji Noda, Abelardo Moralejo, Laura Eisenberger, E. Moretti, Julian Sitarek, Marcos López-Moya, Wlodek Bednarek, L. Di Venere, Ashot Chilingarian, U. Barres de Almeida, Elisa Bernardini, I. Agudo, M. Feige, R. Z. Ivanidze, O. A. Merkulova, D. Depaoli, M. Spencer, Massimo Persic, J. van Scherpenberg, Pratik Majumdar, L. Kunkel, K. Nishijima, Stefano Ansoldi, Juan Cortina, Kai Phillip Schmidt, A. Berti, Riccardo Paoletti, Saverio Lombardi, Daniel Mazin, M. V. Fonseca, Damir Lelas, R. J. C. Vera, Sanae Inoue, Giacomo D'Amico, Dominik Baack, C. Perennes, A. A. Nikiforova, Yating Chai, Stefan Cikota, G. M. Madejski, A. Arbet Engels, Daniel Kerszberg, Manuel Artero, E. Do Souto Espiñeira, Tomislav Terzić, J. Becerra González, Martin Makariev, R. Mirzoyan, Yoshiki Ohtani, G. A. Borman, Pawel Gliwny, Jose Miguel Miranda, A. De Angelis, Vitaly Neustroev, Wara Chamani, Oscar Blanch, T. S. Grishina, Martin Will, M. Vazquez Acosta, Nicola Giglietto, L. V. Larionova, Lea Heckmann, Francesco Gabriele Saturni, Jorge Otero-Santos, R. A. Chigladze, M. Balbo, N. Marchili, D. Hadasch, P. G. Prada Moroni, A. A. Vasilyev, M. G. Nikolashvili, Jordi Delgado, V. Ramakrishnan, Christian Fruck, G. Busetto, Victoria Moreno, Luca Tosti, A. Rugliancich, C. Nigro, Marina Manganaro, Valeri M. Larionov, M. Balokovic, Manuel Delfino, A. Strigachev, J. M. Paredes, Manash R. Samal, Stefano Covino, I. Vovk, H. C. Lin, Ž. Bošnjak, Stefano Menchiari, Rumen Bachev, Marc Ribó, Dorota Sobczyńska, Carolin Wunderlich, Bernd Schleicher, M. Minev, Antonio Stamerra, Maria-Isabel Bernardos, I. S. Troitskiy, Merja Tornikoski, E. N. Kopatskaya, Shunsuke Sakurai, Camilla Maggio, Chiara Righi, F. Verrecchia, P. Temnikov, S. G. Jorstad, T. Schweizer, Hidetoshi Kubo, Lluis Font, A. Y. Lien, Toshiaki Inada, A. Scherbantin, Lorand A. Sigua, G. Maneva, Stefano Truzzi, B. Machado de Oliveira Fraga, V. Bozhilov, M. Palatiello, Alessandro Marchini, Chaitanya Priyadarshi, Alessia Spolon, Léa Jouvin, Konstancja Satalecka, Tomoki Saito, Giovanni Ceribella, Michele Doro, S. O. Kurtanidze, Carlo Vigorito, Pablo Peñil, D. Strom, Giacomo Bonnoli, Adrian Biland, Ana Babić, Alicia Fattorini, D. Hildebrand, Satoshi Fukami, G. Ferrara, Y. Kajiwara, Matteo Cerruti, P. Da Vela, Vassil Verguilov, Lovro Pavletić, C. Delgado Mendez, Emilia Järvelä, S. Mićanović, Sergey S. Savchenko, Ivica Puljak, M. Noethe, Simone Mender, Francesco Dazzi, V. Vitale, Manuela Mallamaci, Ivana Batković, F. Leone, M. I. Martínez, J. Rico, Alan P. Marscher, C. Lorey, S. Ventura, Tjark Miener, Anne Lähteenmäki, David Paneque, Masahiro Teshima, Jarred Gershon Green, Wrijupan Bhattacharyya, Kari Nilsson, R. Walter, M. Strzys, D. Reinhart, E. Zaharieva, Wen Ping Chen, Vitalii Sliusar, Jürgen Besenrieder, Francesco Giordano, Antonio Tutone, Thomas Bretz, J. Buss, Alok C. Gupta, Simona Righini, O. M. Kurtanidze, Ciro Bigongiari, O. Vince, D. Elsaesser, C. Leto, M. Garczarczyk, Sargis Gasparyan, J. Kania, Dario Hrupec, R. López-Coto, Wolfgang Rhode, I. Snidaric, D. A. Morozova, Vladimir A. Hagen-Thorn, Mitsunari Takahashi, J. A. Acosta-Pulido, E. Prandini, Marie Karjalainen, D. Miceli, Goran Damljanović, Evgeni Semkov, Alice Donini, L. A. Antonelli, J. A. Barrio, Y. Suda, D. Carosati, V. D'Elia, Fabrizio Tavecchio, A. C. Sadun, Tihomir Surić, C. Casadio, Karl Mannheim, Santiago Ubach, Y. Kobayashi, F. Di Pierro, European Commission, European Research Council, Ministerio de Ciencia e Innovación (España), Generalitat de Catalunya, Federal Ministry of Education and Research (Germany), German Research Foundation, Swiss National Science Foundation, Croatian Science Foundation, Ministry of Education, Science and Technological Development (Serbia), Bulgarian National Science Fund, National Aeronautics and Space Administration (US), Acciari, V. A., Ansoldi, S., Antonelli, L. A., Arbet Engels, A., Artero, M., Asano, K., Babi??, A., Baquero, A., Barres de Almeida, U., Barrio, J. A., Batkovi??, I., Becerra Gonz??lez, J., Bednarek, W., Bellizzi, L., Bernardini, E., Bernardos, M., Berti, A., Besenrieder, J., Bhattacharyya, W., Bigongiari, C., Blanch, O., Bo??njak, ??., Busetto, G., Carosi, R., Ceribella, G., Cerruti, M., Chai, Y., Chilingarian, A., Cikota, S., Colak, S. M., Colombo, E., Contreras, J. L., Cortina, J., Covino, S., D???amico, G., D???elia, V., Da Vela, P., Dazzi, F., De Angelis, A., De Lotto, B., Delfino, M., Delgado, J., Delgado Mendez, C., Depaoli, D., Di Pierro, F., Di Venere, L., Do Souto Espi??eira, E., Dominis Prester, D., Donini, A., Doro, M., Fallah Ramazani, V., Fattorini, A., Ferrara, G., Fonseca, M. V., Font, L., Fruck, C., Fukami, S., Garc??a L??pez, R. J., Garczarczyk, M., Gasparyan, S., Gaug, M., Giglietto, N., Giordano, F., Gliwny, P., Godinovi??, N., Green, J. G., Green, D., Hadasch, D., Hahn, A., Heckmann, L., Herrera, J., Hoang, J., Hrupec, D., H??tten, M., Inada, T., Inoue, S., Ishio, K., Iwamura, Y., Jim??nez, I., Jormanainen, J., Jouvin, L., Kajiwara, Y., Karjalainen, M., Kerszberg, D., Kobayashi, Y., Kubo, H., Kushida, J., Lamastra, A., Lelas, D., Leone, F., Lindfors, E., Lombardi, S., Longo, F., L??pez-Coto, R., L??pez-Moya, M., L??pez-Oramas, A., Loporchio, S., Machado de Oliveira Fraga, B., Maggio, C., Majumdar, P., Makariev, M., Mallamaci, M., Maneva, G., Manganaro, M., Maraschi, L., Mariotti, M., Mart??nez, M., Mazin, D., Menchiari, S., Mender, S., Mi??anovi??, S., Miceli, D., Miener, T., Minev, M., Miranda, J. M., Mirzoyan, R., Molina, E., Moralejo, A., Morcuende, D., Moreno, V., Moretti, E., Neustroev, V., Nigro, C., Nilsson, K., Nishijima, K., Noda, K., Nozaki, S., Ohtani, Y., Oka, T., Otero-Santos, J., Paiano, S., Palatiello, M., Paneque, D., Paoletti, R., Paredes, J. M., Pavleti??, L., Pe??il, P., Perennes, C., Persic, M., Prada Moroni, P. G., Prandini, E., Priyadarshi, C., Puljak, I., Rib??, M., Rico, J., Righi, C., Rugliancich, A., Saha, L., Sahakyan, N., Saito, T., Sakurai, S., Satalecka, K., Saturni, F. G., Schmidt, K., Schweizer, T., Sitarek, J., nidari??, I., Sobczynska, D., Spolon, A., Stamerra, A., Strom, D., Strzys, M., Suda, Y., Suri??, T., Takahashi, M., Tavecchio, F., Temnikov, P., Terzi??, T., Teshima, M., Tosti, L., Truzzi, S., Tutone, A., Ubach, S., van Scherpenberg, J., Vanzo, G., Vazquez Acosta, M., Ventura, S., Verguilov, V., Vigorito, C. F., Vitale, V., Vovk, I., Will, M., Wunderlich, C., Zari??, D., Baack, D., Balbo, M., Biederbeck, N., Biland, A., Bretz, T., Buss, J., Dorner, D., Eisenberger, L., Elsaesser, D., Hildebrand, D., Iotov, R., Mannheim, K., Neise, D., Noethe, M., Paravac, A., Rhode, W., Schleicher, B., Sliusar, V., Walter, R., D???ammando, F., Horan, D., Lien, A. Y., Balokovi??, M., Madejski, G. M., Perri, M., Verrecchia, F., Leto, C., L??hteenm??ki, A., Tornikoski, M., Ramakrishnan, V., J??rvel??, E., Vera, R. J. C., Chamani, W., Villata, M., Raiteri, C. M., Gupta, A. C., Pandey, A., Fuentes, A., Agudo, I., Casadio, C., Semkov, E., Ibryamov, S., Marchini, A., Bachev, R., Strigachev, A., Ovcharov, E., Bozhilov, V., Valcheva, A., Zaharieva, E., Damljanovic, G., Vince, O., Larionov, V. M., Borman, G. A., Grishina, T. S., Hagen-Thorn, V. A., Kopatskaya, E. N., Larionova, E. G., Larionova, L. V., Morozova, D. A., Nikiforova, A. A., Savchenko, S. S., Troitskiy, I. S., Troitskaya, Y. V., Vasilyev, A. A., Merkulova, O. A., Chen, W. P., Samal, M., Lin, H. C., Moody, J. W., Sadun, A. C., Jorstad, S. G., Marscher, A. P., Weaver, Z. R., Feige, M., Kania, J., Kopp, M., Kunkel, L., Reinhart, D., Scherbantin, A., Schneider, L., Lorey, C., Acosta-Pulido, J. A., Carnerero, M. I., Carosati, D., Kurtanidze, S. O., Kurtanidze, O. M., Nikolashvili, M. G., Chigladze, R. A., Ivanidze, R. Z., Kimeridze, G. N., Sigua, L. A., Joner, M. D., Spencer, M., Giroletti, M., Marchili, N., Righini, S., Rizzi, N., Bonnoli, G., Laboratoire Leprince-Ringuet (LLR), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), MAGIC, FACT, Department of Electronics and Nanoengineering, Aalto-yliopisto, and Aalto University

Subjects
electron, PARTICLE-ACCELERATION, ELECTRON ACCELERATION, Radiation mechanisms: non-thermal, RAY, VHE [gamma ray], galaxies: active, BL Lacertae objects: individual: Mrk 421, radiation mechanisms: non-thermal, Electron, Astrophysics, GeV, 01 natural sciences, 7. Clean energy, LARGE-AREA TELESCOPE, law.invention, OBSERVATIONS, law, ultraviolet, optical, MAGIC (telescope), correlation [flux], 010303 astronomy & astrophysics, X-ray: flux, model: leptonic, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), BL-LACERTAE, individual: Mrk 421 [BL Lacertae objects], flux [X-ray], Gamma ray, flux: correlation, Galaxies: active, non-thermal [radiation mechanisms], Synchrotron, SWIFT OBSERVATIONS, active [galaxies], Spectral energy distribution, Física nuclear, Astrophysics - High Energy Astrophysical Phenomena, Lorentz, Flare, LOG-PARABOLIC SPECTRA, ACTIVE GALACTIC NUCLEI, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, radiation, mechanisms: non-thermal, LIGHT CURVES, X-RAY, MULTIWAVELENGTH, GLAST, leptonic [model], blazar, 0103 physical sciences, TeV, Blazar, 010308 nuclear & particles physics, Astronomy and Astrophysics, MAGIC, gamma ray: VHE, Space and Planetary Science, ddc:520, spectral, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Fermi Gamma-ray Space Telescope
Abstract

Full list of authors: Acciari, V. A.; Ansoldi, S.; Antonelli, L. A.; Arbet Engels, A.; Artero, M.; Asano, K.; Babić, A.; Baquero, A.; Barres de Almeida, U.; Barrio, J. A.; Batković, I.; Becerra González, J.; Bednarek, W.; Bellizzi, L.; Bernardini, E.; Bernardos, M.; Berti, A.; Besenrieder, J.; Bhattacharyya, W.; Bigongiari, C.; Blanch, O.; Bošnjak, Ž.; Busetto, G.; Carosi, R.; Ceribella, G.; Cerruti, M.; Chai, Y.; Chilingarian, A.; Cikota, S.; Colak, S. M.; Colombo, E.; Contreras, J. L.; Cortina, J.; Covino, S.; D'Amico, G.; D'Elia, V.; da Vela, P.; Dazzi, F.; de Angelis, A.; de Lotto, B.; Delfino, M.; Delgado, J.; Delgado Mendez, C.; Depaoli, D.; di Pierro, F.; di Venere, L.; Do Souto Espiñeira, E.; Dominis Prester, D.; Donini, A.; Doro, M.; Fallah Ramazani, V.; Fattorini, A.; Ferrara, G.; Fonseca, M. V.; Font, L.; Fruck, C.; Fukami, S.; García López, R. J.; Garczarczyk, M.; Gasparyan, S.; Gaug, M.; Giglietto, N.; Giordano, F.; Gliwny, P.; Godinović, N.; Green, J. G.; Green, D.; Hadasch, D.; Hahn, A.; Heckmann, L.; Herrera, J.; Hoang, J.; Hrupec, D.; Hütten, M.; Inada, T.; Inoue, S.; Ishio, K.; Iwamura, Y.; Jiménez, I.; Jormanainen, J.; Jouvin, L.; Kajiwara, Y.; Karjalainen, M.; Kerszberg, D.; Kobayashi, Y.; Kubo, H.; Kushida, J.; Lamastra, A.; Lelas, D.; Leone, F.; Lindfors, E.; Lombardi, S.; Longo, F.; López-Coto, R.; López-Moya, M.; López-Oramas, A.; Loporchio, S.; Machado de Oliveira Fraga, B.; Maggio, C.; Majumdar, P.; Makariev, M.; Mallamaci, M.; Maneva, G.; Manganaro, M.; Maraschi, L.; Mariotti, M.; Martínez, M.; Mazin, D.; Menchiari, S.; Mender, S.; Mićanović, S.; Miceli, D.; Miener, T.; Minev, M.; Miranda, J. M.; Mirzoyan, R.; Molina, E.; Moralejo, A.; Morcuende, D.; Moreno, V.; Moretti, E.; Neustroev, V.; Nigro, C.; Nilsson, K.; Nishijima, K.; Noda, K.; Nozaki, S.; Ohtani, Y.; Oka, T.; Otero-Santos, J.; Paiano, S.; Palatiello, M.; Paneque, D.; Paoletti, R.; Paredes, J. M.; Pavletić, L.; Peñil, P.; Perennes, C.; Persic, M.; Prada Moroni, P. G.; Prandini, E.; Priyadarshi, C.; Puljak, I.; Ribó, M.; Rico, J.; Righi, C.; Rugliancich, A.; Saha, L.; Sahakyan, N.; Saito, T.; Sakurai, S.; Satalecka, K.; Saturni, F. G.; Schmidt, K.; Schweizer, T.; Sitarek, J.; Šnidarić, I.; Sobczynska, D.; Spolon, A.; Stamerra, A.; Strom, D.; Strzys, M.; Suda, Y.; Surić, T.; Takahashi, M.; Tavecchio, F.; Temnikov, P.; Terzić, T.; Teshima, M.; Tosti, L.; Truzzi, S.; Tutone, A.; Ubach, S.; van Scherpenberg, J.; Vanzo, G.; Vazquez Acosta, M.; Ventura, S.; Verguilov, V.; Vigorito, C. F.; Vitale, V.; Vovk, I.; Will, M.; Wunderlich, C.; Zarić, D.; Baack, D.; Balbo, M.; Biederbeck, N.; Biland, A.; Bretz, T.; Buss, J.; Dorner, D.; Eisenberger, L.; Elsaesser, D.; Hildebrand, D.; Iotov, R.; Mannheim, K.; Neise, D.; Noethe, M.; Paravac, A.; Rhode, W.; Schleicher, B.; Sliusar, V.; Walter, R.; D'Ammando, F.; Horan, D.; Lien, A. Y.; Baloković, M.; Madejski, G. M.; Perri, M.; Verrecchia, F.; Leto, C.; Lähteenmäki, A.; Tornikoski, M.; Ramakrishnan, V.; Järvelä, E.; Vera, R. J. C.; Chamani, W.; Villata, M.; Raiteri, C. M.; Gupta, A. C.; Pandey, A.; Fuentes, A.; Agudo, I.; Casadio, C.; Semkov, E.; Ibryamov, S.; Marchini, A.; Bachev, R.; Strigachev, A.; Ovcharov, E.; Bozhilov, V.; Valcheva, A.; Zaharieva, E.; Damljanovic, G.; Vince, O.; Larionov, V. M.; Borman, G. A.; Grishina, T. S.; Hagen-Thorn, V. A.; Kopatskaya, E. N.; Larionova, E. G.; Larionova, L. V.; Morozova, D. A.; Nikiforova, A. A.; Savchenko, S. S.; Troitskiy, I. S.; Troitskaya, Y. V.; Vasilyev, A. A.; Merkulova, O. A.; Chen, W. P; Samal, M.; Lin, H. C.; Moody, J. W.; Sadun, A. C.; Jorstad, S. G.; Marscher, A. P.; Weaver, Z. R.; Feige, M.; Kania, J.; Kopp, M.; Kunkel, L.; Reinhart, D.; Scherbantin, A.; Schneider, L.; Lorey, C.; Acosta-Pulido, J. A.; Carnerero, M. I.; Carosati, D.; Kurtanidze, S. O.; Kurtanidze, O. M.; Nikolashvili, M. G.; Chigladze, R. A.; Ivanidze, R. Z.; Kimeridze, G. N.; Sigua, L. A.; Joner, M. D.; Spencer, M.; Giroletti, M.; Marchili, N.; Righini, S.; Rizzi, N.; Bonnoli, G.; MAGIC Collaboration; Fact Collaboration.-- This is an Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited., Aims. We present a detailed characterisation and theoretical interpretation of the broadband emission of the paradigmatic TeV blazar Mrk 421, with a special focus on the multi-band flux correlations. Methods. The dataset has been collected through an extensive multi-wavelength campaign organised between 2016 December and 2017 June. The instruments involved are MAGIC, FACT, Fermi-LAT, Swift, GASP-WEBT, OVRO, Medicina, and Metsahovi. Additionally, four deep exposures (several hours long) with simultaneous MAGIC and NuSTAR observations allowed a precise measurement of the falling segments of the two spectral components. Results. The very-high-energy (VHE; E 100 GeV) gamma rays and X-rays are positively correlated at zero time lag, but the strength and characteristics of the correlation change substantially across the various energy bands probed. The VHE versus X-ray fluxes follow dierent patterns, partly due to substantial changes in the Compton dominance for a few days without a simultaneous increase in the X-ray flux (i.e., orphan gamma-ray activity). Studying the broadband spectral energy distribution (SED) during the days including NuSTAR observations, we show that these changes can be explained within a one-zone leptonic model with a blob that increases its size over time. The peak frequency of the synchrotron bump varies by two orders of magnitude throughout the campaign. Our multi-band correlation study also hints at an anti-correlation between UV-optical and X-ray at a significance higher than 3. A VHE flare observed on MJD 57788 (2017 February 4) shows gamma-ray variability on multi-hour timescales, with a factor ten increase in the TeV flux but only a moderate increase in the keV flux. The related broadband SED is better described by a two-zone leptonic scenario rather than by a one-zone scenario.We find that the flare can be produced by the appearance of a compact second blob populated by high energetic electrons spanning a narrow range of Lorentz factors, from 0 min = 2104 to 0 max = 6105. © 2021 Georg Thieme Verlag. All rights reserved., The MAGIC Collaboration would like to thank the Instituto de Astrofísica de Canarias for the excellent working conditions at the Observatorio del Roque de los Muchachos in La Palma. The financial support of the German BMBF, MPG and HGF; the Italian INFN and INAF; the Swiss National Fund SNF; the ERDF under the Spanish Ministerio de Ciencia e Innovación (MICINN) (FPA2017-87859-P, FPA2017-85668-P, FPA2017-82729-C6-5-R, FPA2017-90566-REDC, PID2019-104114RB-C31, PID2019-104114RB-C32, PID2019-105510GB-C31,PID2019-107847RB-C41, PID2019-107847RB-C42, PID2019-107847RB-C44, PID2019-107988GB-C22); the Indian Department of Atomic Energy; the Japanese ICRR, the University of Tokyo, JSPS, and MEXT; the Bulgarian Ministry of Education and Science, National RI Roadmap Project DO1-268/16.12.2019 and the Academy of Finland grant nr. 320045 is gratefully acknowledged. This work was also supported by the Spanish Centro de Excelencia “Severo Ochoa” SEV-2016-0588, SEV-2017-0709 and CEX2019-000920-S, and “María de Maeztu” CEX2019-000918-M, the Unidad de Excelencia “María de Maeztu” MDM-2015-0509-18-2 and the “la Caixa” Foundation (fellowship LCF/BQ/PI18/11630012) and by the CERCA program of the Generalitat de Catalunya; by the Croatian Science Foundation (HrZZ) Project IP-2016-06-9782 and the University of Rijeka Project 13.12.1.3.02; by the DFG Collaborative Research Centers SFB823/C4 and SFB876/C3; the Polish National Research Centre grant UMO-2016/22/M/ST9/00382; and by the Brazilian MCTIC, CNPq and FAPERJ. The important contributions from ETH Zurich grants ETH-10.08-2 and ETH-27.12-1 as well as the funding by the Swiss SNF and the German BMBF (Verbundforschung Astro- und Astroteilchenphysik) and HAP (Helmoltz Alliance for Astroparticle Physics) are gratefully acknowledged. Part of this work is supported by Deutsche Forschungsgemeinschaft (DFG) within the Collaborative Research Center SFB 876 “Providing Information by Resource-Constrained Analysis”, project C3. We are thankful for the very valuable contributions from E. Lorenz, D. Renker and G. Viertel during the early phase of the project. We thank the Instituto de Astrofísica de Canarias for allowing us to operate the telescope at the Observatorio del Roque de los Muchachos in La Palma, the Max-Planck-Institut für Physik for providing us with the mount of the former HEGRA CT3 telescope, and the MAGIC collaboration for their support. The Fermi LAT Collaboration acknowledges generous ongoing support from a number of agencies and institutes that have supported both the development and the operation of the LAT as well as scientific data analysis. These include the National Aeronautics and Space Administration and the Department of Energy in the United States, the Commissariat à l’Energie Atomique and the Centre National de la Recherche Scientifique/Institut National de Physique Nucléaire et de Physique des Particules in France, the Agenzia Spaziale Italiana and the Istituto Nazionale di Fisica Nucleare in Italy, the Ministry of Education, Culture, Sports, Science and Technology (MEXT), High Energy Accelerator Research Organization (KEK) and Japan Aerospace Exploration Agency (JAXA) in Japan, and the K. A. Wallenberg Foundation, the Swedish Research Council and the Swedish National Space Board in Sweden. Additional support for science analysis during the operations phase is gratefully acknowledged from the Istituto Nazionale di Astrofisica in Italy and the Centre National d’Études Spatiales in France. This work performed in part under DOE Contract DE-AC02-76SF00515. This work made use of data from the NuSTAR mission, a project led by the California Institute of Technology, managed by the Jet Propulsion Laboratory, and funded by the National Aeronautics and Space Administration. We thank the NuSTAR Operations, Software, and Calibration teams for support with the execution and analysis of these observations. This research has made use of the NuSTAR Data Analysis Software (NuSTARDAS) jointly developed by the ASI Science Data Center (ASDC; Italy) and the California Institute of Technology (USA). This research has also made use of the XRT Data Analysis Software (XRTDAS) developed under the responsibility of the ASI Science Data Center (ASDC), Italy. A.A.E and D.P acknowledge support from the Deutsche Forschungs gemeinschaft (DFG, German Research Foundation) under Germany’s Excellence Strategy – EXC-2094 – 390783311. M. B. acknowledges support from the YCAA Prize Postdoctoral Fellowship and from the Black Hole Initiative at Harvard University, which is funded in part by the Gordon and Betty Moore Foundation (grant GBMF8273) and in part by the John Templeton Foundation. This publication makes use of data obtained at the Metsähovi Radio Observatory, operated by Aalto University in Finland. This research has made use of data from the OVRO 40-m monitoring program (Richards et al. 2011) which is supported in part by NASA grants NNX08AW31G, NNX11A043G, and NNX14AQ89G and NSF grants AST-0808050 and AST-1109911. I.A. acknowledges financial support from the Spanish “Ministerio de Ciencia e Innovación” (MCINN) through the “Center of Excellence Severo Ochoa” award for the Instituto de Astrofísica de Andalucía-CSIC (SEV-2017-0709). Acquisition and reduction of the MAPCAT data was supported in part by MICINN through grants AYA2016-80889-P and PID2019-107847RB-C44. The MAPCAT observations were carried out at the German-Spanish Calar Alto Observatory, which is jointly operated by Junta de Andalucía and Consejo Superior de Investigaciones Científicas. C.C. acknowledges support from the European Research Council (ERC) under the European Union Horizon 2020 research and innovation program under the grant agreement No 771282. This research was partially supported by the Bulgarian National Science Fund of the Ministry of Education and Science under grants KP-06-H28/3 (2018), KP-06-H38/4 (2019) and KP-06-KITAJ/2 (2020). We acknowledge support by Bulgarian National Science Fund under grant DN18-10/2017 and National RI Roadmap Projects DO1-277/16.12.2019 and DO1-268/16.12.2019 of the Ministry of Education and Science of the Republic of Bulgaria. This research was supported by the Ministry of Education, Science and Technological Development of the Republic of Serbia (contract No 451-03-68/2020-14/200002). G.D. acknowledges observing grant support from the Institute of Astronomy and Rozhen NAO BAS through the bilateral joint research project “Gaia Celestial Reference Frame (CRF) and fast variable astronomical objects” (2020–2022, head – G. Damljanovic). The BU group was supported in part by NASA Fermi guest investigator program grants 80NSSC19K1505 and 80NSSC20K1566. This study was based in part on observations conducted using the 1.8 m Perkins Telescope Observatory (PTO) in Arizona, which is owned and operated by Boston University. This article is partly based on observations made with the LCOGT Telescopes, one of whose nodes is located at the Observatorios de Canarias del IAC on the island of Tenerife in the Observatorio del Teide. This article is also based partly on data obtained with the STELLA robotic telescopes in Tenerife, an AIP facility jointly operated by AIP and IAC. The Abastumani team acknowledges financial support by the Shota Rustaveli National Science Foundation under contract FR-19-6174. Based on observations with the Medicina telescope operated by INAF – Istituto di Radioastronomia.

Published
2021

15. Simulations Performance of a 55 Imaging Air-Cherenkov Telescopes HAWC’s Eye at High Altitude

Author

Ruben Alfaro, Jan Audehm, Florian Rehbein, Miguel Martinez-Felipe, Maria Magdalena González, José Serna-Franco, Jesús Martínez-Castro, Arturo Iriarte, Francisco Javier Gonzalez, Y. Perez, Thomas Bretz, Merlin Schaufel, Frank Maslowski, Franziska Tischbein, Ibrahim Torres, Giang Do, and Oscar Chaparro-Amaro

Subjects
Environmental science, Effects of high altitude on humans, Cherenkov radiation, Remote sensing
Published
2021

16. Preliminary Cosmic Ray Results from the HAWC's Eye Telescopes

Author

Oscar Chaparro-Amaro, Francisco Javier Gonzalez, Yunior Frainen Perez-Araujo, Giang Do, Jesús Martínez-Castro, Arturo Iriarte, Frank Maslowski, Maria Magdalena González, José Serna-Franco, Florian Rehbein, Thomas Bretz, Ruben Alfaro, Jan Audehm, Merlin Schaufel, Ibrahim Torres, Miguel Martinez-Felipe, and Franziska Tischbein

Subjects
Physics, Astronomy, Cosmic ray
Published
2021

17. Multi-wavelength study of Mrk 421 during a TeV flare

Author

Daniela Dorner, Adrian Biland, Adelina Kalenski, Dominik Elsaesser, M. Noethe, Laura Eisenberger, Bernd Schleicher, A. Arbet-Engels, R. Iotov, Thomas Dauser, Dominik Baack, P. Thalhammer, V. Sliusar, A. Gokus, Alexander Kraus, M. Balbo, D. Hildebrand, Karl Mannheim, Florian Eppel, A. Paravac, J. Buss, J. Wilms, K. Leiter, D. Neise, Jonas Hessdoerfer, Michael Kreter, A. Kreikenbohm, M. Langejahn, I. Kreykenbohm, Matthias Kadler, R. Walter, Thomas Bretz, Wolfgang Rhode, and Alison Mitchell

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Flux, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Light curve, Monitoring program, law.invention, Telescope, Crab Nebula, law, Observatory, Astrophysics - High Energy Astrophysical Phenomena, Blazar, Flare
Abstract

The blazar Mrk 421 shows frequent, short flares in the TeV energy regime. Due to the fast nature of such episodes, we often fail to obtain sufficient simultaneous information about flux variations in several energy bands. To overcome this lack of multi-wavelength (MWL) coverage, especially for the pre- and post-flare periods, we have set up a monitoring program with the FACT telescope (TeV energies) and the Neil Gehrels Swift Observatory (X-rays). On 2019 June 9, Mrk 421 showed a TeV outburst reaching a flux level of more than two times the flux of the Crab Nebula at TeV energies. We acquired simultaneous data in the X-rays with additional observations by XMM-Newton and INTEGRAL. For the first time, we can study a TeV blazar in outburst taking advantage of highly sensitive X-ray data from XMM-Newton and INTEGRAL combined. Our dataset is complemented by pointed radio observations by Effelsberg at GHz frequencies. We present our first results, including the {\gamma}-ray and X-ray light curves, a timing analysis of the X-ray data obtained with XMM-Newton , as well as the radio spectra before, during and after the flare., Comment: 8 pages, 4 figures; Proceedings of the 37th International Cosmic Ray Conference (ICRC2021). 12-23 July, 2021. Berlin, Germany. Online at https://pos.sissa.it/395/

Published
2021

18. The FRAM robotic telescope for atmospheric monitoring at the Pierre Auger Observatory

Author

Jose Chinellato, Ioana Caracas, Lorenzo Cazon, C. Pérez Bertolli, Ioana Codrina Maris, Marina Scornavacche, R. Ulrich, G. C. Hill, Jorge F. Soriano, Ralph Engel, M. Risse, H. J. Mathes, J. Ridky, Xavier Bertou, G. Marsella, David Wittkowski, G. Salina, Olivier Deligny, M. Unger, Tomáš Fodran, Alina Nasr-Esfahani, Stanislav Michal, Jonathan Blazek, Ugo Giaccari, J. Kleinfeller, K. Choi, Julien Manshanden, Andres Travaini, E. Varela, J.D. Sanabria Gomez, K.-H. Becker, M. Pimenta, P.R. Araújo Ferreira, Tobias Winchen, Denis Stanca, Florian Lukas Briechle, F. Canfora, G. Farrar, Antonio Condorelli, Carla Bleve, Rodrigo Guedes Lang, G. De Mauro, Silvia Mollerach, N. Fazzini, Jonas Glombitza, F. C. T. Barbato, P. Abreu, D. Ravignani, Alena Bakalova, G. Matthiae, Jaime Alvarez-Muñiz, J. Rodriguez Rojo, Fridtjof Feldbusch, Enrique Zas, Marvin Gottowik, Carlos Escobar, Kevin-Druis Merenda, R.J. Barreira Luz, G. P. Guedes, G. Parente, L. Zehrer, A. Puyleart, Corinne Berat, M. Giller, Jörg R. Hörandel, Paul Sommers, P. Kubánek, Flavia Gesualdi, Fernando Contreras, Alexandru Gherghel-Lascu, Belén Andrada, P. Tobiska, Antonio Bueno, Violet M. Harvey, D. Harari, J. Chudoba, Valerio Pirronello, Gualberto Avila, B. García, Lukáš Vaclavek, Toshihiro Fujii, Dariusz Gora, Eric Mayotte, A. Zepeda, R. López, G. Mancarella, Pedro Assis, H. Martinez, A. Etchegoyen, Matías J. Roncoroni, Martina Bohacova, A. Aab, J. Biteau, I. Lhenry-Yvon, Karen S. Caballero-Mora, A.L. Garcia Vegas, B. Keilhauer, J. de Oliveira, A.D. Supanitsky, M. Gómez Berisso, Jakub Juryšek, Alejandro Almela, R. C. Shellard, S. J. Sciutto, A. Di Matteo, Alan Coleman, S. J. Saffi, B. Wundheiler, Marcel Köpke, Martin Erdmann, J. de Jesús, Juan Miguel Carceller, C. J. Todero Peixoto, Alina Mihaela Badescu, Cristina Galea, John Farmer, Serguei Vorobiov, M. Platino, Maria Rita Coluccia, Carla Taricco, M. Prouza, G. Cataldi, A. Streich, Gioacchino Alex Anastasi, D. Nitz, Juan Pablo Gongora, F. Pedreira, M. I. Micheletti, F. Salamida, M. Wirtz, Petr Hamal, B. L. Lago, P. Ruehl, Fred Sarazin, Thomas Bretz, A. Taboada, V. Scherini, A. Yushkov, Roger W Clay, Clara Keiko Oliveira Watanabe, Matias Tueros, Raul Sarmento, D. Melo, Mario Buscemi, Thomas Hebbeker, Maria-Teresa Dova, Sergio Dasso, Tristan Sudholz, Martin Vacula, Felix Schlüter, Magdalena Cerdá, E.E. Pereira Martins, Steffen Hahn, Juan Carlos D'Olivo, K. H. Kampert, T. Pierog, Fabian Gobbi, Christian Sarmiento-Cano, Hernán Asorey, Martín Miguel Freire, P.F. Gómez Vitale, Heino Falcke, Maximilian Reininghaus, L. R. Wiencke, Niklas Langner, J. C. Arteaga Velázquez, Petr Janecek, Brian Fick, M. Suárez-Durán, J. Vicha, Corbin Covault, Darko Veberič, Matías Rolf Hampel, Esteban Roulet, Rúben Conceição, R. Sato, Paula Gina Isar, J. Rautenberg, D. Nosek, F. Riehn, L. Nožka, Lourenco Lopes, M. Roth, S. Karpov, J. Perez Armand, E. Santos, Jesús Peña-Rodríguez, Q. Luce, Gaia Silli, Dusan Mandat, Justin M. Albury, A. Filipčič, T. Huege, F. Sanchez, Maximilian Stadelmaier, Frank G. Schröder, Lino Miramonti, Luis A. Nunez, A. Gorgi, A. Insolia, M. Kleifges, D. Zavrtanik, J. F. Valdés Galicia, Marcio Aparecido Muller, M. Zavrtanik, Antoine Letessier-Selvon, A. Fuster, L. Valore, I. De Mitri, Jeffrey Brack, S. Petrera, Marc Weber, W. M. Namasaka, M. Mastrodicasa, D. de Oliveira Franco, K. C. V. Varma, E. De Vito, Olaf Scholten, Marcus Niechciol, Humberto Ibarguen Salazar, C. M. Schäfer, A. C. Rovero, Giovanni Consolati, R.C. dos Anjos, Adriana Vásquez-Ramírez, E. M. Santos, A. Weindl, Bjarni Pont, Alexandru Balaceanu, M. A. Leigui de Oliveira, Roberto Mussa, Lorenzo Caccianiga, G. Golup, M. Palatka, R. Alves Batista, Bruce R. Dawson, C. Trimarelli, N. Kunka, H. Wilczyński, Claudio Galelli, L. Lu, Juan Manuel González, Carla Aramo, Vincenzo Rizi, P.O. Mazur, Julien Souchard, V. Novotny, C. J.W.P. Timmermans, D. Lo Presti, Rossella Caruso, A. Lucero, Fernando Catalani, D. Martello, S. J. De Jong, A. Tapia, Petr Schovanek, O. Martínez Bravo, Piera Luisa Ghia, T. Bister, Jon Paul Lundquist, A. Menshikov, H. Gemmeke, David Schmidt, S. Schröder, Italo Epicoco, M. Schimassek, François Montanet, Miguel Mostafa, Julian Kemp, S. Querchfeld, Sullivan Marafico, Olena Tkachenko, C. Hojvat, Jan Ebr, Valerio Verzi, Eleonora Guido, L. Nellen, Jarryd A. Day, A. Saftoiu, Marco Giammarchi, J. Šupík, Carlo Ventura, Octavian Sima, M. Mašek, B. Tome, C. Morello, Luis A. Anchordoqui, Jacco Vink, Alex Kääpä, Philipp Papenbreer, Samo Stanič, H.O. Klages, Petr Travnicek, L. Bonneau Arbeletche, Trent D. Grubb, Ladislav Chytka, A.C. Cobos Cerutti, R. Cunniffe, N. González, J. R. T. de Mello Neto, Peter L. Biermann, Juan Manuel Figueira, Isabel Goos, Roberta Colalillo, A. G. Mariazzi, J. Stasielak, Kai Daumiller, H. Schieler, Paolo Privitera, A. A. Nucita, Antonella Castellina, D. Heck, M. del Río, I. Ebrová, Denise Boncioli, P. Savina, W. Rodrigues de Carvalho, M. Jelínek, Jeffrey A. Johnsen, Nataliia Borodai, A. Segreto, Vladimir Lenok, L. Perrone, J. Hulsman, Günter Sigl, R. Squartini, Alfred Müller, P. Stassi, Radomir Smida, A. Machado Payeras, J. Eliášek, G. Medina-Tanco, Srijan Sehgal, Miroslav Pech, M. Pothast, Fernando Gollan, F. de Palma, Pavel Horvath, V. de Souza, Sofia Andringa, M. Schimp, B. C. Manning, Ana Martina Botti, Francesco Fenu, Miroslav Hrabovský, A. Haungs, Josina Schulte, Peter Hansen, P. Mantsch, Z. Szadkowski, J. Pkala, F. Guarino, John Matthews, Peter Buchholz, Marco Aglietta, R. M. de Almeida, D. Correia dos Santos, Rodrigo Pelayo, Stijn Buitink, Katie Mulrey, Orazio Zapparrata, Carola Dobrigkeit, M. Muzio, M. E. Bertaina, Alan Watson, M. Perlin, Mihai Niculescu-Oglinzanu, T. Suomijärvi, J. Pallotta, A. C. Fauth, Carla Bonifazi, Jose A. Bellido, Fabio Convenga, I.D. Vergara Quispe, Hernan Wahlberg, A. Parra, M. Trini, P.G. Brichetto Orchera, I. Allekotte, High Energy Astrophys. & Astropart. Phys (API, FNWI), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Institut de Physique Nucléaire d'Orsay (IPNO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Pierre Auger, Aab, A., Abreu, P., Aglietta, M., Albury, J. M., Allekotte, I., Almela, A., Alvarez-Mu??iz, J., Alves Batista, R., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Ara??jo Ferreira, P. R., Arteaga Vel??zquez, J. C., Asorey, H., Assis, P., Avila, G., Badescu, A. M., Bakalova, A., Balaceanu, A., Barbato, F., Barreira Luz, R. J., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Bister, T., Biteau, J., Blazek, J., Bleve, C., Boh????ov??, M., Boncioli, D., Bonifazi, C., Bonneau Arbeletche, L., Borodai, N., Botti, A. M., Brack, J., Bretz, T., Brichetto Orchera, P. G., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero-Mora, K. S., Caccianiga, L., Canfora, F., Caracas, I., Carceller, J. M., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Cerda, M., Chinellato, J. A., Choi, K., Chudoba, J., Chytka, L., Clay, R. W., Cobos Cerutti, A. C., Colalillo, R., Coleman, A., Coluccia, M. R., Concei????o, R., Condorelli, A., Consolati, G., Contreras, F., Convenga, F., Correia dos Santos, D., Covault, C. E., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., de Almeida, R. M., de Jes??s, J., de Jong, S. J., De Mauro, G., de Mello Neto, J. R. T., De Mitri, I., de Oliveira, J., de Oliveira Franco, D., de Palma, F., de Souza, V., De Vito, E., del R??o, M., Deligny, O., Di Matteo, A., Dobrigkeit, C., D'Olivo, J. C., dos Anjos, R. C., Dova, M. T., Ebr, J., Engel, R., Epicoco, I., Erdmann, M., Escobar, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Fick, B., Figueira, J. M., Filip??i??, A., Fodran, T., Freire, M. M., Fujii, T., Fuster, A., Galea, C., Galelli, C., Garc??a, B., Garcia Vegas, A. L., Gemmeke, H., Gesualdi, F., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., Glombitza, J., Gobbi, F., Gollan, F., Golup, G., G??mez Berisso, M., G??mez Vitale, P. F., Gongora, J. P., Gonz??lez, J. M., Gonz??lez, N., Goos, I., G??ra, D., Gorgi, A., Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Hahn, S., Hamal, P., Hampel, M. R., Hansen, P., Harari, D., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Hill, G. C., Hojvat, C., H??randel, J. R., Horvath, P., Hrabovsk??, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Janecek, P., Johnsen, J. A., Jurysek, J., K????p??, A., Kampert, K. H., Keilhauer, B., Kemp, J., Klages, H. O., Kleifges, M., Kleinfeller, J., K??pke, M., Kunka, N., Lago, B. L., Lang, R. G., Langner, N., Leigui de Oliveira, M. A., Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Lo Presti, D., Lopes, L., L??pez, R., Lu, L., Luce, Q., Lucero, A., Lundquist, J. P., Machado Payeras, A., Mancarella, G., Mandat, D., Manning, B. C., Manshanden, J., Mantsch, P., Marafico, S., Mariazzi, A. G., Mari??, I. C., Marsella, G., Martello, D., Martinez, H., Mart??nez Bravo, O., Mastrodicasa, M., Mathes, H. J., Matthews, J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina-Tanco, G., Melo, D., Menshikov, A., Merenda, K. -D., Michal, S., Micheletti, M. I., Miramonti, L., Mollerach, S., Montanet, F., Morello, C., Mostaf??, M., M??ller, A. L., Muller, M. A., Mulrey, K., Mussa, R., Muzio, M., Namasaka, W. M., Nasr-Esfahani, A., Nellen, L., Niculescu-Oglinzanu, M., Niechciol, M., Nitz, D., Nosek, D., Novotny, V., No??ka, L., Nucita, A., N????ez, L. A., Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Pech, M., Pedreira, F., P??kala, J., Pelayo, R., Pe??a-Rodriguez, J., Pereira Martins, E. E., Perez Armand, J., P??rez Bertolli, C., Perlin, M., Perrone, L., Petrera, S., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Pont, B., Pothast, M., Privitera, P., Prouza, M., Puyleart, A., Querchfeld, S., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Rizi, V., Rodrigues de Carvalho, W., Rodriguez Rojo, J., Roncoroni, M. J., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Salina, G., Sanabria Gomez, J. D., S??nchez, F., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Savina, P., Sch??fer, C. M., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schl??ter, F., Schmidt, D., Scholten, O., Schov??nek, P., Schr??der, F. G., Schr??der, S., Schulte, J., Sciutto, S. J., Scornavacche, M., Segreto, A., Sehgal, S., Shellard, R. C., Sigl, G., Silli, G., Sima, O., m??da, R., Sommers, P., Soriano, J. F., Souchard, J., Squartini, R., Stadelmaier, M., Stanca, D., Stani??, S., Stasielak, J., Stassi, P., Streich, A., Su??rez-Dur??n, M., Sudholz, T., Suomij??rvi, T., Supanitsky, A. D., up??k, J., Szadkowski, Z., Taboada, A., Tapia, A., Taricco, C., Timmermans, C., Tkachenko, O., Tobiska, P., Todero Peixoto, C. J., Tom??, B., Travaini, A., Travnicek, P., Trimarelli, C., Trini, M., Tueros, M., Ulrich, R., Unger, M., Vaclavek, L., Vacula, M., Vald??s Galicia, J. F., Valore, L., Varela, E., Varma K. C., V., V??squez-Ram??rez, A., Veberi??, D., Ventura, C., Vergara Quispe, I. D., Verzi, V., Vicha, J., Vink, J., Vorobiov, S., Wahlberg, H., Watanabe, C., Watson, A. A., Weber, M., Weindl, A., Wiencke, L., Wilczy??ski, H., Winchen, T., Wirtz, M., Wittkowski, D., Wundheiler, B., Yushkov, A., Zapparrata, O., Zas, E., Zavrtanik, D., Zavrtanik, M., Zehrer, L., Zepeda, A., Cunniffe, R., Eli????ek, J., Ebrov??, I., Jel??nek, M., Karpov, S., Kub??nek, P., Ma??ek, M., Pierre Auger Collaboration, T., Alvarez-Muniz, J., Araujo Ferreira, P. R., Arteaga Velazquez, J. C., Bohacova, M., Conceicao, R., Correia Dos Santos, D., De Almeida, R. M., De Jesus, J., De Jong, S. J., De Mello Neto, J. R. T., De Oliveira, J., De Oliveira Franco, D., De Palma, F., De Souza, V., Del Rio, M., Dos Anjos, R. C., Filipcic, A., Garcia, B., Gomez Berisso, M., Gomez Vitale, P. F., Gonzalez, J. M., Gonzalez, N., Gora, D., Horandel, J. R., Hrabovsky, M., Kaapa, A., Kopke, M., Leigui De Oliveira, M. A., Lopez, R., Maris, I. C., Martinez Bravo, O., Mostafa, M., Muller, A. L., Nozka, L., Nunez, L. A., Pkala, J., Pena-Rodriguez, J., Perez Bertolli, C., Rodrigues De Carvalho, W., Sanchez, F., Schafer, C. M., Schluter, F., Schovanek, P., Schroder, F. G., Schroder, S., Smida, R., Stanic, S., Suarez-Duran, M., Suomijarvi, T., Supik, J., Tome, B., Valdes Galicia, J. F., Varma, K. C. V., Vasquez-Ramirez, A., Veberic, D., Wilczynski, H., Eliasek, J., Ebrova, I., Jelinek, M., Kubanek, P., Masek, M., Research unit Astroparticle Physics, Pierre Auger Collaboration T., Aab A., Abreu P., Aglietta M., Albury J.M., Allekotte I., Almela A., Alvarez-Muniz J., Alves Batista R., Anastasi G.A., Anchordoqui L., Andrada B., Andringa S., Aramo C., Araujo Ferreira P.R., Arteaga Velazquez J.C., Asorey H., Assis P., Avila G., Badescu A.M., Bakalova A., Balaceanu A., Barbato F., Barreira Luz R.J., Becker K.H., Bellido J.A., Berat C., Bertaina M.E., Bertou X., Biermann P.L., Bister T., Biteau J., Blazek J., Bleve C., Bohacova M., Boncioli D., Bonifazi C., Bonneau Arbeletche L., Borodai N., Botti A.M., Brack J., Bretz T., Brichetto Orchera P.G., Briechle F.L., Buchholz P., Bueno A., Buitink S., Buscemi M., Caballero-Mora K.S., Caccianiga L., Canfora F., Caracas I., Carceller J.M., Caruso R., Castellina A., Catalani F., Cataldi G., Cazon L., Cerda M., Chinellato J.A., Choi K., Chudoba J., Chytka L., Clay R.W., Cobos Cerutti A.C., Colalillo R., Coleman A., Coluccia M.R., Conceicao R., Condorelli A., Consolati G., Contreras F., Convenga F., Correia Dos Santos D., Covault C.E., Dasso S., Daumiller K., Dawson B.R., Day J.A., De Almeida R.M., De Jesus J., De Jong S.J., De Mauro G., De Mello Neto J.R.T., De Mitri I., De Oliveira J., De Oliveira Franco D., De Palma F., De Souza V., De Vito E., Del Rio M., Deligny O., Di Matteo A., Dobrigkeit C., D'Olivo J.C., Dos Anjos R.C., Dova M.T., Ebr J., Engel R., Epicoco I., Erdmann M., Escobar C.O., Etchegoyen A., Falcke H., Farmer J., Farrar G., Fauth A.C., Fazzini N., Feldbusch F., Fenu F., Fick B., Figueira J.M., Filipcic A., Fodran T., Freire M.M., Fujii T., Fuster A., Galea C., Galelli C., Garcia B., Garcia Vegas A.L., Gemmeke H., Gesualdi F., Gherghel-Lascu A., Ghia P.L., Giaccari U., Giammarchi M., Giller M., Glombitza J., Gobbi F., Gollan F., Golup G., Gomez Berisso M., Gomez Vitale P.F., Gongora J.P., Gonzalez J.M., Gonzalez N., Goos I., Gora D., Gorgi A., Gottowik M., Grubb T.D., Guarino F., Guedes G.P., Guido E., Hahn S., Hamal P., Hampel M.R., Hansen P., Harari D., Harvey V.M., Haungs A., Hebbeker T., Heck D., Hill G.C., Hojvat C., Horandel J.R., Horvath P., Hrabovsky M., Huege T., Hulsman J., Insolia A., Isar P.G., Janecek P., Johnsen J.A., Jurysek J., Kaapa A., Kampert K.H., Keilhauer B., Kemp J., Klages H.O., Kleifges M., Kleinfeller J., Kopke M., Kunka N., Lago B.L., Lang R.G., Langner N., Leigui De Oliveira M.A., Lenok V., Letessier-Selvon A., Lhenry-Yvon I., Lo Presti D., Lopes L., Lopez R., Lu L., Luce Q., Lucero A., Lundquist J.P., Machado Payeras A., Mancarella G., Mandat D., Manning B.C., Manshanden J., Mantsch P., Marafico S., Mariazzi A.G., Maris I.C., Marsella G., Martello D., Martinez H., Martinez Bravo O., Mastrodicasa M., Mathes H.J., Matthews J., Matthiae G., Mayotte E., Mazur P.O., Medina-Tanco G., Melo D., Menshikov A., Merenda K.-D., Michal S., Micheletti M.I., Miramonti L., Mollerach S., Montanet F., Morello C., Mostafa M., Muller A.L., Muller M.A., Mulrey K., Mussa R., Muzio M., Namasaka W.M., Nasr-Esfahani A., Nellen L., Niculescu-Oglinzanu M., Niechciol M., Nitz D., Nosek D., Novotny V., Nozka L., Nucita A., Nunez L.A., Palatka M., Pallotta J., Papenbreer P., Parente G., Parra A., Pech M., Pedreira F., Pkala J., Pelayo R., Pena-Rodriguez J., Pereira Martins E.E., Perez Armand J., Perez Bertolli C., Perlin M., Perrone L., Petrera S., Pierog T., Pimenta M., Pirronello V., Platino M., Pont B., Pothast M., Privitera P., Prouza M., Puyleart A., Querchfeld S., Rautenberg J., Ravignani D., Reininghaus M., Ridky J., Riehn F., Risse M., Rizi V., Rodrigues De Carvalho W., Rodriguez Rojo J., Roncoroni M.J., Roth M., Roulet E., Rovero A.C., Ruehl P., Saffi S.J., Saftoiu A., Salamida F., Salazar H., Salina G., Sanabria Gomez J.D., Sanchez F., Santos E.M., Santos E., Sarazin F., Sarmento R., Sarmiento-Cano C., Sato R., Savina P., Schafer C.M., Scherini V., Schieler H., Schimassek M., Schimp M., Schluter F., Schmidt D., Scholten O., Schovanek P., Schroder F.G., Schroder S., Schulte J., Sciutto S.J., Scornavacche M., Segreto A., Sehgal S., Shellard R.C., Sigl G., Silli G., Sima O., Smida R., Sommers P., Soriano J.F., Souchard J., Squartini R., Stadelmaier M., Stanca D., Stanic S., Stasielak J., Stassi P., Streich A., Suarez-Duran M., Sudholz T., Suomijarvi T., Supanitsky A.D., Supik J., Szadkowski Z., Taboada A., Tapia A., Taricco C., Timmermans C., Tkachenko O., Tobiska P., Todero Peixoto C.J., Tome B., Travaini A., Travnicek P., Trimarelli C., Trini M., Tueros M., Ulrich R., Unger M., Vaclavek L., Vacula M., Valdes Galicia J.F., Valore L., Varela E., Varma K.C.V., Vasquez-Ramirez A., Veberic D., Ventura C., Vergara Quispe I.D., Verzi V., Vicha J., Vink J., Vorobiov S., Wahlberg H., Watanabe C., Watson A.A., Weber M., Weindl A., Wiencke L., Wilczynski H., Winchen T., Wirtz M., Wittkowski D., Wundheiler B., Yushkov A., Zapparrata O., Zas E., Zavrtanik D., Zavrtanik M., Zehrer L., Zepeda A., Cunniffe R., Eliasek J., Ebrova I., Jelinek M., Karpov S., Kubanek P., Masek M., and Physics

Subjects
Astronomy, Large detector systems for particle and astroparticle physics, Optics, Photon detectors for UV, visible and IR photons (solid-state) (PIN diodes, APDs, Si-PMTs, G-APDs, CCDs, EBCCDs, EMCCDs, CMOS imagers, etc), Real-time monitoring, 01 natural sciences, Auger, Successful operation, Observatory, optical, APDs, hardware, Astrophysics::Solar and Stellar Astrophysics, 010303 astronomy & astrophysics, Instrumentation, Photon detectors for UV, Mathematical Physics, High Energy Astrophysical Phenomena (astro-ph.HE), astro-ph.HE, EBCCDs, Settore FIS/01 - Fisica Sperimentale, Astrophysics::Instrumentation and Methods for Astrophysics, Si-PMTs, observatory, Robotic telescope, G-APDs, Astrophysics::Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Sciences exactes et naturelles, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, programming, detector: fluorescence, Photometry (optics), 0103 physical sciences, ddc:610, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], High Energy Physics, visible and IR photons (solid-state) (PIN diodes, CMOS imagers, Instrumentation and Methods for Astrophysics (astro-ph.IM), Astrophysics::Galaxy Astrophysics, Remote sensing, etc), fluorescence [detector], Pierre Auger Observatory, 010308 nuclear & particles physics, Active monitoring, CCDs, laser, monitoring, EMCCDs, Large detector systems for particle and astroparticle physic, atmosphere, Experimental High Energy Physics, Optic, Environmental science, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], RAIOS CÓSMICOS, astro-ph.IM
Abstract

FRAM (F/Photometric Robotic Atmospheric Monitor) is a robotic telescope operated at the Pierre Auger Observatory in Argentina for the purposes of atmospheric monitoring using stellar photometry. As a passive system which does not produce any light that could interfere with the observations of the fluorescence telescopes of the observatory, it complements the active monitoring systems that use lasers. We discuss the applications of stellar photometry for atmospheric monitoring at optical observatories in general and the particular modes of operation employed by the Auger FRAM. We describe in detail the technical aspects of FRAM, the hardware and software requirements for a successful operation of a robotic telescope for such a purpose and their implementation within the FRAM system., Published version, 27 pages, 8 figures

Published
2021

19. The relentless variability of Mrk 421 from the TeV to the radio

Author

E. von Willert, Daniela Dorner, Karl Mannheim, M. Bulinski, Sebastian Achim Mueller, Vitalii Sliusar, Thomas Bretz, J. Buss, Manuel Doerr, D. Hildebrand, Wolfgang Rhode, Adrian Biland, A. Arbet-Engels, K. Sedlaczek, M. Noethe, K. Bruegge, D. Elsaesser, Bernd Schleicher, Michael Blank, D. Neise, M. Balbo, A. Shukla, R. Walter, A. Paravac, and Dominik Baack

Subjects
Cosmology and Nongalactic Astrophysics (astro-ph.CO), Astrophysics::High Energy Astrophysical Phenomena, Hadron, FOS: Physical sciences, Context (language use), Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, law.invention, Telescope, law, 0103 physical sciences, Radiative transfer, Blazar, 010303 astronomy & astrophysics, Astroparticle physics, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), 010308 nuclear & particles physics, Astronomy and Astrophysics, Light curve, Astrophysics - Astrophysics of Galaxies, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), High Energy Physics::Experiment, Astrophysics - High Energy Astrophysical Phenomena, Fermi Gamma-ray Space Telescope, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

The origin of the gamma-ray emission of the blazar Mrk 421 is still a matter of debate. We used 5.5 years of unbiased observing campaign data, obtained using the FACT telescope and the Fermi LAT detector at TeV and GeV energies, the longest and densest so far, together with contemporaneous multi-wavelength observations, to characterise the variability of Mrk 421 and to constrain the underlying physical mechanisms. We studied and correlated light curves obtained by ten different instruments and found two significant results. The TeV and X-ray light curves are very well correlated with a lag of, 10 pages, 8 figures, 1 table

Published
2021

20. Studying the long-term spectral and temporal evolution of 1ES 1959$\mathplus$650

Author

Shunsuke, Sakurai, Acciari, Victor A., Stefano, Ansoldi, Lucio Angelo Antonelli, Axel Arbet Engels, Manuel, Artero, Katsuaki, Asano, Dominik, Baack, Ana, Babi('(c)), Andr('(e))s, Baquero, Ulisses Barres de Almeida, Juan Abel Barrio, Ivana, Batkovi('(c)), Josefa Becerra Gonz('(a))lez, Wlodek, Bednarek, Lorenzo, Bellizzi, Elisa, Bernardini, Maria-Isabel, Bernardos, Alessio, Berti, Jürgen, Besenrieder, Wrijupan, Bhattacharyya, Ciro, Bigongiari, Adrian, Biland, Oscar, Blanch, Hendrik, Bökenkamp, Giacomo Bonnoli, ( (Z))eljka Bo( (s))njak, Giovanni, Busetto, Roberto, Carosi, Giovanni, Ceribella, Matteo, Cerruti, Yating, Chai, Ashot, Chilingarian, Stefan, Cikota, Sidika Merve Colak, Eduardo, Colombo, Jose Luis Contreras, Juan, Cortina, Stefano, Covino, Giacomo D( extquotesingle)Amico, Valerio D( extquotesingle)Elia, Paolo Da Vela, Francesco, Dazzi, Alessandro De Angelis, Barbara De Lotto, Manuel, Delfino, Jordi, Delgado, Carlos Delgado Mendez, Davide, Depaoli, Federico Di Pierro, Leonardo Di Venere, Elia Do Souto Espi(~(n))eira, Dijana Dominis Prester, Alice, Donini, Daniela, Dorner, Michele, Doro, Dominik, Elsaesser, Vandad Fallah Ramazani, Alicia, Fattorini, Maria Victoria Fonseca, Lluis, Font, Christian, Fruck, Satoshi, Fukami, Yasushi, Fukazawa, Garc('(i))a L('(o))pez, Ramon J., Markus, Garczarczyk, Sargis, Gasparyan, Markus, Gaug, Giglietto, Nicola, Francesco, Giordano, Pawel, Gliwny, Nikola, Godinovi('(c)), David, Green, Jarred Gershon Green, Daniela, Hadasch, Alexander, Hahn, Lea, Heckmann, Javier, Herrera, John, Hoang, Dario, Hrupec, Moritz, Hütten, Tomohiro, Inada, Kazuma, Ishio, Yuki, Iwamura, Irene Jim('(e))nez Mart('(i))nez, Jenni, Jormanainen, L('(e))a, Jouvin, Marie, Karjalainen, Daniel, Kerszberg, Yukiho, Kobayashi, Hidetoshi, Kubo, Junko, Kushida, Alessandra, Lamastra, Damir, Lelas, Francesco, Leone, Elina, Lindfors, Lena, Linhoff, Saverio, Lombardi, Francesco, Longo, Rub('(e))n, L('(o))pez-Coto, Marcos, L('(o))pez-Moya, Alicia, L('(o))pez-Oramas, Loporchio, Serena, Bernardo Machado de Oliveira Fraga, Camilla, Maggio, Pratik, Majumdar, Martin, Makariev, Manuela, Mallamaci, Galina, Maneva, Marina, Manganaro, Karl, Mannheim, Laura, Maraschi, Mos(`(e)), Mariotti, Manel, Mart('(i))nez, Daniel, Mazin, Stefano, Menchiari, Simone, Mender, Sa( (s))a Mi('(c))anovi('(c)), Davide, Miceli, Tjark, Miener, Jose Miguel Miranda, Razmik, Mirzoyan, Edgar, Molina, Abelardo, Moralejo, Daniel, Morcuende, Victoria, Moreno, Elena, Moretti, Takeshi, Nakamori, Lara, Nava, Vitaly, Neustroev, Cosimo, Nigro, Kari, Nilsson, Kyoshi, Nishijima, Koji, Noda, Seiya, Nozaki, Yoshiki, Ohtani, Tomohiko, Oka, Jorge, Otero-Santos, Simona, Paiano, Michele, Palatiello, David, Paneque, Riccardo, Paoletti, Paredes, Josep M., Lovro, Pavleti('(c)), Pablo, Pe(~(n))il, Massimo, Persic, Marine, Pihet, Pier Giorgio Prada Moroni, Elisa, Prandini, Chaitanya, Priyadarshi, Ivica, Puljak, Wolfgang, Rhode, Marc, Rib('(o)), Javier, Rico, Chiara, Righi, Andrea, Rugliancich, Narek, Sahakyan, Takayuki, Saito, Konstancja, Satalecka, Francesco Gabriele Saturni, Bernd, Schleicher, Kevin, Schmidt, Thomas, Schweizer, Julian, Sitarek, Iva, ( (S))nidari('(c)), Dorota, Sobczy('(n))ska, Alessia, Spolon, Antonio, Stamerra, Jelena Stri( (s))kovi('(c)), Derek, Strom, Marcel, Strzys, Yusuke, Suda, Tihomir, Suri('(c)), Mitsunari, Takahashi, Ryuji, Takeishi, Fabrizio, Tavecchio, Petar, Temnikov, Tomislav, Terzi('(c)), Masahiro, Teshima, Luca, Tosti, Stefano, Truzzi, Antonio, Tutone, Santiago, Ubach, Juliane van Scherpenberg, Gaia, Vanzo, Monica VAZQUEZ ACOSTA, Sofia, Ventura, Vassil, Verguilov, Carlo Francesco Vigorito, Vincenzo, Vitale, Ievgen, Vovk, Martin, Will, Carolin, Wunderlich, Tokonatsu, Yamamoto, Darko, Zari('(c)), Matteo, Balbo, Thomas, Bretz, Jens, Buss, Laura, Eisenberger, Dorothee, Hildebrand, Roman, Iotov, Adelina, Kalenski, Alison, Mitchell, Dominik, Neise, Maximilian, Noethe, Aleksander, Paravac, Vitalii, Sliusar, Roland, Walter, Pietro, Grespan, Mari, Takahashi, Yasuyuki, Nabatame, and And

Published
2021

21. Multiwavelength variability and correlation studies of Mrk421 during historically low X-ray and $\upgamma$-ray activity in 2015{\textendash}2016

Author

Biswajit, Banerjee, Acciari, Victor A., Stefano, Ansoldi, Lucio Angelo Antonelli, Axel Arbet Engels, Manuel, Artero, Katsuaki, Asano, Dominik, Baack, Ana, Babi('(c)), Andr('(e))s, Baquero, Ulisses Barres de Almeida, Juan Abel Barrio, Ivana, Batkovi('(c)), Josefa Becerra Gonz('(a))lez, Wlodek, Bednarek, Lorenzo, Bellizzi, Elisa, Bernardini, Maria-Isabel, Bernardos, Alessio, Berti, Jürgen, Besenrieder, Wrijupan, Bhattacharyya, Ciro, Bigongiari, Adrian, Biland, Oscar, Blanch, Hendrik, Bökenkamp, Giacomo Bonnoli, ( (Z))eljka Bo( (s))njak, Giovanni, Busetto, Roberto, Carosi, Giovanni, Ceribella, Matteo, Cerruti, Yating, Chai, Ashot, Chilingarian, Stefan, Cikota, Sidika Merve Colak, Eduardo, Colombo, Jose Luis Contreras, Juan, Cortina, Stefano, Covino, Giacomo D( extquotesingle)Amico, Valerio D( extquotesingle)Elia, Paolo Da Vela, Francesco, Dazzi, Alessandro De Angelis, Barbara De Lotto, Manuel, Delfino, Jordi, Delgado, Carlos Delgado Mendez, Davide, Depaoli, Federico Di Pierro, Leonardo Di Venere, Elia Do Souto Espi(~(n))eira, Dijana Dominis Prester, Alice, Donini, Daniela, Dorner, Michele, Doro, Dominik, Elsaesser, Vandad Fallah Ramazani, Alicia, Fattorini, Maria Victoria Fonseca, Lluis, Font, Christian, Fruck, Satoshi, Fukami, Yasushi, Fukazawa, Garc('(i))a L('(o))pez, Ramon J., Markus, Garczarczyk, Sargis, Gasparyan, Markus, Gaug, Giglietto, Nicola, Francesco, Giordano, Pawel, Gliwny, Nikola, Godinovi('(c)), David, Green, Jarred Gershon Green, Daniela, Hadasch, Alexander, Hahn, Lea, Heckmann, Javier, Herrera, John, Hoang, Dario, Hrupec, Moritz, Hütten, Tomohiro, Inada, Kazuma, Ishio, Yuki, Iwamura, Irene Jim('(e))nez Mart('(i))nez, Jenni, Jormanainen, L('(e))a, Jouvin, Marie, Karjalainen, Daniel, Kerszberg, Yukiho, Kobayashi, Hidetoshi, Kubo, Junko, Kushida, Alessandra, Lamastra, Damir, Lelas, Francesco, Leone, Elina, Lindfors, Lena, Linhoff, Saverio, Lombardi, Francesco, Longo, Rub('(e))n, L('(o))pez-Coto, Marcos, L('(o))pez-Moya, Alicia, L('(o))pez-Oramas, Loporchio, Serena, Bernardo Machado de Oliveira Fraga, Camilla, Maggio, Pratik, Majumdar, Martin, Makariev, Manuela, Mallamaci, Galina, Maneva, Marina, Manganaro, Karl, Mannheim, Laura, Maraschi, Mos(`(e)), Mariotti, Manel, Mart('(i))nez, Daniel, Mazin, Stefano, Menchiari, Simone, Mender, Sa( (s))a Mi('(c))anovi('(c)), Davide, Miceli, Tjark, Miener, Jose Miguel Miranda, Razmik, Mirzoyan, Edgar, Molina, Abelardo, Moralejo, Daniel, Morcuende, Victoria, Moreno, Elena, Moretti, Takeshi, Nakamori, Lara, Nava, Vitaly, Neustroev, Cosimo, Nigro, Kari, Nilsson, Kyoshi, Nishijima, Koji, Noda, Seiya, Nozaki, Yoshiki, Ohtani, Tomohiko, Oka, Jorge, Otero-Santos, Simona, Paiano, Michele, Palatiello, David, Paneque, Riccardo, Paoletti, Paredes, Josep M., Lovro, Pavleti('(c)), Pablo, Pe(~(n))il, Massimo, Persic, Marine, Pihet, Pier Giorgio Prada Moroni, Elisa, Prandini, Chaitanya, Priyadarshi, Ivica, Puljak, Wolfgang, Rhode, Marc, Rib('(o)), Javier, Rico, Chiara, Righi, Andrea, Rugliancich, Narek, Sahakyan, Takayuki, Saito, Shunsuke, Sakurai, Konstancja, Satalecka, Francesco Gabriele Saturni, Bernd, Schleicher, Kevin, Schmidt, Thomas, Schweizer, Julian, Sitarek, Iva, ( (S))nidari('(c)), Dorota, Sobczy('(n))ska, Alessia, Spolon, Antonio, Stamerra, Jelena Stri( (s))kovi('(c)), Derek, Strom, Marcel, Strzys, Yusuke, Suda, Tihomir, Suri('(c)), Mitsunari, Takahashi, Ryuji, Takeishi, Fabrizio, Tavecchio, Petar, Temnikov, Tomislav, Terzi('(c)), Masahiro, Teshima, Luca, Tosti, Stefano, Truzzi, Antonio, Tutone, Santiago, Ubach, Juliane van Scherpenberg, Gaia, Vanzo, Monica VAZQUEZ ACOSTA, Sofia, Ventura, Vassil, Verguilov, Carlo Francesco Vigorito, Vincenzo, Vitale, Ievgen, Vovk, Martin, Will, Carolin, Wunderlich, Tokonatsu, Yamamoto, Darko, Zari('(c)), Matteo, Balbo, Thomas, Bretz, Jens, Buss, Laura, Eisenberger, Dorothee, Hildebrand, Roman, Iotov, Adelina, Kalenski, Alison, Mitchell, Dominik, Neise, Maximilian, Noethe, Aleksander, Paravac, Vitalii, Sliusar, Roland, Walter, Valverde, J., Horan, D., Giroletti, M., Perri, M., Verrecchia, F., Leto, C., Sadun, A. C., Moody, J. W., Joner, M., Marscher, A. P., Jorstad, S. G., Lähteenmäki, A., ( extasciitilde)Tornikoski, M., Ramakrishnan, V., Järvelä, E., Vera, R. J. C., Righini, S., Lien, A. Y., and And

Published
2021

22. Measurement of the Fluctuations in the Number of Muons in Extensive Air Showers with the Pierre Auger Observatory

Author

H. J. Mathes, Stanislav Michal, Miroslav Pech, Antonio Condorelli, M. Pothast, Pavel Horvath, A.L. Garcia Vegas, W. M. Namasaka, A. C. Rovero, M. Risse, J. Rodriguez Rojo, Fridtjof Feldbusch, B. Andrada, Alexandru Balaceanu, Jonathan Blazek, Carla Aramo, Vincenzo Rizi, J. F. Valdés Galicia, Julien Souchard, Sofia Andringa, Enrique Zas, Magdalena Cerdá, Hernán Asorey, I. De Mitri, D. Martello, David Wittkowski, O. Martínez Bravo, K. Mulrey, P. Abreu, D. Ravignani, G. Salina, Danielle LaHurd, Olivier Deligny, Marcel Köpke, M. Platino, Fernando Contreras, A. Tapia, H. Gemmeke, G. Parente, Fabrizia Canfora, L. Zehrer, L. Lopes, Tomáš Fodran, Jaime Alvarez-Muñiz, Alexandru Gherghel-Lascu, M. A. Leigui de Oliveira, Flavia Gesualdi, G. Kukec Mezek, G. Marsella, Valerio Pirronello, R. Lorek, G. De Mauro, M. Unger, Ugo Giaccari, Silvia Mollerach, H. Dembinski, N. Fazzini, Jonas Glombitza, F. C. T. Barbato, Dariusz Gora, M. E. Bertaina, Jon Paul Lundquist, A. Menshikov, K.-H. Becker, M. Pimenta, P.R. Araújo Ferreira, J. de Oliveira, Alejandro Almela, C. J. Todero Peixoto, M. Zavrtanik, Lukáš Vaclavek, W. Rodrigues de Carvalho, Jörg R. Hörandel, B. Keilhauer, Marcus Niechciol, A. C. Fauth, Teresa Bister, J. Chudoba, Alan Coleman, B. Tome, Josina Schulte, S. J. Saffi, Tobias Winchen, Julian Kemp, S. J. Sciutto, Carla Bleve, Rodrigo Guedes Lang, Florian Lukas Briechle, Peter Hansen, Lorenzo Caccianiga, Marvin Gottowik, Julien Manshanden, G. Cataldi, E. De Vito, F. Guarino, John Matthews, I. Lhenry-Yvon, Nataliia Borodai, V. Scherini, Paul Sommers, Peter Buchholz, Andres Travaini, Giovanni Consolati, E. Varela, J.D. Sanabria Gomez, Juan Miguel Carceller, Christian Sarmiento-Cano, R. M. de Almeida, P. Tobiska, Alex Kääpä, F. Pedreira, Carla Bonifazi, D. Lo Presti, Jose A. Bellido, S. J. De Jong, Marco Aglietta, Vladimir Lenok, Eric Mayotte, Raul Sarmento, Fabio Convenga, M. M. Freire, Felix Schlüter, H. Wilczyński, Jeffrey A. Johnsen, Fabian Gobbi, Jose Chinellato, F. Sánchez, Serguei Vorobiov, L. Perrone, Alena Bakalova, E. M. Santos, D. Nitz, R. Squartini, Alfred Müller, Petr Schovanek, Valerio Verzi, A. Fuster, G. Golup, M. Gómez Berisso, R. C. Shellard, Octavian Sima, Jarryd A. Day, A. Saftoiu, A.C. Cobos Cerutti, J. R. T. de Mello Neto, G. Torralba Elipe, R. Alves Batista, Bruce R. Dawson, G. Matthiae, Jesús Peña-Rodríguez, Antonio Bueno, Thomas Hebbeker, Sergio Dasso, Tristan Sudholz, H. Schieler, Antonella Castellina, Maria Rita Coluccia, A. Di Matteo, M. Schimp, B. Wundheiler, B. C. Manning, A. Insolia, M. Kleifges, D. Zavrtanik, A.D. Supanitsky, Fred Sarazin, J. Pȩkala, Ioana Caracas, A. Letessier-Selvon, B. García, R. López, Karen S. Caballero-Mora, P.O. Mazur, Thomas Bretz, Lorenzo Cazon, Darko Veberič, Mario Buscemi, Roberto Mussa, T. Huege, I.D. Vergara Quispe, G. Medina-Tanco, R. Halliday, L. Valore, J. Rautenberg, Jeffrey Brack, Günter Sigl, Olaf Scholten, F. Riehn, Marina Scornavacche, Corbin Covault, Jonathan Biteau, Francesco Fenu, Xavier Bertou, Humberto Ibarguen Salazar, L. R. Wiencke, Rodrigo Pelayo, Stijn Buitink, Niklas Langner, S. Querchfeld, Olena Tkachenko, J. Šupík, Carlo Ventura, Gualberto Avila, Q. Luce, M. Suárez-Durán, Maximilian Reininghaus, A. Zepeda, Brian Fick, Nicolás González, P. Stassi, Ladislav Chytka, Lino Miramonti, Ioana Codrina Maris, Pedro Assis, François Montanet, Radomir Smida, A. Machado Payeras, Martin Erdmann, J. de Jesús, H. Martinez, A. Etchegoyen, Maximilian Stadelmaier, Sullivan Marafico, Miguel Mostafa, P. Ruehl, D. de Oliveira Franco, A. Streich, Gioacchino Alex Anastasi, Dusan Mandat, J. Stasielak, J. Hulsman, J. Kleinfeller, G. C. Hill, Marco Giammarchi, M. Wirtz, Frank G. Schröder, Eleonora Guido, Roger W Clay, Jorge F. Soriano, Ralph Engel, Denis Stanca, C. M. Schäfer, Fernando Gollan, Massimo Mastrodicasa, Hernan Wahlberg, L. Nellen, Carlos Escobar, Kevin-Druis Merenda, Samo Stanič, K. H. Kampert, J. Ridky, R.J. Barreira Luz, Martin Vacula, John Farmer, C. Morello, Heino Falcke, A. Puyleart, V. de Souza, R. Conceição, Miroslav Hrabovský, Corinne Berat, M. Giller, Isabel Goos, Luis A. Anchordoqui, A. Parra, J. Perez Armand, Kai Daumiller, D. Heck, Maria-Teresa Dova, M. R. Hampel, J. Vicha, A. Haungs, L. Bonneau Arbeletche, Peter L. Biermann, Philipp Papenbreer, M. Schimassek, M. del Río, C. Hojvat, Petr Travnicek, Jan Ebr, Claudio Galelli, Denise Boncioli, Trent D. Grubb, Paolo Privitera, P. Ristori, Jacco Vink, M. Trini, H.O. Klages, M. A. Muller, Markus Roth, Juan Manuel Figueira, Roberta Colalillo, A. G. Mariazzi, P. Savina, A. Aab, A. A. Nucita, Ralf Ulrich, Martina Bohacova, M. I. Micheletti, B. L. Lago, R.C. dos Anjos, Adriana Vásquez-Ramírez, Giovanni Mancarella, Juan Pablo Gongora, M. Palatka, P. Mantsch, A. Cancio, Z. Szadkowski, Matias Tueros, Luis A. Nunez, Paula Gina Isar, F. Salamida, V. Novotny, I. Allekotte, M. J. Roncoroni, Rossella Caruso, A. Lucero, Fernando Catalani, T. Suomijärvi, Caterina Trimarelli, A. Yushkov, D. Melo, D. Nosek, E. Santos, R. Sato, J. Pallotta, A. M. Botti, Niraj Dhital, I. Valiño, G. P. Guedes, Alessio Gorgi, A. Weindl, L. Nožka, Toshihiro Fujii, Orazio Zapparrata, Jakub Juryšek, J. Debatin, Carola Dobrigkeit, M. Muzio, Steffen Hahn, Juan Carlos D'Olivo, T. Pierog, Esteban Roulet, Justin M. Albury, Alan Watson, David Schmidt, S. Schröder, Italo Epicoco, M. Perlin, Mihai Niculescu-Oglinzanu, Piera Luisa Ghia, G. Farrar, A. Taboada, P.F. Gómez Vitale, Violet M. Harvey, D. Harari, Alina Mihaela Badescu, Cristina Galea, M. Prouza, Gaia Silli, A. Filipčič, S. Petrera, Marc Weber, Bjarni Pont, C. J.W.P. Timmermans, K. Choi, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Institut de Physique Nucléaire d'Orsay (IPNO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Pierre Auger, Aab, A, Abreu, P, Aglietta, M, Albury, J M, Allekotte, I, Almela, A, Alvarez-Muñiz, J, Alves Batista, R, Anastasi, G A, Anchordoqui, L, Andrada, B, Andringa, S, Aramo, C, Araújo Ferreira, P R, Asorey, H, Assis, P, Avila, G, Badescu, A M, Bakalova, A, Balaceanu, A, Barbato, F, Barreira Luz, R J, Becker, K H, Bellido, J A, Berat, C, Bertaina, M E, Bertou, X, Biermann, P L, Bister, T, Biteau, J, Blazek, J, Bleve, C, Boháčová, M, Boncioli, D, Bonifazi, C, Bonneau Arbeletche, L, Borodai, N, Botti, A M, Brack, J, Bretz, T, Briechle, F L, Buchholz, P, Bueno, A, Buitink, S, Buscemi, M, Caballero-Mora, K S, Caccianiga, L, Cancio, A, Canfora, F, Caracas, I, Carceller, J M, Caruso, R, Castellina, A, Catalani, F, Cataldi, G, Cazon, L, Cerda, M, Chinellato, J A, Choi, K, Chudoba, J, Chytka, L, Clay, R W, Cobos Cerutti, A C, Colalillo, R, Coleman, A, Coluccia, M R, Conceição, R, Condorelli, A, Consolati, G, Contreras, F, Convenga, F, Covault, C E, Dasso, S, Daumiller, K, Dawson, B R, Day, J A, de Almeida, R M, de Jesús, J, de Jong, S J, De Mauro, G, de Mello Neto, J R T, De Mitri, I, de Oliveira, J, de Oliveira Franco, D, de Souza, V, De Vito, E, Debatin, J, Del Río, M, Deligny, O, Dembinski, H, Dhital, N, Di Matteo, A, Dobrigkeit, C, D'Olivo, J C, Dos Anjos, R C, Dova, M T, Ebr, J, Engel, R, Epicoco, I, Erdmann, M, Escobar, C O, Etchegoyen, A, Falcke, H, Farmer, J, Farrar, G, Fauth, A C, Fazzini, N, Feldbusch, F, Fenu, F, Fick, B, Figueira, J M, Filipčič, A, Fodran, T, Freire, M M, Fujii, T, Fuster, A, Galea, C, Galelli, C, García, B, Garcia Vegas, A L, Gemmeke, H, Gesualdi, F, Gherghel-Lascu, A, Ghia, P L, Giaccari, U, Giammarchi, M, Giller, M, Glombitza, J, Gobbi, F, Gollan, F, Golup, G, Gómez Berisso, M, Gómez Vitale, P F, Gongora, J P, González, N, Goos, I, Góra, D, Gorgi, A, Gottowik, M, Grubb, T D, Guarino, F, Guedes, G P, Guido, E, Hahn, S, Halliday, R, Hampel, M R, Hansen, P, Harari, D, Harvey, V M, Haungs, A, Hebbeker, T, Heck, D, Hill, G C, Hojvat, C, Hörandel, J R, Horvath, P, Hrabovský, M, Huege, T, Hulsman, J, Insolia, A, Isar, P G, Johnsen, J A, Jurysek, J, Kääpä, A, Kampert, K H, Keilhauer, B, Kemp, J, Klages, H O, Kleifges, M, Kleinfeller, J, Köpke, M, Kukec Mezek, G, Lago, B L, Lahurd, D, Lang, R G, Langner, N, Leigui de Oliveira, M A, Lenok, V, Letessier-Selvon, A, Lhenry-Yvon, I, Lo Presti, D, Lopes, L, López, R, Lorek, R, Luce, Q, Lucero, A, Lundquist, J P, Machado Payeras, A, Mancarella, G, Mandat, D, Manning, B C, Manshanden, J, Mantsch, P, Marafico, S, Mariazzi, A G, Mariş, I C, Marsella, G, Martello, D, Martinez, H, Martínez Bravo, O, Mastrodicasa, M, Mathes, H J, Matthews, J, Matthiae, G, Mayotte, E, Mazur, P O, Medina-Tanco, G, Melo, D, Menshikov, A, Merenda, K-D, Michal, S, Micheletti, M I, Miramonti, L, Mollerach, S, Montanet, F, Morello, C, Mostafá, M, Müller, A L, Muller, M A, Mulrey, K, Mussa, R, Muzio, M, Namasaka, W M, Nellen, L, Niculescu-Oglinzanu, M, Niechciol, M, Nitz, D, Nosek, D, Novotny, V, Nožka, L, Nucita, A, Núñez, L A, Palatka, M, Pallotta, J, Papenbreer, P, Parente, G, Parra, A, Pech, M, Pedreira, F, Pȩkala, J, Pelayo, R, Peña-Rodriguez, J, Perez Armand, J, Perlin, M, Perrone, L, Petrera, S, Pierog, T, Pimenta, M, Pirronello, V, Platino, M, Pont, B, Pothast, M, Privitera, P, Prouza, M, Puyleart, A, Querchfeld, S, Rautenberg, J, Ravignani, D, Reininghaus, M, Ridky, J, Riehn, F, Risse, M, Ristori, P, Rizi, V, Rodrigues de Carvalho, W, Rodriguez Rojo, J, Roncoroni, M J, Roth, M, Roulet, E, Rovero, A C, Ruehl, P, Saffi, S J, Saftoiu, A, Salamida, F, Salazar, H, Salina, G, Sanabria Gomez, J D, Sánchez, F, Santos, E M, Santos, E, Sarazin, F, Sarmento, R, Sarmiento-Cano, C, Sato, R, Savina, P, Schäfer, C M, Scherini, V, Schieler, H, Schimassek, M, Schimp, M, Schlüter, F, Schmidt, D, Scholten, O, Schovánek, P, Schröder, F G, Schröder, S, Schulte, J, Sciutto, S J, Scornavacche, M, Shellard, R C, Sigl, G, Silli, G, Sima, O, Šmída, R, Sommers, P, Soriano, J F, Souchard, J, Squartini, R, Stadelmaier, M, Stanca, D, Stanič, S, Stasielak, J, Stassi, P, Streich, A, Suárez-Durán, M, Sudholz, T, Suomijärvi, T, Supanitsky, A D, Šupík, J, Szadkowski, Z, Taboada, A, Tapia, A, Timmermans, C, Tkachenko, O, Tobiska, P, Todero Peixoto, C J, Tomé, B, Torralba Elipe, G, Travaini, A, Travnicek, P, Trimarelli, C, Trini, M, Tueros, M, Ulrich, R, Unger, M, Vaclavek, L, Vacula, M, Valdés Galicia, J F, Valiño, I, Valore, L, Varela, E, Varma K C, V, Vásquez-Ramírez, A, Veberič, D, Ventura, C, Vergara Quispe, I D, Verzi, V, Vicha, J, Vink, J, Vorobiov, S, Wahlberg, H, Watson, A A, Weber, M, Weindl, A, Wiencke, L, Wilczyński, H, Winchen, T, Wirtz, M, Wittkowski, D, Wundheiler, B, Yushkov, A, Zapparrata, O, Zas, E, Zavrtanik, D, Zavrtanik, M, Zehrer, L, Zepeda, A, High Energy Astrophys. & Astropart. Phys (API, FNWI), Gravitation and Astroparticle Physics Amsterdam, Physics, Aab, A., Abreu, P., Aglietta, M., Albury, J. M., Allekotte, I., Almela, A., Alvarez-Muniz, J., Alves Batista, R., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Araujo Ferreira, P. R., Asorey, H., Assis, P., Avila, G., Badescu, A. M., Bakalova, A., Balaceanu, A., Barbato, F., Barreira Luz, R. J., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Bister, T., Biteau, J., Blazek, J., Bleve, C., Bohacova, M., Boncioli, D., Bonifazi, C., Bonneau Arbeletche, L., Borodai, N., Botti, A. M., Brack, J., Bretz, T., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero-Mora, K. S., Caccianiga, L., Cancio, A., Canfora, F., Caracas, I., Carceller, J. M., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Cerda, M., Chinellato, J. A., Choi, K., Chudoba, J., Chytka, L., Clay, R. W., Cobos Cerutti, A. C., Colalillo, R., Coleman, A., Coluccia, M. R., Conceicao, R., Condorelli, A., Consolati, G., Contreras, F., Convenga, F., Covault, C. E., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., De Almeida, R. M., De Jesus, J., De Jong, S. J., De Mauro, G., De Mello Neto, J. R. T., De Mitri, I., De Oliveira, J., De Oliveira Franco, D., De Souza, V., De Vito, E., Debatin, J., Del Rio, M., Deligny, O., Dembinski, H., Dhital, N., Di Matteo, A., Dobrigkeit, C., D'Olivo, J. C., Dos Anjos, R. C., Dova, M. T., Ebr, J., Engel, R., Epicoco, I., Erdmann, M., Escobar, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Fick, B., Figueira, J. M., Filipcic, A., Fodran, T., Freire, M. M., Fujii, T., Fuster, A., Galea, C., Galelli, C., Garcia, B., Garcia Vegas, A. L., Gemmeke, H., Gesualdi, F., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., Glombitza, J., Gobbi, F., Gollan, F., Golup, G., Gomez Berisso, M., Gomez Vitale, P. F., Gongora, J. P., Gonzalez, N., Goos, I., Gora, D., Gorgi, A., Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Hahn, S., Halliday, R., Hampel, M. R., Hansen, P., Harari, D., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Hill, G. C., Hojvat, C., Horandel, J. R., Horvath, P., Hrabovsky, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Johnsen, J. A., Jurysek, J., Kaapa, A., Kampert, K. H., Keilhauer, B., Kemp, J., Klages, H. O., Kleifges, M., Kleinfeller, J., Kopke, M., Kukec Mezek, G., Lago, B. L., Lahurd, D., Lang, R. G., Langner, N., Leigui De Oliveira, M. A., Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Lo Presti, D., Lopes, L., Lopez, R., Lorek, R., Luce, Q., Lucero, A., Lundquist, J. P., Machado Payeras, A., Mancarella, G., Mandat, D., Manning, B. C., Manshanden, J., Mantsch, P., Marafico, S., Mariazzi, A. G., Maris, I. C., Marsella, G., Martello, D., Martinez, H., Martinez Bravo, O., Mastrodicasa, M., Mathes, H. J., Matthews, J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina-Tanco, G., Melo, D., Menshikov, A., Merenda, K. -D., Michal, S., Micheletti, M. I., Miramonti, L., Mollerach, S., Montanet, F., Morello, C., Mostafa, M., Muller, A. L., Muller, M. A., Mulrey, K., Mussa, R., Muzio, M., Namasaka, W. M., Nellen, L., Niculescu-Oglinzanu, M., Niechciol, M., Nitz, D., Nosek, D., Novotny, V., Nozka, L., Nucita, A., Nunez, L. A., Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Pech, M., Pedreira, F., Pkala, J., Pelayo, R., Pena-Rodriguez, J., Perez Armand, J., Perlin, M., Perrone, L., Petrera, S., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Pont, B., Pothast, M., Privitera, P., Prouza, M., Puyleart, A., Querchfeld, S., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Ristori, P., Rizi, V., Rodrigues De Carvalho, W., Rodriguez Rojo, J., Roncoroni, M. J., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Salina, G., Sanabria Gomez, J. D., Sanchez, F., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Savina, P., Schafer, C. M., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schluter, F., Schmidt, D., Scholten, O., Schovanek, P., Schroder, F. G., Schroder, S., Schulte, J., Sciutto, S. J., Scornavacche, M., Shellard, R. C., Sigl, G., Silli, G., Sima, O., Smida, R., Sommers, P., Soriano, J. F., Souchard, J., Squartini, R., Stadelmaier, M., Stanca, D., Stanic, S., Stasielak, J., Stassi, P., Streich, A., Suarez-Duran, M., Sudholz, T., Suomijarvi, T., Supanitsky, A. D., Supik, J., Szadkowski, Z., Taboada, A., Tapia, A., Timmermans, C., Tkachenko, O., Tobiska, P., Todero Peixoto, C. J., Tome, B., Torralba Elipe, G., Travaini, A., Travnicek, P., Trimarelli, C., Trini, M., Tueros, M., Ulrich, R., Unger, M., Vaclavek, L., Vacula, M., Valdes Galicia, J. F., Valino, I., Valore, L., Varela, E., Varma, K. C. V., Vasquez-Ramirez, A., Veberic, D., Ventura, C., Vergara Quispe, I. D., Verzi, V., Vicha, J., Vink, J., Vorobiov, S., Wahlberg, H., Watson, A. A., Weber, M., Weindl, A., Wiencke, L., Wilczynski, H., Winchen, T., Wirtz, M., Wittkowski, D., Wundheiler, B., Yushkov, A., Zapparrata, O., Zas, E., Zavrtanik, D., Zavrtanik, M., Zehrer, L., Zepeda, A., Astronomy, Aab A., Abreu P., Aglietta M., Albury J.M., Allekotte I., Almela A., Alvarez-Muniz J., Alves Batista R., Anastasi G.A., Anchordoqui L., Andrada B., Andringa S., Aramo C., Araujo Ferreira P.R., Asorey H., Assis P., Avila G., Badescu A.M., Bakalova A., Balaceanu A., Barbato F., Barreira Luz R.J., Becker K.H., Bellido J.A., Berat C., Bertaina M.E., Bertou X., Biermann P.L., Bister T., Biteau J., Blazek J., Bleve C., Bohacova M., Boncioli D., Bonifazi C., Bonneau Arbeletche L., Borodai N., Botti A.M., Brack J., Bretz T., Briechle F.L., Buchholz P., Bueno A., Buitink S., Buscemi M., Caballero-Mora K.S., Caccianiga L., Cancio A., Canfora F., Caracas I., Carceller J.M., Caruso R., Castellina A., Catalani F., Cataldi G., Cazon L., Cerda M., Chinellato J.A., Choi K., Chudoba J., Chytka L., Clay R.W., Cobos Cerutti A.C., Colalillo R., Coleman A., Coluccia M.R., Conceicao R., Condorelli A., Consolati G., Contreras F., Convenga F., Covault C.E., Dasso S., Daumiller K., Dawson B.R., Day J.A., De Almeida R.M., De Jesus J., De Jong S.J., De Mauro G., De Mello Neto J.R.T., De Mitri I., De Oliveira J., De Oliveira Franco D., De Souza V., De Vito E., Debatin J., Del Rio M., Deligny O., Dembinski H., Dhital N., Di Matteo A., Dobrigkeit C., D'Olivo J.C., Dos Anjos R.C., Dova M.T., Ebr J., Engel R., Epicoco I., Erdmann M., Escobar C.O., Etchegoyen A., Falcke H., Farmer J., Farrar G., Fauth A.C., Fazzini N., Feldbusch F., Fenu F., Fick B., Figueira J.M., Filipcic A., Fodran T., Freire M.M., Fujii T., Fuster A., Galea C., Galelli C., Garcia B., Garcia Vegas A.L., Gemmeke H., Gesualdi F., Gherghel-Lascu A., Ghia P.L., Giaccari U., Giammarchi M., Giller M., Glombitza J., Gobbi F., Gollan F., Golup G., Gomez Berisso M., Gomez Vitale P.F., Gongora J.P., Gonzalez N., Goos I., Gora D., Gorgi A., Gottowik M., Grubb T.D., Guarino F., Guedes G.P., Guido E., Hahn S., Halliday R., Hampel M.R., Hansen P., Harari D., Harvey V.M., Haungs A., Hebbeker T., Heck D., Hill G.C., Hojvat C., Horandel J.R., Horvath P., Hrabovsky M., Huege T., Hulsman J., Insolia A., Isar P.G., Johnsen J.A., Jurysek J., Kaapa A., Kampert K.H., Keilhauer B., Kemp J., Klages H.O., Kleifges M., Kleinfeller J., Kopke M., Kukec Mezek G., Lago B.L., Lahurd D., Lang R.G., Langner N., Leigui De Oliveira M.A., Lenok V., Letessier-Selvon A., Lhenry-Yvon I., Lo Presti D., Lopes L., Lopez R., Lorek R., Luce Q., Lucero A., Lundquist J.P., Machado Payeras A., Mancarella G., Mandat D., Manning B.C., Manshanden J., Mantsch P., Marafico S., Mariazzi A.G., Maris I.C., Marsella G., Martello D., Martinez H., Martinez Bravo O., Mastrodicasa M., Mathes H.J., Matthews J., Matthiae G., Mayotte E., Mazur P.O., Medina-Tanco G., Melo D., Menshikov A., Merenda K.-D., Michal S., Micheletti M.I., Miramonti L., Mollerach S., Montanet F., Morello C., Mostafa M., Muller A.L., Muller M.A., Mulrey K., Mussa R., Muzio M., Namasaka W.M., Nellen L., Niculescu-Oglinzanu M., Niechciol M., Nitz D., Nosek D., Novotny V., NoZka L., Nucita A., Nunez L.A., Palatka M., Pallotta J., Papenbreer P., Parente G., Parra A., Pech M., Pedreira F., Pkala J., Pelayo R., Pena-Rodriguez J., Perez Armand J., Perlin M., Perrone L., Petrera S., Pierog T., Pimenta M., Pirronello V., Platino M., Pont B., Pothast M., Privitera P., Prouza M., Puyleart A., Querchfeld S., Rautenberg J., Ravignani D., Reininghaus M., Ridky J., Riehn F., Risse M., Ristori P., Rizi V., Rodrigues De Carvalho W., Rodriguez Rojo J., Roncoroni M.J., Roth M., Roulet E., Rovero A.C., Ruehl P., Saffi S.J., Saftoiu A., Salamida F., Salazar H., Salina G., Sanabria Gomez J.D., Sanchez F., Santos E.M., Santos E., Sarazin F., Sarmento R., Sarmiento-Cano C., Sato R., Savina P., Schafer C.M., Scherini V., Schieler H., Schimassek M., Schimp M., Schluter F., Schmidt D., Scholten O., Schovanek P., Schroder F.G., Schroder S., Schulte J., Sciutto S.J., Scornavacche M., Shellard R.C., Sigl G., Silli G., Sima O., Smida R., Sommers P., Soriano J.F., Souchard J., Squartini R., Stadelmaier M., Stanca D., Stanic S., Stasielak J., Stassi P., Streich A., Suarez-Duran M., Sudholz T., Suomijarvi T., Supanitsky A.D., Supik J., Szadkowski Z., Taboada A., Tapia A., Timmermans C., Tkachenko O., Tobiska P., Todero Peixoto C.J., Tome B., Torralba Elipe G., Travaini A., Travnicek P., Trimarelli C., Trini M., Tueros M., Ulrich R., Unger M., Vaclavek L., Vacula M., Valdes Galicia J.F., Valino I., Valore L., Varela E., Varma K. C. V., Vasquez-Ramirez A., Veberic D., Ventura C., Vergara Quispe I.D., Verzi V., Vicha J., Vink J., Vorobiov S., Wahlberg H., Watson A.A., Weber M., Weindl A., Wiencke L., Wilczynski H., Winchen T., Wirtz M., Wittkowski D., Wundheiler B., Yushkov A., Zapparrata O., Zas E., Zavrtanik D., Zavrtanik M., Zehrer L., and Zepeda A.

Subjects
interaction: model, Physics::Instrumentation and Detectors, Astronomy, Hadron, General Physics and Astronomy, Ultra-high energy cosmic rays, muons properties, hadronic models, 01 natural sciences, cosmic ray, particle interaction, astroparticle detectors, Auger, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), iron, surface [detector], Observatory, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Physics, 4. Education, Settore FIS/01 - Fisica Sperimentale, measured [fluctuation], model [interaction], Astrophysics::Instrumentation and Methods for Astrophysics, model: hadronic, fluctuation: measured, 3. Good health, observatory, Sciences exactes et naturelles, atmosphere [showers], model [particle], air, Cherenkov counter: water, Astrophysics::High Energy Astrophysical Phenomena, UHE [cosmic radiation], FOS: Physical sciences, Cosmic ray, detector: fluorescence, Nuclear physics, cosmic rays, muon, 0103 physical sciences, calorimeter, ddc:530, 14. Life underwater, cosmic radiation: UHE, High Energy Physics, distribution function, electromagnetic component, 010306 general physics, Astrophysique, Pierre Auger Observatory, fluorescence [detector], Muon, showers: atmosphere, hep-ex, detector: surface, water [Cherenkov counter], particle: model, Small deviations, Física, ASTROFÍSICA, Air shower, Experimental High Energy Physics, Elementary Particles and Fields, hadronic [model], High Energy Physics::Experiment
Abstract

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargue. We are very grateful to the following agencies and organizations for financial support: Argentina-Comision Nacional de Energia Atomica, Agencia Nacional de Promocion Cientifica y Tecnologica (ANPCyT), Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET), Gobierno de la Provincia de Mendoza, Municipalidad de Malargue, NDM Holdings and Valle Las Lenas; in gratitude for their continuing cooperation over land access; Australia-the Australian Research Council; BrazilConselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq), Financiadora de Estudos e Projetos (FINEP), Fundacao de Amparo a Pesquisa do Estado de Rio de Janeiro (FAPERJ), Sao Paulo Research Foundation (FAPESP) Grants No. 2019/10151-2, No. 2010/07359-6, and No. 1999/05404-3, Ministerio da Ciencia, Tecnologia, Inovacoes e Comunicacoes (MCTIC); Ministry of Education, Youth and Sports of the Czech RepublicGrants No. MSMT CR LTT18004, No. LM2015038, No. LM2018102, No. CZ.02.1.01/0.0/0.0/16_013/0001402, No. CZ.02.1.01/0.0/0.0/18_046/0016010, and No. CZ.02.1.01/0.0/0.0/17_049/0008422; France-Centre de Calcul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), Conseil Regional Ile-de-France, Departement Physique Nucl ' eaire et Corpusculaire (PNC-IN2P3/CNRS), Departement Sciences de l'Univers (SDU-INSU/CNRS), Institut Lagrange de Paris (ILP) Grant No. LABEX ANR-10-LABX-63 within the Investissements d'Avenir Programme Grant No. ANR11-IDEX-0004-02; Germany-Bundesministerium fur Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Finanzministerium Baden-Wurttemberg, Helmholtz Alliance for Astroparticle Physics (HAP), Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF), Ministerium fur Innovation, Wissenschaft und Forschung des Landes Nordrhein-Westfalen, Ministerium fur Wissenschaft, Forschung und Kunst des Landes Baden-Wurttemberg; Italy-Istituto Nazionale di Fisica Nucleare (INFN), Istituto Nazionale di Astrofisica (INAF), Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR), CETEMPS Center of Excellence, Ministero degli Affari Esteri (MAE); Mexico-Consejo Nacional de Ciencia y Tecnologia (CONACYT) Grant No. 167733, Universidad Nacional Autonoma de Mexico (UNAM), PAPIIT DGAPA-UNAM; The Netherlands-Ministry of Education, Culture and Science, Netherlands Organisation for Scientific Research (NWO), Dutch national e-infrastructure with the support of SURF Cooperative; Poland-Ministry of Science and Higher Education, Grant No. DIR/WK/2018/11, National Science Centre, Grants No. 2013/08/M/ST9/00322, No. 2016/23/B/ST9/01635, and No. HARMONIA 5-2013/10/M/ST9/00062, UMO-2016/22/M/ST9/00198; Portugal -Portuguese national funds and FEDER funds within Programa Operacional Factores de Competitividade through Fundacao para a Ciencia e a Tecnologia (COMPETE); Romania-Romanian Ministry of Education and Research, the Program Nucleu within MCI (PN19150201/16N/2019 and PN19060102), and project PN-III-P1-1.2-PCCDI-2017-0839/19PCCDI/2018 within PNCDI III; Slovenia-Slovenian Research Agency, Grants No. P1-0031, No. P1-0385, No. I00033, No. N1-0111; Spain-Ministerio de Economia, Industria y Competitividad (FPA2017-85114-P and FPA2017-85197-P), Xunta de Galicia (ED431C 2017/07), Junta de Andalucia (SOMM17/6104/UGR), Feder Funds, RENATA Red Nacional Tematica de Astroparticulas (FPA2015-68783-REDT), and Maria de Maeztu Unit of Excellence (MDM-2016-0692); U.S.Department of Energy, Awards No. DE-AC0207CH11359, No. DE-FR02-04ER41300, No. DE-FG0299ER41107, and No. DE-SC0011689, National Science Foundation, Grant No. 0450696, The Grainger Foundation, Marie Curie-IRSES/EPLANET, European Particle Physics Latin American Network, and UNESCO., We present the first measurement of the fluctuations in the number of muons in extensive air showers produced by ultrahigh energy cosmic rays. We find that the measured fluctuations are in good agreement with predictions from air shower simulations. This observation provides new insights into the origin of the previously reported deficit of muons in air shower simulations and constrains models of hadronic interactions at ultrahigh energies. Our measurement is compatible with the muon deficit originating from small deviations in the predictions from hadronic interaction models of particle production that accumulate as the showers develop., Argentina-Comision Nacional de Energia Atomica, ANPCyT, Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET), Gobierno de la Provincia de Mendoza, Municipalidad de Malargue, NDM Holdings, Valle Las Lenas, Australian Research Council, Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPQ), Fundacao de Apoio a Pesquisa do Distrito Federal (FAPDF), Financiadora de Inovacao e Pesquisa (Finep), Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio De Janeiro (FAPERJ), Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP) 2019/10151-2 2010/07359-6 1999/05404-3, Ministerio da Ciencia, Tecnologia, Inovacoes e Comunicacoes (MCTIC), Ministry of Education, Youth & Sports - Czech Republic MSMT CR LTT18004 LM2015038 LM2018102 CZ.02.1.01/0.0/0.0/16_013/0001402 CZ.02.1.01/0.0/0.0/18_046/0016010 CZ.02.1.01/0.0/0.0/17_049/0008422, France-Centre de Calcul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), Region Ile-de-France, Departement Sciences de l'Univers (SDU-INSU/CNRS), French National Research Agency (ANR) LABEX ANR-10-LABX-63 ANR11-IDEX-0004-02, Federal Ministry of Education & Research (BMBF), German Research Foundation (DFG), Finanzministerium Baden-Wurttemberg, Helmholtz Alliance for Astroparticle Physics (HAP), Helmholtz Association, Ministerium fur Innovation, Wissenschaft und Forschung des Landes Nordrhein-Westfalen, Ministerium fur Wissenschaft, Forschung und Kunst des Landes Baden-Wurttemberg, Italy-Istituto Nazionale di Fisica Nucleare (INFN), Istituto Nazionale Astrofisica (INAF), Ministry of Education, Universities and Research (MIUR), CETEMPS Center of Excellence, Ministry of Foreign Affairs and International Cooperation (Italy), Consejo Nacional de Ciencia y Tecnologia (CONACyT) 167733, Universidad Nacional Autonoma de Mexico (UNAM), PAPIIT DGAPA-UNAM, Netherlands-Ministry of Education, Culture and Science, Netherlands Organization for Scientific Research (NWO), Dutch national e-infrastructure, SURF Cooperative, Poland-Ministry of Science and Higher Education DIR/WK/2018/11, National Science Centre, Poland 2013/08/M/ST9/00322 2016/23/B/ST9/01635 HARMONIA 5-2013/10/M/ST9/00062 UMO-2016/22/M/ST9/00198, Portugal -Portuguese national funds, FEDER funds within Programa Operacional Factores de Competitividade through Fundacao para a Ciencia e a Tecnologia (COMPETE), Romania-Romanian Ministry of Education and Research, the Program Nucleu within MCI PN19150201/16N/2019 PN19060102, Romania-Romanian Ministry of Educatio n and Research, the Program Nucleu within PNCDI III PN-III-P1-1.2-PCCDI-2017-0839/19PCCDI/2018, Slovenian Research Agency - Slovenia P1-0031 P1-0385 I00033 N1-0111, Spain-Ministerio de Economia, Industria y Competitividad FPA2017-85114-P FPA2017-85197-P, Xunta de Galicia European Commission ED431C 2017/07, Junta de Andalucia SOMM17/6104/UGR, European Commission, RENATA Red Nacional Tematica de Astroparticulas FPA2015-68783-REDT, Maria de Maeztu Unit of Excellence MDM-2016-0692, United States Department of Energy (DOE) DE-AC0207CH11359 DE-FR02-04ER41300 DE-FG0299ER41107 DE-SC0011689, National Science Foundation (NSF) 0450696, Grainger Foundation, Marie Curie-IRSES/EPLANET, European Particle Physics Latin American Network, UNESCO

Published
2021

23. Design, upgrade and characterization of the silicon photomultiplier front-end for the AMIGA detector at the Pierre Auger Observatory

Author

Silvia Mollerach, N. Fazzini, Jonas Glombitza, F. C. T. Barbato, D. Zavrtanik, Serguei Vorobiov, J. Kleinfeller, Marcos Cerda, Denis Stanca, D. Melo, W. M. Namasaka, L. Lopes, A. C. Rovero, Alexandru Balaceanu, Carla Aramo, Julien Souchard, D. Martello, O. Martínez Bravo, K. Mulrey, Carla Bleve, Rodrigo Guedes Lang, Jaime Alvarez-Muñiz, Kevin-Druis Merenda, Alexandru Gherghel-Lascu, E. Santos, Thomas Bretz, Tiina Suomijarvi, V. Rizi, Corbin Covault, Vladimir Lenok, J. Stasielak, P. Tobiska, L. Perrone, L. Valore, R. Sato, Lino Miramonti, D. de Oliveira Franco, Lukáš Vaclavek, G. Mancarella, G. Marsella, A. Weindl, P. Savina, W. Rodrigues de Carvalho, Teresa Bister, Dalibor Nosek, M. Schimp, B. C. Manning, G. P. Guedes, Bjarni Pont, Luis A. Anchordoqui, A. Di Matteo, Marvin Gottowik, B. Keilhauer, P. Abreu, D. Ravignani, Alessio Gorgi, Maximilian Reininghaus, Flavia Gesualdi, Dusan Mandat, Sullivan Marafico, M. Risse, Orazio Zapparrata, Francesco Fenu, Ralf Ulrich, B. Wundheiler, Paul Sommers, Patricia María Hansen, Philipp Papenbreer, E. M. Santos, Eric Mayotte, Toshihiro Fujii, S. J. Sciutto, Juan Miguel Carceller, David Schmidt, J. Perez Armand, M. Gómez Berisso, S. Schröder, Italo Epicoco, Kai Daumiller, F. Sánchez, Marco Giammarchi, Nataliia Borodai, Christian Sarmiento-Cano, G. Parente, Fabrizia Canfora, K. Choi, L. Zehrer, Miroslav Pech, M. Pothast, Valerio Pirronello, C. J.W.P. Timmermans, C. M. Schäfer, C. J. Todero Peixoto, J. F. Valdés Galicia, I. De Mitri, Denise Boncioli, Jakub Juryšek, J. Debatin, Antonio Condorelli, Carola Dobrigkeit, M. Muzio, J. de Oliveira, Martin Vacula, Marcel Köpke, M. Platino, R. Alves Batista, Bruce R. Dawson, Trent D. Grubb, D. Nitz, Alejandro Almela, P. Horvath, J. Chudoba, P.O. Mazur, Darko Veberič, Julian Kemp, B. Andrada, A.L. Garcia Vegas, Sofia Andringa, M. A. Muller, A. Aab, G. Cataldi, Michael Prouza, Fred Sarazin, F. Riehn, T. Huege, Marina Scornavacche, A. Tapia, B. Tome, Josina Schulte, Alex Kääpä, Martina Bohacova, L. Nožka, G. De Mauro, F. Guarino, John Matthews, Peter Buchholz, Steffen Hahn, Claudio Galelli, Juan Carlos D'Olivo, T. Pierog, Juan Manuel Figueira, Mario Buscemi, L. R. Wiencke, Niklas Langner, Roberta Colalillo, Heino Falcke, V. Scherini, Maria Rita Coluccia, Jeffrey Brack, Olaf Scholten, Octavian Sima, Marco Aglietta, Marko Zavrtanik, H. Schieler, Esteban Roulet, A. G. Mariazzi, Justin M. Albury, Humberto Ibarguen Salazar, Hernán Asorey, M. I. Micheletti, Karl-Heinz Kampert, Antonella Castellina, Jonathan Biteau, J. Vicha, G. Farrar, Juan Pablo Gongora, K.-H. Becker, Nicolás González, Jose Chinellato, Alan Watson, H. Wilczyński, M. Suárez-Durán, Xavier Bertou, M. Perlin, Matias Tueros, Mihai Niculescu-Oglinzanu, M. Pimenta, I. Lhenry-Yvon, Jiri Blazek, E. De Vito, Giovanni Consolati, A. Zepeda, Gaetano Salina, Violet M. Harvey, D. Harari, Luis A. Nunez, Pedro Assis, P.R. Araújo Ferreira, Brian Fick, Piera Luisa Ghia, D. Lo Presti, S. J. De Jong, C. O. Escobar, A. Insolia, M. Kleifges, A.D. Supanitsky, H. Martinez, A. Etchegoyen, Marcus Niechciol, A. Taboada, J. Pȩkala, A. Fuster, Miguel Mostafa, Frank G. Schröder, Jarryd A. Day, A. Saftoiu, R.J. Barreira Luz, Tobias Winchen, Julien Manshanden, R. Conceição, A. Puyleart, Corinne Berat, M. Giller, Petr Schovanek, A.C. Cobos Cerutti, P.F. Gómez Vitale, Alina Mihaela Badescu, S. Querchfeld, Andres Travaini, E. Varela, J.D. Sanabria Gomez, Olena Tkachenko, V. Novotny, Ioana Caracas, Cristina Galea, J. R. T. de Mello Neto, L. Bonneau Arbeletche, A. Haungs, Rossella Caruso, A. Lucero, Fernando Catalani, J. Šupík, Carlo Ventura, Florian Lukas Briechle, Massimo Mastrodicasa, P. Ruehl, M. Schimassek, Caterina Trimarelli, Alena Bakalova, C. Hojvat, Jan Ebr, Ladislav Chytka, Samo Stanič, M. E. Bertaina, Markus Roth, M. HrabovskÃ, Jon Paul Lundquist, A. Menshikov, J. Hulsman, Juan Manuel González, P. Mantsch, B. L. Lago, P. Travnicek, Jacco Vink, H. Gemmeke, M. Unger, Jeffrey A. Johnsen, Z. Szadkowski, Gaia Silli, Isabel Goos, R. Squartini, A. Filipčič, D. Heck, Alfred Müller, H.O. Klages, Thomas Hebbeker, Sergio Dasso, Tristan Sudholz, S. Petrera, Marc Weber, A. Letessier-Selvon, Paula Gina Isar, M. del Río, Günter Sigl, Martín Miguel Freire, Roberto Mussa, P. Stassi, Radomir Smida, G. Medina-Tanco, A. A. Nucita, J. Rautenberg, A. Machado Payeras, B. García, R.C. Shellard, Q. Luce, F. Salamida, Maximilian Stadelmaier, R. López, Karen S. Caballero-Mora, R. M. de Almeida, A. Yushkov, Lorenzo Caccianiga, Lorenzo Cazon, G. Golup, Rodrigo Pelayo, Stijn Buitink, Martin Erdmann, François Montanet, J. de Jesús, A. Streich, Gioacchino Alex Anastasi, M. Wirtz, Eleonora Guido, Valerio Verzi, L. Nellen, Roger W Clay, Fernando Gollan, C. Morello, V. de Souza, Peter L. Biermann, Paolo Privitera, David Wittkowski, Olivier Deligny, Tomáš Fodran, Ugo Giaccari, Ioana Codrina Maris, A. C. Fauth, Carla Bonifazi, Jose A. Bellido, Fabio Convenga, G. C. Hill, I.D. Vergara Quispe, Jorge F. Soriano, Hernan Wahlberg, Ralph Engel, A. Parra, P. Ristori, M. Trini, I. Allekotte, M. J. Roncoroni, J. Pallotta, J. Ridky, A. M. Botti, Jörg R. Hörandel, H. J. Mathes, Stanislav Michal, J. Rodriguez Rojo, G. Matthiae, Fridtjof Feldbusch, Enrique Zas, Antonio Bueno, Fernando Contreras, Gualberto Avila, Dariusz Gora, John Farmer, Alan Coleman, Maria-Teresa Dova, M. R. Hampel, S. J. Saffi, F. Pedreira, Raul Sarmento, R.C. dos Anjos, Felix Schlüter, Adriana Vásquez-Ramírez, M. Palatka, Fabian Gobbi, Jesús Peña-Rodríguez, M.A. Leigui de Oliveira, High Energy Astrophys. & Astropart. Phys (API, FNWI), Aab, A., Abreu, P., Aglietta, M., Albury, J. M., Allekotte, I., Almela, A., Alvarez-Muniz, J., Alves Batista, R., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Araujo Ferreira, P. R., Asorey, H., Assis, P., Avila, G., Badescu, A. M., Bakalova, A., Balaceanu, A., Barbato, F., Barreira Luz, R. J., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Bister, T., Biteau, J., Blazek, J., Bleve, C., Bohacova, M., Boncioli, D., Bonifazi, C., Bonneau Arbeletche, L., Borodai, N., Botti, A. M., Brack, J., Bretz, T., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero-Mora, K. S., Caccianiga, L., Canfora, F., Caracas, I., Carceller, J. M., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Cerda, M., Chinellato, J. A., Choi, K., Chudoba, J., Chytka, L., Clay, R. W., Cobos Cerutti, A. C., Colalillo, R., Coleman, A., Coluccia, M. R., Conceicao, R., Condorelli, A., Consolati, G., Contreras, F., Convenga, F., Covault, C. E., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., de Almeida, R. M., de Jesus, J., de Jong, S. J., de Mauro, G., de Mello Neto, J. R. T., de Mitri, I., de Oliveira, J., de Oliveira Franco, D., de Souza, V., de Vito, E., Debatin, J., del Rio, M., Deligny, O., Di Matteo, A., Dobrigkeit, C., D'Olivo, J. C., dos Anjos, R. C., Dova, M. T., Ebr, J., Engel, R., Epicoco, I., Erdmann, M., Escobar, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Fick, B., Figueira, J. M., Filipcic, A., Fodran, T., Freire, M. M., Fujii, T., Fuster, A., Galea, C., Galelli, C., Garcia, B., Garcia Vegas, A. L., Gemmeke, H., Gesualdi, F., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., Glombitza, J., Gobbi, F., Gollan, F., Golup, G., Gomez Berisso, M., Gomez Vitale, P. F., Gongora, J. P., Gonzalez, J. M., Gonzalez, N., Goos, I., Gora, D., Gorgi, A., Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Hahn, S., Hampel, M. R., Hansen, P., Harari, D., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Hill, G. C., Hojvat, C., Horandel, J. R., Horvath, P., Hrabovsky, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Johnsen, J. A., Jurysek, J., Kaapa, A., Kampert, K. H., Keilhauer, B., Kemp, J., Klages, H. O., Kleifges, M., Kleinfeller, J., Kopke, M., Lago, B. L., Lang, R. G., Langner, N., Leigui de Oliveira, M. A., Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Lo Presti, D., Lopes, L., Lopez, R., Luce, Q., Lucero, A., Lundquist, J. P., Machado Payeras, A., Mancarella, G., Mandat, D., Manning, B. C., Manshanden, J., Mantsch, P., Marafico, S., Mariazzi, A. G., Maris, I. C., Marsella, G., Martello, D., Martinez, H., Martinez Bravo, O., Mastrodicasa, M., Mathes, H. J., Matthews, J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina-Tanco, G., Melo, D., Menshikov, A., Merenda, K. -D., Michal, S., Micheletti, M. I., Miramonti, L., Mollerach, S., Montanet, F., Morello, C., Mostafa, M., Muller, A. L., Muller, M. A., Mulrey, K., Mussa, R., Muzio, M., Namasaka, W. M., Nellen, L., Niculescu-Oglinzanu, M., Niechciol, M., Nitz, D., Nosek, D., Novotny, V., Nozka, L., Nucita, A., Nunez, L. A., Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Pech, M., Pedreira, F., Pekala, J., Pelayo, R., Pena-Rodriguez, J., Perez Armand, J., Perlin, M., Perrone, L., Petrera, S., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Pont, B., Pothast, M., Privitera, P., Prouza, M., Puyleart, A., Querchfeld, S., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Ristori, P., Rizi, V., Rodrigues de Carvalho, W., Rodriguez Rojo, J., Roncoroni, M. J., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Salina, G., Sanabria Gomez, J. D., Sanchez, F., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Savina, P., Schafer, C. M., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schluter, F., Schmidt, D., Scholten, O., Schovanek, P., Schroder, F. G., Schroder, S., Schulte, J., Sciutto, S. J., Scornavacche, M., Shellard, R. C., Sigl, G., Silli, G., Sima, O., Smida, R., Sommers, P., Soriano, J. F., Souchard, J., Squartini, R., Stadelmaier, M., Stanca, D., Stanic, S., Stasielak, J., Stassi, P., Streich, A., Suarez-Duran, M., Sudholz, T., Suomijarvi, T., Supanitsky, A. D., Supik, J., Szadkowski, Z., Taboada, A., Tapia, A., Timmermans, C., Tkachenko, O., Tobiska, P., Todero Peixoto, C. J., Tome, B., Travaini, A., Travnicek, P., Trimarelli, C., Trini, M., Tueros, M., Ulrich, R., Unger, M., Vaclavek, L., Vacula, M., Valdes Galicia, J. F., Valore, L., Varela, E., Varma, V. K. C., Vasquez-Ramirez, A., Veberic, D., Ventura, C., Vergara Quispe, I. D., Verzi, V., Vicha, J., Vink, J., Vorobiov, S., Wahlberg, H., Watson, A. A., Weber, M., Weindl, A., Wiencke, L., Wilczynski, H., Winchen, T., Wirtz, M., Wittkowski, D., Wundheiler, B., Yushkov, A., Zapparrata, O., Zas, E., Zavrtanik, D., Zavrtanik, M., Zehrer, L., Zepeda, A., Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Institut de Physique Nucléaire d'Orsay (IPNO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Pierre Auger, Physics, Aab A., Abreu P., Aglietta M., Albury J.M., Allekotte I., Almela A., Alvarez-Muniz J., Alves Batista R., Anastasi G.A., Anchordoqui L., Andrada B., Andringa S., Aramo C., Araujo Ferreira P.R., Asorey H., Assis P., Avila G., Badescu A.M., Bakalova A., Balaceanu A., Barbato F., Barreira Luz R.J., Becker K.H., Bellido J.A., Berat C., Bertaina M.E., Bertou X., Biermann P.L., Bister T., Biteau J., Blazek J., Bleve C., Bohacova M., Boncioli D., Bonifazi C., Bonneau Arbeletche L., Borodai N., Botti A.M., Brack J., Bretz T., Briechle F.L., Buchholz P., Bueno A., Buitink S., Buscemi M., Caballero-Mora K.S., Caccianiga L., Canfora F., Caracas I., Carceller J.M., Caruso R., Castellina A., Catalani F., Cataldi G., Cazon L., Cerda M., Chinellato J.A., Choi K., Chudoba J., Chytka L., Clay R.W., Cobos Cerutti A.C., Colalillo R., Coleman A., Coluccia M.R., Conceicao R., Condorelli A., Consolati G., Contreras F., Convenga F., Covault C.E., Dasso S., Daumiller K., Dawson B.R., Day J.A., de Almeida R.M., de Jesus J., de Jong S.J., de Mauro G., de Mello Neto J.R.T., de Mitri I., de Oliveira J., de Oliveira Franco D., de Souza V., de Vito E., Debatin J., del Rio M., Deligny O., Di Matteo A., Dobrigkeit C., D'Olivo J.C., dos Anjos R.C., Dova M.T., Ebr J., Engel R., Epicoco I., Erdmann M., Escobar C.O., Etchegoyen A., Falcke H., Farmer J., Farrar G., Fauth A.C., Fazzini N., Feldbusch F., Fenu F., Fick B., Figueira J.M., Filipcic A., Fodran T., Freire M.M., Fujii T., Fuster A., Galea C., Galelli C., Garcia B., Garcia Vegas A.L., Gemmeke H., Gesualdi F., Gherghel-Lascu A., Ghia P.L., Giaccari U., Giammarchi M., Giller M., Glombitza J., Gobbi F., Gollan F., Golup G., Gomez Berisso M., Gomez Vitale P.F., Gongora J.P., Gonzalez J.M., Gonzalez N., Goos I., Gora D., Gorgi A., Gottowik M., Grubb T.D., Guarino F., Guedes G.P., Guido E., Hahn S., Hampel M.R., Hansen P., Harari D., Harvey V.M., Haungs A., Hebbeker T., Heck D., Hill G.C., Hojvat C., Horandel J.R., Horvath P., Hrabovsky M., Huege T., Hulsman J., Insolia A., Isar P.G., Johnsen J.A., Jurysek J., Kaapa A., Kampert K.H., Keilhauer B., Kemp J., Klages H.O., Kleifges M., Kleinfeller J., Kopke M., Lago B.L., Lang R.G., Langner N., Leigui de Oliveira M.A., Lenok V., Letessier-Selvon A., Lhenry-Yvon I., Lo Presti D., Lopes L., Lopez R., Luce Q., Lucero A., Lundquist J.P., Machado Payeras A., Mancarella G., Mandat D., Manning B.C., Manshanden J., Mantsch P., Marafico S., Mariazzi A.G., Maris I.C., Marsella G., Martello D., Martinez H., Martinez Bravo O., Mastrodicasa M., Mathes H.J., Matthews J., Matthiae G., Mayotte E., Mazur P.O., Medina-Tanco G., Melo D., Menshikov A., Merenda K.-D., Michal S., Micheletti M.I., Miramonti L., Mollerach S., Montanet F., Morello C., Mostafa M., Muller A.L., Muller M.A., Mulrey K., Mussa R., Muzio M., Namasaka W.M., Nellen L., Niculescu-Oglinzanu M., Niechciol M., Nitz D., Nosek D., Novotny V., Nozka L., Nucita A., Nunez L.A., Palatka M., Pallotta J., Papenbreer P., Parente G., Parra A., Pech M., Pedreira F., Pekala J., Pelayo R., Pena-Rodriguez J., Perez Armand J., Perlin M., Perrone L., Petrera S., Pierog T., Pimenta M., Pirronello V., Platino M., Pont B., Pothast M., Privitera P., Prouza M., Puyleart A., Querchfeld S., Rautenberg J., Ravignani D., Reininghaus M., Ridky J., Riehn F., Risse M., Ristori P., Rizi V., Rodrigues de Carvalho W., Rodriguez Rojo J., Roncoroni M.J., Roth M., Roulet E., Rovero A.C., Ruehl P., Saffi S.J., Saftoiu A., Salamida F., Salazar H., Salina G., Sanabria Gomez J.D., Sanchez F., Santos E.M., Santos E., Sarazin F., Sarmento R., Sarmiento-Cano C., Sato R., Savina P., Schafer C.M., Scherini V., Schieler H., Schimassek M., Schimp M., Schluter F., Schmidt D., Scholten O., Schovanek P., Schroder F.G., Schroder S., Schulte J., Sciutto S.J., Scornavacche M., Shellard R.C., Sigl G., Silli G., Sima O., Smida R., Sommers P., Soriano J.F., Souchard J., Squartini R., Stadelmaier M., Stanca D., Stanic S., Stasielak J., Stassi P., Streich A., Suarez-Duran M., Sudholz T., Suomijarvi T., Supanitsky A.D., Supik J., Szadkowski Z., Taboada A., Tapia A., Timmermans C., Tkachenko O., Tobiska P., Todero Peixoto C.J., Tome B., Travaini A., Travnicek P., Trimarelli C., Trini M., Tueros M., Ulrich R., Unger M., Vaclavek L., Vacula M., Valdes Galicia J.F., Valore L., Varela E., Varma V.K.C., Vasquez-Ramirez A., Veberic D., Ventura C., Vergara Quispe I.D., Verzi V., Vicha J., Vink J., Vorobiov S., Wahlberg H., Watson A.A., Weber M., Weindl A., Wiencke L., Wilczynski H., Winchen T., Wirtz M., Wittkowski D., Wundheiler B., Yushkov A., Zapparrata O., Zas E., Zavrtanik D., Zavrtanik M., Zehrer L., Zepeda A., and Research unit Astroparticle Physics

Subjects
Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, Astronomy, Performance of High Energy Physics Detector, 01 natural sciences, 7. Clean energy, Etc), 030218 nuclear medicine & medical imaging, 0302 clinical medicine, Front-end electronics for detector readout, APDs, Instrumentation, physics.ins-det, Photon detectors for UV, Mathematical Physics, Instrumentation et méthodes en physique, EBCCDs, Visible and IR photons (solid-state) (PIN diodes, APDs, Si-PMTs, G-APDs, CCDs, EBCCDs, EMCCDs, CMOS imagers, etc), electronics, Settore FIS/01 - Fisica Sperimentale, Calibration and fitting methods, Performance of High Energy Physics Detectors, Photon detectors for UV, visible and IR photons (solid-state) (PIN diodes, APDs, Si-PMTs, G-APDs, CCDs, EBCCDs, EMCCDs, CMOS imagers, etc), Astrophysics::Instrumentation and Methods for Astrophysics, Si-PMTs, Instrumentation and Detectors (physics.ins-det), charged particle, CCDs, Cluster finding, CMOS imagers, EMCCDs, Pattern recognition, G-APDs, Visible and IR photons (solid-state) (PIN diodes, Auger, observatory, density [muon], Pattern recognition, cluster finding, calibration and fitting method, Christian ministry, upgrade, ddc:620, Astrophysics - Instrumentation and Methods for Astrophysics, performance, atmosphere [showers], Land access, Cherenkov counter: water, air, Astrophysics::High Energy Astrophysical Phenomena, UHE [cosmic radiation], FOS: Physical sciences, 03 medical and health sciences, Political science, 0103 physical sciences, muon: density, photomultiplier: silicon, High Energy Physics, cosmic radiation: UHE, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], ddc:610, Instrumentation and Methods for Astrophysics (astro-ph.IM), Engineering & allied operations, scintillation counter, showers: atmosphere, 010308 nuclear & particles physics, water [Cherenkov counter], Autres mathématiques, Research council, efficiency, Experimental High Energy Physics, silicon [photomultiplier], High Energy Physics::Experiment, Humanities, RAIOS CÓSMICOS, astro-ph.IM
Abstract

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargue. We are very grateful to the following agencies and organizations for financial support: Argentina -Comision Nacional de Energia Atomica; Agencia Nacional de Promocion Cientifica y Tecnologica (ANPCyT); Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET); Gobierno de la Provincia de Mendoza; Municipalidad de Malargue; NDM Holdings and Valle Las Lenas; in gratitude for their continuing cooperation over land access; Australia -the Australian Research Council; Brazil -Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq); Financiadora de Estudos e Projetos (FINEP); Fundacao de Amparo a Pesquisa do Estado de Rio de Janeiro (FAPERJ); Sao Paulo Research Foundation (FAPESP) Grants No. 2019/10151-2, No. 2010/07359-6 and No. 1999/05404-3; Ministerio da Ciencia, Tecnologia, Inovacoes e Comunicacoes (MCTIC); Czech Republic Grant No. MSMT CR LTT18004, LM2015038, LM2018102, CZ.02.1.01/0.0/0.0/16_013/0001402, CZ.02.1.01/0.0/0.0/18_046/0016010 and CZ.02.1.01/0.0/0.0/17_049/0008422; France -Centre de Calcul IN2P3/CNRS; Centre National de la Recherche Scientifique (CNRS); Conseil Regional Ile-de-France; Departement Physique Nucleaire et Corpusculaire (PNC-IN2P3/CNRS); Departement Sciences de l'Univers (SDU-INSU/CNRS); Institut Lagrange de Paris (ILP) Grant No. LABEX ANR-10-LABX-63 within the Investissements d'Avenir Programme Grant No. ANR-11-IDEX-0004-02; Germany-Bundesministerium fur Bildung und Forschung (BMBF); Deutsche Forschungsgemeinschaft (DFG); Finanzministerium Baden-Wurttemberg; Helmholtz Alliance for Astroparticle Physics (HAP); Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF); Ministerium fur Innovation, Wissenschaft und Forschung des Landes Nordrhein-Westfalen; Ministerium fur Wissenschaft, Forschung und Kunst des Landes Baden-Wurttemberg; Italy-Istituto Nazionale di Fisica Nucleare (INFN); Istituto Nazionale di Astrofisica (INAF); Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR); CETEMPS Center of Excellence; Ministero degli Affari Esteri (MAE); Mexico-Consejo Nacional de Ciencia y Tecnologia (CONACYT) No. 167733; Universidad Nacional Autonoma de Mexico (UNAM); PAPIIT DGAPA-UNAM; The Netherlands -Ministry of Education, Culture and Science; Netherlands Organisation for Scientific Research (NWO); Dutch national e-infrastructure with the support of SURF Cooperative; Poland-Ministry of Science and Higher Education, grant No. DIR/WK/2018/11; National Science Centre, Grants No. 2013/08/M/ST9/00322, No. 2016/23/B/ST9/01635 and No. HARMONIA 5-2013/10/M/ST9/00062, UMO-2016/22/M/ST9/00198; Portugal -Portuguese national funds and FEDER funds within Programa Operacional Factores de Competitividade through Fundacao para a Ciencia e a Tecnologia (COMPETE); Romania-Romanian Ministry of Education and Research, the Program Nucleu within MCI(PN19150201/16N/2019 and PN19060102) and project PN-III-P1-1.2-PCCDI-2017-0839/19PCCDI/2018 within PNCDI III; Slovenia -Slovenian Research Agency, grants P1-0031, P1-0385, I0-0033, N1-0111; Spain-Ministerio de Economia, Industria y Competitividad (FPA2017-85114-P and FPA2017-85197-P), Xunta de Galicia (ED431C 2017/07), Junta de Andalucia (SOMM17/6104/UGR), Feder Funds, RENATA Red Nacional Tematica de Astroparticulas (FPA2015-68783-REDT) and Maria de Maeztu Unit of Excellence (MDM-2016-0692); U.S.A. -Department of Energy, Contracts No. DE-AC02-07CH11359, No. DE-FR02-04ER41300, No. DE-FG02-99ER41107 and No. DE-SC0011689; National Science Foundation, Grant No. 0450696; The Grainger Foundation; Marie Curie-IRSES/EPLANET; European Particle Physics Latin American Network; and UNESCO., AMIGA (Auger Muons and Infill for the Ground Array) is an upgrade of the Pierre Auger Observatory to complement the study of ultra-high-energy cosmic rays (UHECR) by measuring the muon content of extensive air showers (EAS). It consists of an array of 61 water Cherenkov detectors on a denser spacing in combination with underground scintillation detectors used for muon density measurement. Each detector is composed of three scintillation modules, with 10 m(2) detection area per module, buried at 2.3 m depth, resulting in a total detection area of 30 m(2). Silicon photomultiplier sensors (SiPM) measure the amount of scintillation light generated by charged particles traversing the modules. In this paper, the design of the front-end electronics to process the signals of those SiPMs and test results from the laboratory and from the Pierre Auger Observatory are described. Compared to our previous prototype, the new electronics shows a higher performance, higher efficiency and lower power consumption, and it has a new acquisition system with increased dynamic range that allows measurements closer to the shower core. The new acquisition system is based on the measurement of the total charge signal that the muonic component of the cosmic ray shower generates in the detector., Argentina - Comision Nacional de Energia Atomica, Argentina - Agencia Nacional de Promocion Cientifica y Tecnologica (ANPCyT), Argentina - Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET), Argentina - Gobierno de la Provincia de Mendoza, Argentina - Municipalidad de Malargue, Argentina - NDM Holdings, Argentina - Valle Las Lenas, Australian Research Council, Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPQ) Fundacao de Apoio a Pesquisa do Distrito Federal (FAPDF) Brazil - Financiadora de Estudos e Projetos (FINEP), Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio De Janeiro (FAPERJ), Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP) 2019/10151-2 2010/07359-6 1999/05404-3, Brazil - Ministerio da Ciencia, Tecnologia, Inovacoes e Comunicacoes (MCTIC), Brazil - Czech Republic Grant MSMT CR LTT18004 LM2015038 LM2018102 CZ.02.1.01/0.0/0.0/16_013/0001402 CZ.02.1.01/0.0/0.0/18_046/0016010 CZ.02.1.01/0.0/0.0/17_049/0008422, France - Centre de Calcul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), France - Conseil Regional Ile-de-France, France - Departement Physique Nucleaire et Corpusculaire (PNC-IN2P3/CNRS), France - Departement Sciences de l'Univers (SDU-INSU/CNRS), French National Research Agency (ANR) LABEX ANR-10-LABX-63, Institut Lagrange de Paris (ILP) within the Investissements d'Avenir Programme ANR-11-IDEX-0004-02, Federal Ministry of Education & Research (BMBF), Bundesministerium fur Bildung und Forschung (BMBF), German Research Foundation (DFG), Germany - Finanzministerium Baden-Wurttemberg, Germany - Helmholtz Alliance for Astroparticle Physics (HAP), Germany - Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF), Germany - Ministerium fur Innovation, Wissenschaft und Forschung des Landes Nordrhein-Westfalen, Germany - Ministerium fur Wissenschaft, Forschung und Kunst des Landes Baden-Wurttemberg, Italy - Istituto Nazionale di Fisica Nucleare (INFN), Italy - Istituto Nazionale di Astrofisica (INAF), Italy - Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR), Italy - CETEMPS Center of Excellence, Consejo Nacional de Ciencia y Tecnologia (CONACyT) 167733, Mexico - Universidad Nacional Autonoma de Mexico (UNAM), Mexico - PAPIIT DGAPA-UNAM, Netherlands - Ministry of Education, Culture and Science, Netherlands Organization for Scientific Research (NWO), Netherlands Organisation for Scientific Research (NWO), The Netherlands - SURF Cooperative, Poland - Ministry of Science and Higher Education DIR/WK/2018/11 Poland - National Science Centre 2013/08/M/ST9/00322 2016/23/B/ST9/01635 HARMONIA 5-2013/10/M/ST9/00062 UMO-2016/22/M/ST9/00198, Portugal - Portuguese national funds Portugal - FEDER funds within Programa Operacional Factores de Competitividade through Fundacao para a Ciencia e a Tecnologia (COMPETE), Romania - Romanian Ministry of Education and Research Romania - Program Nucleu within MCI PN19150201/16N/2019 PN19060102 Romania - PNCDI III PN-III-P1-1.2-PCCDI-2017-0839/19PCCDI/2018, Slovenian Research Agency - Slovenia P1-0031 P1-0385 I0-0033 N1-0111, Spain - Ministerio de Economia, Industria y Competitividad FPA2017-85114-P FPA2017-85197-P, Spain - Xunta de Galicia ED431C 2017/07, Junta de Andalucia SOMM17/6104/UGR, Spain - Feder Funds, Spain - RENATA Red Nacional Tematica de Astroparticulas FPA2015-68783-REDT, Spain - Maria de Maeztu Unit of Excellence MDM-2016-0692, United States Department of Energy (DOE) DE-AC02-07CH11359, National Science Foundation (NSF) 0450696, U.S.A. - Grainger Foundation U.S.A. - Marie Curie-IRSES/EPLANET U.S.A. - European Particle Physics Latin American Network U.S.A. - UNESCO, Italy - Ministero degli Affari Esteri (MAE), The Netherlands - Dutch national e-infrastructure

Published
2021

24. Deep-learning based reconstruction of the shower maximum X max using the water-Cherenkov detectors of the Pierre Auger Observatory

Author

A. Segreto, Günter Sigl, Orazio Zapparrata, P. Stassi, Radomir Smida, A. Machado Payeras, G. Cataldi, V. Scherini, Carola Dobrigkeit, M. Muzio, Marcio Aparecido Muller, Srijan Sehgal, Fernando Gollan, Carla Bleve, Rodrigo Guedes Lang, M. E. Bertaina, F. de Palma, Alan Watson, M. Perlin, Mihai Niculescu-Oglinzanu, L. Valore, Belén Andrada, Marina Scornavacche, V. de Souza, G. Golup, Violet M. Harvey, D. Harari, N. Kunka, T. Bister, F. Riehn, P. Tobiska, Jonathan Biteau, M. I. Micheletti, A. Insolia, Jesús Peña-Rodríguez, Matías J. Roncoroni, Sullivan Marafico, M. Kleifges, D. Zavrtanik, Marco Giammarchi, R.J. Barreira Luz, D. Melo, G. P. Guedes, F. Salamida, N. Fazzini, Jonas Glombitza, F. C. T. Barbato, A. Yushkov, Alina Mihaela Badescu, Ioana Codrina Maris, R. Sato, Lourenco Lopes, Toshihiro Fujii, S. Schröder, Italo Epicoco, Marvin Gottowik, Cristina Galea, M. Prouza, Brian Fick, Xavier Bertou, A. Di Matteo, Julian Kemp, Eric Mayotte, D. Nitz, Esteban Roulet, P. Abreu, D. Ravignani, R. M. de Almeida, K. H. Kampert, J. C. Arteaga Velázquez, J. Kleinfeller, A. Zepeda, M. Gómez Berisso, R. C. Shellard, Roberto Mussa, A. Puyleart, Jakub Juryšek, Petr Hamal, Steffen Hahn, Juan Carlos D'Olivo, Julien Manshanden, Lorenzo Caccianiga, Pedro Assis, H. Martinez, A. Etchegoyen, G. C. Hill, Corinne Berat, M. Giller, Jan Pękala, Rúben Conceição, Valerio Verzi, B. Tome, J. Chudoba, L. Lu, H. J. Mathes, Stanislav Michal, B. Wundheiler, Andres Travaini, K. Choi, Alex Kääpä, Ralph Engel, Flavia Gesualdi, J. Perez Armand, E. Varela, D. Correia dos Santos, J. Ridky, L. R. Wiencke, T. Pierog, François Montanet, Justin M. Albury, P. L. Ghia, Marcel Köpke, M. Platino, J.D. Sanabria Gomez, Rodrigo Pelayo, Jose J. Gonzalez, Stijn Buitink, Katie Mulrey, Carlos Escobar, G. De Mauro, Kevin-Druis Merenda, Vladimir Lenok, L. Perrone, H. Schieler, C. J. Todero Peixoto, Mario Buscemi, D. Nosek, E. Santos, Niklas Langner, Antonella Castellina, Eleonora Guido, Antonio Condorelli, M. Risse, Jörg R. Hörandel, J. F. Valdés Galicia, I. De Mitri, Jonathan Blazek, Jose Chinellato, J. Rodriguez Rojo, Fridtjof Feldbusch, A.L. Garcia Vegas, Enrique Zas, I. Lhenry-Yvon, C. Trimarelli, Gaia Silli, A. Filipčič, A.D. Supanitsky, Philipp Papenbreer, Claudio Galelli, A. Weindl, M. Suárez-Durán, J. Stasielak, T. Huege, Hernán Gonzalo Asorey, L. Nellen, L. Anchordoqui, Alena Bakalova, C. Morello, Miroslav Hrabovský, Petr Travnicek, Trent D. Grubb, G. Parente, Fabrizia Canfora, Fernando Contreras, A. Haungs, Juan Manuel Figueira, Roberta Colalillo, Paul Sommers, Clara Keiko Oliveira Watanabe, B. García, M. Schimp, A. G. Mariazzi, R. López, Karen S. Caballero-Mora, H. Wilczyński, Ioana Caracas, A. Letessier-Selvon, Lorenzo Cazon, C. Pérez Bertolli, F. Sanchez, F. Sarazin, S. Petrera, Marc Weber, David Schmidt, G. Farrar, L. Zehrer, J. de Oliveira, Alejandro Almela, P. Mantsch, Z. Szadkowski, M. Schimassek, C. Hojvat, Jan Ebr, Jacco Vink, Peter L. Biermann, L. Bonneau Arbeletche, Maximilian Reininghaus, Paolo Privitera, M. A. Leigui de Oliveira, Jaime Alvarez-Muñiz, Alexandru Gherghel-Lascu, Martin Erdmann, J. de Jesús, A. Taboada, G. Marsella, E. M. Santos, A. Gorgi, H.O. Klages, B. C. Manning, Dariusz Gora, Bjarni Pont, Thomas Bretz, Petr Janecek, Corbin Covault, Matías Rolf Hampel, Frank G. Schröder, R. Squartini, Alfred Müller, P.F. Gómez Vitale, A. Streich, Gioacchino Alex Anastasi, M. Wirtz, David Wittkowski, G. Salina, Roger W Clay, Olivier Deligny, W. M. Namasaka, M. Mastrodicasa, A. C. Rovero, Alexandru Balaceanu, A. A. Nucita, Alan Coleman, Lino Miramonti, S. J. Saffi, Lukáš Vaclavek, J. F. Soriano, D. de Oliveira Franco, R. Alves Batista, Bruce R. Dawson, Octavian Sima, Ana Martina Botti, Jeffrey Brack, Olaf Scholten, P.O. Mazur, K.-H. Becker, Maria Rita Coluccia, Dusan Mandat, Francesco Fenu, Humberto Ibarguen Salazar, M. Pimenta, Tomáš Fodran, Alina Nasr-Esfahani, P.R. Araújo Ferreira, Tobias Winchen, G. Mancarella, B. Keilhauer, Florian Lukas Briechle, Darko Veberič, Ugo Giaccari, S. J. Sciutto, F. Pedreira, Christian Sarmiento-Cano, Raul Sarmento, G. Medina-Tanco, Felix Schlüter, P. Ruehl, Carla Aramo, Vincenzo Rizi, C. J.W.P. Timmermans, Julien Souchard, Jon Paul Lundquist, A. Menshikov, D. Martello, Juan Miguel Carceller, C. M. Schäfer, Markus Roth, Silvia Mollerach, O. Martínez Bravo, Isabel Goos, D. Heck, A. Tapia, Josina Schulte, Peter Hansen, M. del Río, H. Gemmeke, Fabian Gobbi, B. L. Lago, P. Savina, W. Rodrigues de Carvalho, Denise Boncioli, M. Unger, F. Guarino, John Matthews, Peter Buchholz, Marco Aglietta, Miguel Mostafa, E.E. Pereira Martins, Serguei Vorobiov, Martina Bohacova, Miroslav Pech, M. Pothast, J. Hulsman, J. Rautenberg, Pavel Horvath, Q. Luce, Marcus Niechciol, Juan Pablo Gongora, Paula Gina Isar, Sofia Andringa, Maximilian Stadelmaier, Nataliia Borodai, Marcos Cerda, D. Lo Presti, S. J. De Jong, Samo Stanič, Jarryd A. Day, A. Saftoiu, A.C. Cobos Cerutti, Martin Vacula, J. R. T. de Mello Neto, V. Novotny, V. K.C. Varma, Rossella Caruso, A. Lucero, Fernando Catalani, N. González, Kai Daumiller, Heino Falcke, S. Querchfeld, Olena Tkachenko, Thomas Hebbeker, Sergio Dasso, Tristan Sudholz, J. Šupík, Carlo Ventura, Martín Miguel Freire, V. Pirronello, J. Vicha, Ladislav Chytka, A. Aab, Carla Taricco, Matias Tueros, Luis A. Nunez, T. Suomijärvi, J. Pallotta, Hernan Wahlberg, A. Parra, A. Fuster, M. Trini, P.G. Brichetto Orchera, I. Allekotte, A. C. Fauth, Carla Bonifazi, Jose A. Bellido, Fabio Convenga, I.D. Vergara Quispe, M. Zavrtanik, E. De Vito, Giovanni Consolati, Petr Schovanek, Denis Stanca, Ralf Ulrich, L. Nožka, G. Matthiae, Antonio Bueno, Gualberto Avila, John Farmer, Maria-Teresa Dova, R.C. dos Anjos, Adriana Vásquez-Ramírez, M. Palatka, Jeffrey A. Johnsen, Aab, A., Abreu, P., Aglietta, M., Albury, J. M., Allekotte, I., Almela, A., Alvarez-Mu??iz, J., Alves Batista, R., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Ara??jo Ferreira, P. R., Arteaga Vel??zquez, J. C., Asorey, H., Assis, P., Avila, G., Badescu, A. M., Bakalova, A., Balaceanu, A., Barbato, F., Barreira Luz, R. J., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Bister, T., Biteau, J., Blazek, J., Bleve, C., Boh????ov??, M., Boncioli, D., Bonifazi, C., Bonneau Arbeletche, L., Borodai, N., Botti, A. M., Brack, J., Bretz, T., Brichetto Orchera, P. G., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero-Mora, K. S., Caccianiga, L., Canfora, F., Caracas, I., Carceller, J. M., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Cerda, M., Chinellato, J. A., Choi, K., Chudoba, J., Chytka, L., Clay, R. W., Cobos Cerutti, A. C., Colalillo, R., Coleman, A., Coluccia, M. R., Concei????o, R., Condorelli, A., Consolati, G., Contreras, F., Convenga, F., Correia dos Santos, D., Covault, C. E., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., de Almeida, R. M., de Jes??s, J., de Jong, S. J., De Mauro, G., de Mello Neto, J. R. T., De Mitri, I., de Oliveira, J., de Oliveira Franco, D., de Palma, F., de Souza, V., De Vito, E., del R??o, M., Deligny, O., Di Matteo, A., Dobrigkeit, C., D'Olivo, J. C., dos Anjos, R. C., Dova, M. T., Ebr, J., Engel, R., Epicoco, I., Erdmann, M., Escobar, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Fick, B., Figueira, J. M., Filip??i??, A., Fodran, T., Freire, M. M., Fujii, T., Fuster, A., Galea, C., Galelli, C., Garc??a, B., Garcia Vegas, A. L., Gemmeke, H., Gesualdi, F., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., Glombitza, J., Gobbi, F., Gollan, F., Golup, G., G??mez Berisso, M., G??mez Vitale, P. F., Gongora, J. P., Gonz??lez, J. M., Gonz??lez, N., Goos, I., G??ra, D., Gorgi, A., Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Hahn, S., Hamal, P., Hampel, M. R., Hansen, P., Harari, D., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Hill, G. C., Hojvat, C., H??randel, J. R., Horvath, P., Hrabovsk??, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Janecek, P., Johnsen, J. A., Jurysek, J., K????p??, A., Kampert, K. H., Keilhauer, B., Kemp, J., Klages, H. O., Kleifges, M., Kleinfeller, J., K??pke, M., Kunka, N., Lago, B. L., Lang, R. G., Langner, N., Leigui de Oliveira, M. A., Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Lo Presti, D., Lopes, L., L??pez, R., Lu, L., Luce, Q., Lucero, A., Lundquist, J. P., Machado Payeras, A., Mancarella, G., Mandat, D., Manning, B. C., Manshanden, J., Mantsch, P., Marafico, S., Mariazzi, A. G., Mari??, I. C., Marsella, G., Martello, D., Martinez, H., Mart??nez Bravo, O., Mastrodicasa, M., Mathes, H. J., Matthews, J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina-Tanco, G., Melo, D., Menshikov, A., Merenda, K. -D., Michal, S., Micheletti, M. I., Miramonti, L., Mollerach, S., Montanet, F., Morello, C., Mostaf??, M., M??ller, A. L., Muller, M. A., Mulrey, K., Mussa, R., Muzio, M., Namasaka, W. M., Nasr-Esfahani, A., Nellen, L., Niculescu-Oglinzanu, M., Niechciol, M., Nitz, D., Nosek, D., Novotny, V., No??ka, L., Nucita, A., N????ez, L. A., Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Pech, M., Pedreira, F., P??kala, J., Pelayo, R., Pe??a-Rodriguez, J., Pereira Martins, E. E., Perez Armand, J., P??rez Bertolli, C., Perlin, M., Perrone, L., Petrera, S., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Pont, B., Pothast, M., Privitera, P., Prouza, M., Puyleart, A., Querchfeld, S., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Rizi, V., Rodrigues de Carvalho, W., Rodriguez Rojo, J., Roncoroni, M. J., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Salina, G., Sanabria Gomez, J. D., S??nchez, F., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Savina, P., Sch??fer, C. M., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schl??ter, F., Schmidt, D., Scholten, O., Schov??nek, P., Schr??der, F. G., Schr??der, S., Schulte, J., Sciutto, S. J., Scornavacche, M., Segreto, A., Sehgal, S., Shellard, R. C., Sigl, G., Silli, G., Sima, O., m??da, R., Sommers, P., Soriano, J. F., Souchard, J., Squartini, R., Stadelmaier, M., Stanca, D., Stani??, S., Stasielak, J., Stassi, P., Streich, A., Su??rez-Dur??n, M., Sudholz, T., Suomij??rvi, T., Supanitsky, A. D., up??k, J., Szadkowski, Z., Taboada, A., Tapia, A., Taricco, C., Timmermans, C., Tkachenko, O., Tobiska, P., Todero Peixoto, C. J., Tom??, B., Travaini, A., Travnicek, P., Trimarelli, C., Trini, M., Tueros, M., Ulrich, R., Unger, M., Vaclavek, L., Vacula, M., Galicia, J. F. Vald??s., Valore, L., Varela, E., Varma K. C., V., V??squez-Ram??rez, A., Veberi??, D., Ventura, C., Vergara Quispe, I. D., Verzi, V., Vicha, J., Vink, J., Vorobiov, S., Wahlberg, H., Watanabe, C., Watson, A. A., Weber, M., Weindl, A., Wiencke, L., Wilczy??ski, H., Winchen, T., Wirtz, M., Wittkowski, D., Wundheiler, B., Yushkov, A., Zapparrata, O., Zas, E., Zavrtanik, D., Zavrtanik, M., Zehrer, L., Zepeda, A., High Energy Astrophys. & Astropart. Phys (API, FNWI), Gravitation and Astroparticle Physics Amsterdam, Astronomy and Astrophysics Research Group, Physics, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Institut de Physique Nucléaire d'Orsay (IPNO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Pierre Auger, Aab A., Abreu P., Aglietta M., Albury J.M., Allekotte I., Almela A., Alvarez-Muniz J., Batista R.A., Anastasi G.A., Anchordoqui L., Andrada B., Andringa S., Aramo C., Ferreira P.R.A., Velazquez J.C.A., Asorey H., Assis P., Avila G., Badescu A.M., Bakalova A., Balaceanu A., Barbato F., Luz R.J.B., Becker K.H., Bellido J.A., Berat C., Bertaina M.E., Bertou X., Biermann P.L., Bister T., Biteau J., Blazek J., Bleve C., Bohacova M., Boncioli D., Bonifazi C., Arbeletche L.B., Borodai N., Botti A.M., Brack J., Bretz T., Orchera P.G.B., Briechle F.L., Buchholz P., Bueno A., Buitink S., Buscemi M., Caballero-Mora K.S., Caccianiga L., Canfora F., Caracas I., Carceller J.M., Caruso R., Castellina A., Catalani F., Cataldi G., Cazon L., Cerda M., Chinellato J.A., Choi K., Chudoba J., Chytka L., Clay R.W., Cerutti A.C.C., Colalillo R., Coleman A., Coluccia M.R., Conceicao R., Condorelli A., Consolati G., Contreras F., Convenga F., dos Santos D.C., Covault C.E., Dasso S., Daumiller K., Dawson B.R., Day J.A., de Almeida R.M., de Jesus J., de Jong S.J., de Mauro G., de Mello Neto J.R.T., de Mitri I., de Oliveira J., de Oliveira Franco D., de Palma F., de Souza V., de Vito E., del Rio M., Deligny O., Di Matteo A., Dobrigkeit C., D'Olivo J.C., dos Anjos R.C., Dova M.T., Ebr J., Engel R., Epicoco I., Erdmann M., Escobar C.O., Etchegoyen A., Falcke H., Farmer J., Farrar G., Fauth A.C., Fazzini N., Feldbusch F., Fenu F., Fick B., Figueira J.M., Filipcic A., Fodran T., Freire M.M., Fujii T., Fuster A., Galea C., Galelli C., Garcia B., Vegas A.L.G., Gemmeke H., Gesualdi F., Gherghel-Lascu A., Ghia P.L., Giaccari U., Giammarchi M., Giller M., Glombitza J., Gobbi F., Gollan F., Golup G., Berisso M.G., Vitale P.F.G., Gongora J.P., Gonzalez J.M., Gonzalez N., Goos I., Gora D., Gorgi A., Gottowik M., Grubb T.D., Guarino F., Guedes G.P., Guido E., Hahn S., Hamal P., Hampel M.R., Hansen P., Harari D., Harvey V.M., Haungs A., Hebbeker T., Heck D., Hill G.C., Hojvat C., Horandel J.R., Horvath P., Hrabovsky M., Huege T., Hulsman J., Insolia A., Isar P.G., Janecek P., Johnsen J.A., Jurysek J., Kaapa A., Kampert K.H., Keilhauer B., Kemp J., Klages H.O., Kleifges M., Kleinfeller J., Kopke M., Kunka N., Lago B.L., Lang R.G., Langner N., de Oliveira M.A.L., Lenok V., Letessier-Selvon A., Lhenry-Yvon I., Presti D.L., Lopes L., Lopez R., Lu L., Luce Q., Lucero A., Lundquist J.P., Payeras A.M., Mancarella G., Mandat D., Manning B.C., Manshanden J., Mantsch P., Marafico S., Mariazzi A.G., Maris I.C., Marsella G., Martello D., Martinez H., Bravo O.M., Mastrodicasa M., Mathes H.J., Matthews J., Matthiae G., Mayotte E., Mazur P.O., Medina-Tanco G., Melo D., Menshikov A., Merenda K.-D., Michal S., Micheletti M.I., Miramonti L., Mollerach S., Montanet F., Morello C., Mostafa M., Muller A.L., Muller M.A., Mulrey K., Mussa R., Muzio M., Namasaka W.M., Nasr-Esfahani A., Nellen L., Niculescu-Oglinzanu M., Niechciol M., Nitz D., Nosek D., Novotny V., Nozka L., Nucita A., Nunez L.A., Palatka M., Pallotta J., Papenbreer P., Parente G., Parra A., Pech M., Pedreira F., Pekala J., Pelayo R., Pena-Rodriguez J., Martins E.E.P., Armand J.P., Bertolli C.P., Perlin M., Perrone L., Petrera S., Pierog T., Pimenta M., Pirronello V., Platino M., Pont B., Pothast M., Privitera P., Prouza M., Puyleart A., Querchfeld S., Rautenberg J., Ravignani D., Reininghaus M., Ridky J., Riehn F., Risse M., Rizi V., Rodrigues de Carvalho W., Rojo J.R., Roncoroni M.J., Roth M., Roulet E., Rovero A.C., Ruehl P., Saffi S.J., Saftoiu A., Salamida F., Salazar H., Salina G., Gomez J.D.S., Sanchez F., Santos E.M., Santos E., Sarazin F., Sarmento R., Sarmiento-Cano C., Sato R., Savina P., Schafer C.M., Scherini V., Schieler H., Schimassek M., Schimp M., Schluter F., Schmidt D., Scholten O., Schovanek P., Schroder F.G., Schroder S., Schulte J., Sciutto S.J., Scornavacche M., Segreto A., Sehgal S., Shellard R.C., Sigl G., Silli G., Sima O., Smida R., Sommers P., Soriano J.F., Souchard J., Squartini R., Stadelmaier M., Stanca D., Stanic S., Stasielak J., Stassi P., Streich A., Suarez-Duran M., Sudholz T., Suomijarvi T., Supanitsky A.D., Supik J., Szadkowski Z., Taboada A., Tapia A., Taricco C., Timmermans C., Tkachenko O., Tobiska P., Peixoto C.J.T., Tome B., Travaini A., Travnicek P., Trimarelli C., Trini M., Tueros M., Ulrich R., Unger M., Vaclavek L., Vacula M., Galicia J.F.V., Valore L., Varela E., Varma V.K.C., Vasquez-Ramirez A., Veberic D., Ventura C., Quispe I.D.V., Verzi V., Vicha J., Vink J., Vorobiov S., Wahlberg H., Watanabe C., Watson A.A., Weber M., Weindl A., Wiencke L., Wilczynski H., Winchen T., Wirtz M., Wittkowski D., Wundheiler B., Yushkov A., Zapparrata O., Zas E., Zavrtanik D., Zavrtanik M., Zehrer L., Zepeda A., Research unit Astroparticle Physics, Alvarez-Muniz, J., Batista, R. A., Ferreira, P. R. A., Velazquez, J. C. A., Luz, R. J. B., Bohacova, M., Arbeletche, L. B., Orchera, P. G. B., Cerutti, A. C. C., Conceicao, R., dos Santos, D. C., de Jesus, J., de Mauro, G., de Mitri, I., de Vito, E., del Rio, M., Filipcic, A., Garcia, B., Vegas, A. L. G., Berisso, M. G., Vitale, P. F. G., Gonzalez, J. M., Gonzalez, N., Gora, D., Horandel, J. R., Hrabovsky, M., Kaapa, A., Kopke, M., de Oliveira, M. A. L., Presti, D. L., Lopez, R., Payeras, A. M., Maris, I. C., Bravo, O. M., Mostafa, M., Muller, A. L., Nozka, L., Nunez, L. A., Pekala, J., Pena-Rodriguez, J., Martins, E. E. P., Armand, J. P., Bertolli, C. P., Rojo, J. R., Gomez, J. D. S., Sanchez, F., Schafer, C. M., Schluter, F., Schovanek, P., Schroder, F. G., Schroder, S., Smida, R., Stanic, S., Suarez-Duran, M., Suomijarvi, T., Supik, J., Peixoto, C. J. T., Tome, B., Galicia, J. F. V., Varma, V. K. C., Vasquez-Ramirez, A., Veberic, D., Quispe, I. D. V., and Wilczynski, H.

Subjects
showers: energy, longitudinal [showers], interaction: model, Physics::Instrumentation and Detectors, Astronomy, Calibration and fitting methods, Cluster finding, Data analysis, Large detector systems for particle and astroparticle physics, Particle identification methods, Pattern recognition, 01 natural sciences, High Energy Physics - Experiment, Auger, High Energy Physics - Experiment (hep-ex), cluster finding, surface [detector], Observatory, Large detector systems, Instrumentation, Mathematical Physics, High Energy Astrophysical Phenomena (astro-ph.HE), astro-ph.HE, Physics, Pattern recognition, cluster finding, calibration and fitting methods, Settore FIS/01 - Fisica Sperimentale, model [interaction], Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Data analysi, calibration and fitting methods, energy [showers], observatory, Pattern recognition, cluster finding, calibration and fitting method, astroparticle physics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, atmosphere [showers], air, neural network, Astrophysics::High Energy Astrophysical Phenomena, UHE [cosmic radiation], FOS: Physical sciences, Cosmic ray, detector: fluorescence, 0103 physical sciences, ddc:530, High Energy Physics, ddc:610, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], cosmic radiation: UHE, structure, particle physics, network: performance, 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Ciencias Exactas, Cherenkov radiation, fluorescence [detector], Pierre Auger Observatory, mass spectrum [nucleus], showers: atmosphere, detector: surface, hep-ex, 010308 nuclear & particles physics, Física, resolution, calibration, Computational physics, performance [network], Cherenkov counter, Air shower, Large detector systems for particle and astroparticle physic, Experimental High Energy Physics, High Energy Physics::Experiment, nucleus: mass spectrum, showers: longitudinal, RAIOS CÓSMICOS, Energy (signal processing), astro-ph.IM
Abstract

The atmospheric depth of the air shower maximum $X_{\mathrm{max}}$ is an observable commonly used for the determination of the nuclear mass composition of ultra-high energy cosmic rays. Direct measurements of $X_{\mathrm{max}}$ are performed using observations of the longitudinal shower development with fluorescence telescopes. At the same time, several methods have been proposed for an indirect estimation of $X_{\mathrm{max}}$ from the characteristics of the shower particles registered with surface detector arrays. In this paper, we present a deep neural network (DNN) for the estimation of $X_{\mathrm{max}}$. The reconstruction relies on the signals induced by shower particles in the ground based water-Cherenkov detectors of the Pierre Auger Observatory. The network architecture features recurrent long short-term memory layers to process the temporal structure of signals and hexagonal convolutions to exploit the symmetry of the surface detector array. We evaluate the performance of the network using air showers simulated with three different hadronic interaction models. Thereafter, we account for long-term detector effects and calibrate the reconstructed $X_{\mathrm{max}}$ using fluorescence measurements. Finally, we show that the event-by-event resolution in the reconstruction of the shower maximum improves with increasing shower energy and reaches less than $25~\mathrm{g/cm^{2}}$ at energies above $2\times 10^{19}~\mathrm{eV}$., Published version, 29 pages, 12 figures

Published
2021

25. The energy spectrum of cosmic rays beyond the turn-down around 1017 eV as measured with the surface detector of the Pierre Auger Observatory

Author

A. C. Fauth, Vladimir Lenok, L. Perrone, M. I. Micheletti, M. Risse, Jonathan Blazek, Alessio Gorgi, Carla Bonifazi, Jose A. Bellido, Fabio Convenga, Marvin Gottowik, G. Matthiae, Brian Fick, Orazio Zapparrata, Antonio Bueno, Carola Dobrigkeit, M. Muzio, G. Parente, D. Melo, J. Rautenberg, M. E. Bertaina, Abha Khakurdikar, P. Abreu, Fabrizia Canfora, D. Ravignani, L. Bonneau Arbeletche, L. Zehrer, Q. Luce, M. Schimassek, C. Hojvat, Jan Ebr, Alan Watson, I.D. Vergara Quispe, G. P. Guedes, Toshihiro Fujii, Jakub Juryšek, Petr Hamal, Steffen Hahn, Juan Carlos D'Olivo, T. Pierog, Eric Mayotte, Esteban Roulet, M. Gómez Berisso, R. C. Shellard, Justin M. Albury, P. L. Ghia, Gualberto Avila, Sara Martinelli, M. Perlin, Mihai Niculescu-Oglinzanu, Zoé Torrès, Dariusz Gora, B. Tome, Josina Schulte, Maximilian Stadelmaier, F. Riehn, Marina Scornavacche, Jonathan Biteau, K. H. Kampert, J. C. Arteaga Velázquez, Ioana Codrina Maris, Octavian Sima, J. de Oliveira, R. Conceição, Alejandro Almela, Jacco Vink, H.O. Klages, Alan Coleman, Peter Hansen, F. Guarino, John Matthews, Peter Buchholz, J. F. Valdés Galicia, L. Valore, D. Nitz, W. M. Namasaka, A. C. Rovero, S. J. Saffi, Isabel Goos, D. Heck, Jeffrey A. Johnsen, Miroslav Hrabovský, A. Haungs, Julien Manshanden, V. V. Kizakke Covilakam, Andres Travaini, A. Segreto, Günter Sigl, D. Nosek, E. Santos, A. A. Nucita, I. De Mitri, R. Sato, M. del Río, P. Stassi, Hernan Wahlberg, Radomir Smida, Mario Buscemi, John Farmer, F. Fenu, A. Machado Payeras, Violet M. Harvey, D. Harari, Marcel Köpke, M. Platino, G. C. Hill, P. Mantsch, D. Lo Presti, S. J. De Jong, Alexandru Balaceanu, Z. Szadkowski, E. Varela, J.D. Sanabria Gomez, Roberto Mussa, Marco Aglietta, Julian Kemp, Paul Sommers, Srijan Sehgal, Jorge F. Soriano, Thomas Hebbeker, Fernando Gollan, Max Büsken, Sergio Dasso, Tristan Sudholz, Martín Miguel Freire, M. A. Leigui de Oliveira, F. Pedreira, V. de Souza, Carla Aramo, Vincenzo Rizi, J. Perez Armand, Maria-Teresa Dova, M. R. Hampel, Pierre Billoir, A. Puyleart, Corinne Berat, Julien Souchard, Thomas Fitoussi, D. Martello, Alena Bakalova, Jarryd A. Day, A. Saftoiu, Ralph Engel, J. Ridky, A. Parra, M. Zavrtanik, L. R. Wiencke, Niklas Langner, Alex Kääpä, Marcio Aparecido Muller, Martina Bohacova, Giovanni Mancarella, O. Martínez Bravo, K. Mulrey, F. Sánchez, Miroslav Pech, V. Pirronello, Raul Sarmento, Felix Schlüter, Fabian Gobbi, Sullivan Marafico, Juan Pablo Gongora, Alina Mihaela Badescu, A. Weindl, Cristina Galea, François Montanet, M. Pothast, A.C. Cobos Cerutti, F. de Palma, E. De Vito, Darko Veberič, M. Suárez-Durán, Pavel Horvath, Claudio Galelli, M. Prouza, P. Ruehl, Marco Giammarchi, Clara Keiko Oliveira Watanabe, Flavia Gesualdi, J. R. T. de Mello Neto, Carla Taricco, Carla Bleve, Rodrigo Guedes Lang, R. M. de Almeida, T. Huege, Jeffrey Brack, Matias Tueros, G. Golup, Humberto Ibarguen Salazar, Eleonora Guido, Giovanni Consolati, Frank G. Schröder, N. Kunka, Maria Rita Coluccia, Maximilian Reininghaus, P. Tobiska, B. Andrada, K.-H. Becker, M. Pimenta, Silvia Mollerach, T. Bister, G. Marsella, H. Schieler, Jesús Peña-Rodríguez, P.G. Brichetto Orchera, David Wittkowski, G. Salina, Olivier Deligny, D. Correia dos Santos, Rodrigo Pelayo, Antonella Castellina, Stijn Buitink, V. Novotny, Luis A. Nunez, J. Stasielak, Jannis Pawlowsky, Rossella Caruso, Fernando Catalani, D. D. dos Santos, Sofia Andringa, R.C. dos Anjos, N. Fazzini, David Schmidt, Adriana Vásquez-Ramírez, Jonas Glombitza, F. C. T. Barbato, I. Allekotte, M. J. Roncoroni, Caterina Trimarelli, P.R. Araújo Ferreira, S. Schröder, Italo Epicoco, A. L. Müller, Tomáš Fodran, Alina Nasr-Esfahani, Thomas Bretz, Miguel Mostafa, Daniela Mockler, Petr Schovanek, L. Lopes, A. Di Matteo, R. Squartini, Florian Lukas Briechle, Petr Janecek, Corbin Covault, T. Suomijärvi, J. Pallotta, Juan Manuel González, G. De Mauro, M. Palatka, Gaia Silli, A. Tapia, A. Filipčič, Jörg R. Hörandel, L. Lu, Jaime Alvarez-Muñiz, Alexandru Gherghel-Lascu, J. Chudoba, M. Schimp, G. Cataldi, Ugo Giaccari, B. Wundheiler, Martin Vacula, Christian Sarmiento-Cano, W. Rodrigues de Carvalho, Virginia Binet, Luis A. Anchordoqui, Massimo Mastrodicasa, F. Sarazin, Lino Miramonti, B. C. Manning, H. Gemmeke, Jon Paul Lundquist, Markus Roth, A. M. Botti, M. Unger, S. Petrera, H. J. Mathes, Marc Weber, Stanislav Michal, Dusan Mandat, V. Scherini, Philipp Papenbreer, Jose Chinellato, Heino Falcke, D. de Oliveira Franco, Samo Stanič, A. Menshikov, Denis Stanca, Lukáš Vaclavek, R.J. Barreira Luz, Petr Travnicek, A. Fuster, I. Lhenry-Yvon, Denise Boncioli, L. Nellen, B. García, Bjarni Pont, B. Keilhauer, C. M. Schäfer, J. Kleinfeller, Ioana Caracas, J. Rodriguez Rojo, J. Vicha, Trent D. Grubb, A. Letessier-Selvon, Serguei Vorobiov, R. López, Karen S. Caballero-Mora, Lorenzo Cazon, C. Pérez Bertolli, N. González, P. Savina, G. Medina-Tanco, Nataliia Borodai, Marcus Niechciol, Fridtjof Feldbusch, Enrique Zas, André Schulz, Juan Manuel Figueira, Roberta Colalillo, S. J. Sciutto, C. J.W.P. Timmermans, C. Morello, L. M. Domingues Mendes, Carlos Escobar, A. G. Mariazzi, Kevin-Druis Merenda, Kai Daumiller, Ralf Ulrich, Martin Erdmann, Fernando Contreras, Juan Miguel Carceller, Xavier Bertou, G. Farrar, Nikolaos Karastathis, Antonio Condorelli, Peter L. Biermann, S. Querchfeld, Olena Tkachenko, Marcos Cerda, Pedro Assis, H. Martinez, J. de Jesús, A. Streich, Gioacchino Alex Anastasi, C. J. Todero Peixoto, A. Insolia, A. Etchegoyen, M. Kleifges, D. Zavrtanik, A.D. Supanitsky, J. Pȩkala, A.L. Garcia Vegas, M. Wirtz, Roger W Clay, Paolo Privitera, Carlo Ventura, F. Salamida, A. Yushkov, Ladislav Chytka, L. Nožka, Lorenzo Caccianiga, P.F. Gómez Vitale, Hernán Asorey, H. Wilczyński, E. M. Santos, Valerio Verzi, Kathrin Bismark, O. Scholten, R. Alves Batista, Bruce R. Dawson, P.O. Mazur, B. L. Lago, E.E. Pereira Martins, Paula Gina Isar, High Energy Astrophys. & Astropart. Phys (API, FNWI), Abreu, P., Aglietta, M., Albury, J. M., Allekotte, I., Almela, A., Alvarez-Muniz, J., Alves Batista, R., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Araujo Ferreira, P. R., Arteaga Velazquez, J. C., Asorey, H., Assis, P., Avila, G., Badescu, A. M., Bakalova, A., Balaceanu, A., Barbato, F., Barreira Luz, R. J., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Billoir, P., Binet, V., Bismark, K., Bister, T., Biteau, J., Blazek, J., Bleve, C., Bohacova, M., Boncioli, D., Bonifazi, C., Bonneau Arbeletche, L., Borodai, N., Botti, A. M., Brack, J., Bretz, T., Brichetto Orchera, P. G., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Busken, M., Caballero-Mora, K. S., Caccianiga, L., Canfora, F., Caracas, I., Carceller, J. M., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Cerda, M., Chinellato, J. A., Chudoba, J., Chytka, L., Clay, R. W., Cobos Cerutti, A. C., Colalillo, R., Coleman, A., Coluccia, M. R., Conceicao, R., Condorelli, A., Consolati, G., Contreras, F., Convenga, F., Correia dos Santos, D., Covault, C. E., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., de Almeida, R. M., de Jesus, J., de Jong, S. J., De Mauro, G., de Mello Neto, J. R. T., De Mitri, I., de Oliveira, J., de Oliveira Franco, D., de Palma, F., de Souza, V., De Vito, E., del Rio, M., Deligny, O., Di Matteo, A., Dobrigkeit, C., D'Olivo, J. C., Domingues Mendes, L. M., dos Anjos, R. C., dos Santos, D., Dova, M. T., Ebr, J., Engel, R., Epicoco, I., Erdmann, M., Escobar, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Fick, B., Figueira, J. M., Filipcic, A., Fitoussi, T., Fodran, T., Freire, M. M., Fujii, T., Fuster, A., Galea, C., Galelli, C., Garcia, B., Garcia Vegas, A. L., Gemmeke, H., Gesualdi, F., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Glombitza, J., Gobbi, F., Gollan, F., Golup, G., Gomez Berisso, M., Gomez Vitale, P. F., Gongora, J. P., Gonzalez, J. M., Gonzalez, N., Goos, I., Gora, D., Gorgi, A., Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Hahn, S., Hamal, P., Hampel, M. R., Hansen, P., Harari, D., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Hill, G. C., Hojvat, C., Horandel, J. R., Horvath, P., Hrabovsky, M., Huege, T., Insolia, A., Isar, P. G., Janecek, P., Johnsen, J. A., Jurysek, J., Kaapa, A., Kampert, K. H., Karastathis, N., Keilhauer, B., Kemp, J., Khakurdikar, A., Kizakke Covilakam, V. V., Klages, H. O., Kleifges, M., Kleinfeller, J., Kopke, M., Kunka, N., Lago, B. L., Lang, R. G., Langner, N., Leigui de Oliveira, M. A., Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Lo Presti, D., Lopes, L., Lopez, R., Lu, L., Luce, Q., Lundquist, J. P., Machado Payeras, A., Mancarella, G., Mandat, D., Manning, B. C., Manshanden, J., Mantsch, P., Marafico, S., Mariazzi, A. G., Maris, I. C., Marsella, G., Martello, D., Martinelli, S., Martinez, H., Martinez Bravo, O., Mastrodicasa, M., Mathes, H. J., Matthews, J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina-Tanco, G., Melo, D., Menshikov, A., Merenda, K. -D., Michal, S., Micheletti, M. I., Miramonti, L., Mockler, D., Mollerach, S., Montanet, F., Morello, C., Mostafa, M., Muller, A. L., Muller, M. A., Mulrey, K., Mussa, R., Muzio, M., Namasaka, W. M., Nasr-Esfahani, A., Nellen, L., Niculescu-Oglinzanu, M., Niechciol, M., Nitz, D., Nosek, D., Novotny, V., Nozka, L., Nucita, A., Nunez, L. A., Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Pawlowsky, J., Pech, M., Pedreira, F., Pekala, J., Pelayo, R., Pena-Rodriguez, J., Pereira Martins, E. E., Perez Armand, J., Perez Bertolli, C., Perlin, M., Perrone, L., Petrera, S., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Pont, B., Pothast, M., Privitera, P., Prouza, M., Puyleart, A., Querchfeld, S., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Rizi, V., Rodrigues de Carvalho, W., Rodriguez Rojo, J., Roncoroni, M. J., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Salina, G., Sanabria Gomez, J. D., Sanchez, F., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Savina, P., Schafer, C. M., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schluter, F., Schmidt, D., Scholten, O., Schovanek, P., Schroder, F. G., Schroder, S., Schulte, J., Schulz, A., Sciutto, S. J., Scornavacche, M., Segreto, A., Sehgal, S., Shellard, R. C., Sigl, G., Silli, G., Sima, O., Smida, R., Sommers, P., Soriano, J. F., Souchard, J., Squartini, R., Stadelmaier, M., Stanca, D., Stanic, S., Stasielak, J., Stassi, P., Streich, A., Suarez-Duran, M., Sudholz, T., Suomijarvi, T., Supanitsky, A. D., Szadkowski, Z., Tapia, A., Taricco, C., Timmermans, C., Tkachenko, O., Tobiska, P., Todero Peixoto, C. J., Tome, B., Torres, Z., Travaini, A., Travnicek, P., Trimarelli, C., Tueros, M., Ulrich, R., Unger, M., Vaclavek, L., Vacula, M., Valdes Galicia, J. F., Valore, L., Varela, E., Vasquez-Ramirez, A., Veberic, D., Ventura, C., Vergara Quispe, I. D., Verzi, V., Vicha, J., Vink, J., Vorobiov, S., Wahlberg, H., Watanabe, C., Watson, A. A., Weber, M., Weindl, A., Wiencke, L., Wilczynski, H., Wirtz, M., Wittkowski, D., Wundheiler, B., Yushkov, A., Zapparrata, O., Zas, E., Zavrtanik, D., Zavrtanik, M., Zehrer, L., Physics, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Pierre Auger, Abreu P., Aglietta M., Albury J.M., Allekotte I., Almela A., Alvarez-Muniz J., Alves Batista R., Anastasi G.A., Anchordoqui L., Andrada B., Andringa S., Aramo C., Araujo Ferreira P.R., Arteaga Velazquez J.C., Asorey H., Assis P., Avila G., Badescu A.M., Bakalova A., Balaceanu A., Barbato F., Barreira Luz R.J., Becker K.H., Bellido J.A., Berat C., Bertaina M.E., Bertou X., Biermann P.L., Billoir P., Binet V., Bismark K., Bister T., Biteau J., Blazek J., Bleve C., Bohacova M., Boncioli D., Bonifazi C., Bonneau Arbeletche L., Borodai N., Botti A.M., Brack J., Bretz T., Brichetto Orchera P.G., Briechle F.L., Buchholz P., Bueno A., Buitink S., Buscemi M., Busken M., Caballero-Mora K.S., Caccianiga L., Canfora F., Caracas I., Carceller J.M., Caruso R., Castellina A., Catalani F., Cataldi G., Cazon L., Cerda M., Chinellato J.A., Chudoba J., Chytka L., Clay R.W., Cobos Cerutti A.C., Colalillo R., Coleman A., Coluccia M.R., Conceicao R., Condorelli A., Consolati G., Contreras F., Convenga F., Correia dos Santos D., Covault C.E., Dasso S., Daumiller K., Dawson B.R., Day J.A., de Almeida R.M., de Jesus J., de Jong S.J., De Mauro G., de Mello Neto J.R.T., De Mitri I., de Oliveira J., de Oliveira Franco D., de Palma F., de Souza V., De Vito E., del Rio M., Deligny O., Di Matteo A., Dobrigkeit C., D'Olivo J.C., Domingues Mendes L.M., dos Anjos R.C., dos Santos D., Dova M.T., Ebr J., Engel R., Epicoco I., Erdmann M., Escobar C.O., Etchegoyen A., Falcke H., Farmer J., Farrar G., Fauth A.C., Fazzini N., Feldbusch F., Fenu F., Fick B., Figueira J.M., Filipcic A., Fitoussi T., Fodran T., Freire M.M., Fujii T., Fuster A., Galea C., Galelli C., Garcia B., Garcia Vegas A.L., Gemmeke H., Gesualdi F., Gherghel-Lascu A., Ghia P.L., Giaccari U., Giammarchi M., Glombitza J., Gobbi F., Gollan F., Golup G., Gomez Berisso M., Gomez Vitale P.F., Gongora J.P., Gonzalez J.M., Gonzalez N., Goos I., Gora D., Gorgi A., Gottowik M., Grubb T.D., Guarino F., Guedes G.P., Guido E., Hahn S., Hamal P., Hampel M.R., Hansen P., Harari D., Harvey V.M., Haungs A., Hebbeker T., Heck D., Hill G.C., Hojvat C., Horandel J.R., Horvath P., Hrabovsky M., Huege T., Insolia A., Isar P.G., Janecek P., Johnsen J.A., Jurysek J., Kaapa A., Kampert K.H., Karastathis N., Keilhauer B., Kemp J., Khakurdikar A., Kizakke Covilakam V.V., Klages H.O., Kleifges M., Kleinfeller J., Kopke M., Kunka N., Lago B.L., Lang R.G., Langner N., Leigui de Oliveira M.A., Lenok V., Letessier-Selvon A., Lhenry-Yvon I., Lo Presti D., Lopes L., Lopez R., Lu L., Luce Q., Lundquist J.P., Machado Payeras A., Mancarella G., Mandat D., Manning B.C., Manshanden J., Mantsch P., Marafico S., Mariazzi A.G., Maris I.C., Marsella G., Martello D., Martinelli S., Martinez H., Martinez Bravo O., Mastrodicasa M., Mathes H.J., Matthews J., Matthiae G., Mayotte E., Mazur P.O., Medina-Tanco G., Melo D., Menshikov A., Merenda K.-D., Michal S., Micheletti M.I., Miramonti L., Mockler D., Mollerach S., Montanet F., Morello C., Mostafa M., Muller A.L., Muller M.A., Mulrey K., Mussa R., Muzio M., Namasaka W.M., Nasr-Esfahani A., Nellen L., Niculescu-Oglinzanu M., Niechciol M., Nitz D., Nosek D., Novotny V., Nozka L., Nucita A., Nunez L.A., Palatka M., Pallotta J., Papenbreer P., Parente G., Parra A., Pawlowsky J., Pech M., Pedreira F., Pekala J., Pelayo R., Pena-Rodriguez J., Pereira Martins E.E., Perez Armand J., Perez Bertolli C., Perlin M., Perrone L., Petrera S., Pierog T., Pimenta M., Pirronello V., Platino M., Pont B., Pothast M., Privitera P., Prouza M., Puyleart A., Querchfeld S., Rautenberg J., Ravignani D., Reininghaus M., Ridky J., Riehn F., Risse M., Rizi V., Rodrigues de Carvalho W., Rodriguez Rojo J., Roncoroni M.J., Roth M., Roulet E., Rovero A.C., Ruehl P., Saffi S.J., Saftoiu A., Salamida F., Salazar H., Salina G., Sanabria Gomez J.D., Sanchez F., Santos E.M., Santos E., Sarazin F., Sarmento R., Sarmiento-Cano C., Sato R., Savina P., Schafer C.M., Scherini V., Schieler H., Schimassek M., Schimp M., Schluter F., Schmidt D., Scholten O., Schovanek P., Schroder F.G., Schroder S., Schulte J., Schulz A., Sciutto S.J., Scornavacche M., Segreto A., Sehgal S., Shellard R.C., Sigl G., Silli G., Sima O., Smida R., Sommers P., Soriano J.F., Souchard J., Squartini R., Stadelmaier M., Stanca D., Stanic S., Stasielak J., Stassi P., Streich A., Suarez-Duran M., Sudholz T., Suomijarvi T., Supanitsky A.D., Szadkowski Z., Tapia A., Taricco C., Timmermans C., Tkachenko O., Tobiska P., Todero Peixoto C.J., Tome B., Torres Z., Travaini A., Travnicek P., Trimarelli C., Tueros M., Ulrich R., Unger M., Vaclavek L., Vacula M., Valdes Galicia J.F., Valore L., Varela E., Vasquez-Ramirez A., Veberic D., Ventura C., Vergara Quispe I.D., Verzi V., Vicha J., Vink J., Vorobiov S., Wahlberg H., Watanabe C., Watson A.A., Weber M., Weindl A., Wiencke L., Wilczynski H., Wirtz M., Wittkowski D., Wundheiler B., Yushkov A., Zapparrata O., Zas E., Zavrtanik D., Zavrtanik M., and Zehrer L.

Subjects
Physics and Astronomy (miscellaneous), Astronomy, Astrophysics::High Energy Astrophysical Phenomena, UHE [cosmic radiation], FOS: Physical sciences, Flux, Cosmic ray, Astrophysics, 7. Clean energy, 01 natural sciences, detector: fluorescence, Auger, cosmic rays, surface [detector], Observatory, 0103 physical sciences, calorimeter, ddc:530, High Energy Physics, cosmic radiation: UHE, spectrum [cosmic radiation], 010303 astronomy & astrophysics, Engineering (miscellaneous), Engineering & allied operations, High Energy Astrophysical Phenomena (astro-ph.HE), fluorescence [detector], Pierre Auger Observatory, Physics, astro-ph.HE, cosmic radiation: energy spectrum, cosmic radiation: spectrum, detector: surface, 010308 nuclear & particles physics, Settore FIS/01 - Fisica Sperimentale, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Calorimeter, flux, observatory, spectral, ddc:620, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - High Energy Astrophysical Phenomena, energy spectrum [cosmic radiation], Energy (signal processing), RAIOS CÓSMICOS, ultra-high energy cosmic rays, energy spectrum features
Abstract

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargüe. We are very grateful to the following agencies and organizations for financial support: Argentina – Comisión Nacional de Energía Atómica; Agencia Nacional de Promoción Científica y Tecnológica (ANPCyT); Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET); Gobierno de la Provincia de Mendoza; Municipalidad de Malargüe; NDM Holdings and Valle Las Leñas; in gratitude for their continuing cooperation over land access; Australia – the Australian Research Council; Belgium – Fonds de la Recherche Scientifique (FNRS); Research Foundation Flanders (FWO); Brazil – Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq); Financiadora de Estudos e Projetos (FINEP); Fundação de Amparo à Pesquisa do Estado de Rio de Janeiro (FAPERJ); São Paulo Research Foundation (FAPESP) Grants No. 2019/10151-2, No. 2010/07359-6 and No. 1999/05404-3; Ministério da Ciência, Tecnologia, Inovações e Comunicações (MCTIC); Czech Republic – Grant No. MSMT CR LTT18004, LM2015038, LM2018102, CZ.02.1.01/0.0/0.0/16_013/0001402, CZ.02.1.01/0.0/0.0/18_046/0016010 and CZ.02.1.01/0.0/0.0/17_049/0008422; France – Centre de Calcul IN2P3/CNRS; Centre National de la Recherche Scientifique (CNRS); Conseil Régional Ile-de-France; Département Physique Nucléaire et Corpusculaire (PNC-IN2P3/CNRS); Département Sciences de l’Univers (SDU-INSU/CNRS); Institut Lagrange de Paris (ILP) Grant No. LABEX ANR-10-LABX-63 within the Investissements d’Avenir Programme Grant No. ANR-11-IDEX-0004-02; Germany – Bundesministerium für Bildung und Forschung (BMBF); Deutsche Forschungsgemeinschaft (DFG); Finanzministerium Baden-Württemberg; Helmholtz Alliance for Astroparticle Physics (HAP); Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF); Ministerium für Innovation, Wissenschaft und Forschung des Landes Nordrhein-Westfalen; Ministerium für Wissenschaft, Forschung und Kunst des Landes Baden-Württemberg; Italy – Istituto Nazionale di Fisica Nucleare (INFN); Istituto Nazionale di Astrofisica (INAF); Ministero dell’Istruzione, dell’Universitá e della Ricerca (MIUR); CETEMPS Center of Excellence; Ministero degli Affari Esteri (MAE); México – Consejo Nacional de Ciencia y Tecnología (CONACYT) No. 167733; Universidad Nacional Autónoma de México (UNAM); PAPIIT DGAPA-UNAM; The Netherlands – Ministry of Education, Culture and Science; Netherlands Organisation for Scientific Research (NWO); Dutch national e-infrastructure with the support of SURF Cooperative; Poland -Ministry of Science and Higher Education, grant No. DIR/WK/2018/11; National Science Centre, Grants No. 2013/08/M/ST9/00322, No. 2016/23/B/ST9/01635 and No. HARMONIA 5–2013/10/M/ST9/00062, UMO-2016/22/M/ST9/00198; Portugal – Portuguese national funds and FEDER funds within Programa Operacional Factores de Competitividade through Fundação para a Ciência e a Tecnologia (COMPETE); Romania – Romanian Ministry of Education and Research, the Program Nucleu within MCI (PN19150201/16N/2019 and PN19060102) and project PN-III-P1-1.2-PCCDI-2017-0839/19PCCDI/2018 within PNCDI III; Slovenia – Slovenian Research Agency, grants P1-0031, P1-0385, I0-0033, N1-0111; Spain – Ministerio de Economía, Industria y Competitividad (FPA2017-85114-P and PID2019-104676GB-C32), Xunta de Galicia (ED431C 2017/07), Junta de Andalucía (SOMM17/6104/UGR, P18-FR-4314) Feder Funds, RENATA Red Nacional Temática de Astropartículas (FPA2015-68783-REDT) and María de Maeztu Unit of Excellence (MDM-2016-0692); USA – Department of Energy, Contracts No. DE-AC02-07CH11359, No. DE-FR02-04ER41300, No. DE-FG02-99ER41107 and No. DE-SC0011689; National Science Foundation, Grant No. 0450696; The Grainger Foundation; Marie Curie-IRSES/EPLANET; European Particle Physics Latin American Network; University of Delaware Research Foundation (UDRF) – 2019; and UNESCO., We present a measurement of the cosmic-ray spectrum above 100 PeV using the part of the surface detector of the Pierre Auger Observatory that has a spacing of 750 m. An inflection of the spectrum is observed, confirming the presence of the so-called second-knee feature. The spectrum is then combined with that of the 1500 m array to produce a single measurement of the flux, linking this spectral feature with the three additional breaks at the highest energies. The combined spectrum, with an energy scale set calorimetrically via fluorescence telescopes and using a single detector type, results in the most statistically and systematically precise measurement of spectral breaks yet obtained. These measurements are critical for furthering our understanding of the highest energy cosmic rays., ANR-10-LABX-63 ANR-11-IDEX-0004-02, Belgium – Fonds de la Recherche Scientifique, Comisión Nacional de Energía Atómica, Département Physique Nucléaire et Corpusculaire PNC-IN2P3/CNRS, Département Sciences de l’Univers, Feder Funds, María de Maeztu Unit of Excellence MDM-2016-0692, Ministero degli Affari Esteri, RENATA Red Nacional Temática de Astropartículas FPA2015-68783-REDT, SURF, National Science Foundation 0450696, U.S. Department of Energy DE-AC02-07CH11359, DE-FG02-99ER41107, DE-FR02-04ER41300, DE-SC0011689, University of Delaware Research Foundation, United Nations Educational, Scientific and Cultural Organization, Australian Research Council, Helmholtz-Gemeinschaft, Deutsche Forschungsgemeinschaft, Fundação de Amparo à Pesquisa do Estado de São Paulo 1999/05404-3, 2010/07359-6, 2019/10151-2, Fundação para a Ciência e a Tecnologia, Bundesministerium für Bildung und Forschung, Fonds De La Recherche Scientifique - FNRS, Consejo Nacional de Investigaciones Científicas y Técnicas, Agencia Nacional de Promoción Científica y Tecnológica, Fonds Wetenschappelijk Onderzoek, Consejo Nacional de Ciencia y Tecnología 167733, Ministerie van Onderwijs, Cultuur en Wetenschap, Nederlandse Organisatie voor Wetenschappelijk Onderzoek, Ministero dell’Istruzione, dell’Università e della Ricerca, Ministerium für Wissenschaft, Forschung und Kunst Baden-Württemberg, Conselho Nacional de Desenvolvimento Científico e Tecnológico, Conseil Régional, Île-de-France, Instituto Nazionale di Fisica Nucleare, Narodowe Centrum Nauki 2013/08/M/ST9/00322, 2013/10/M/ST9/00062, 2016/23/B/ST9/01635, UMO-2016/22/M/ST9/00198, Javna Agencija za Raziskovalno Dejavnost RS I0-0033, N1-0111, P1-0031, P1-0385, Ministerstwo Edukacji i Nauki DIR/WK/2018/11, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Centre National de la Recherche Scientifique, Financiadora de Estudos e Projetos, Istituto Nazionale di Astrofisica, Universidad Nacional Autónoma de México, Ministry of Education and Research, Romania PN-III-P1-1.2-PCCDI-2017-0839/19PCCDI/2018, PN19060102, PN19150201/16N/2019, European Regional Development Fund, Ministerium für Innovation, Wissenschaft und Forschung des Landes Nordrhein-Westfalen, Ministerio de Economía, Industria y Competitividad, Gobierno de España FPA2017-85114-P, PID2019-104676GB-C32, Xunta de Galicia ED431C 2017/07, Junta de Andalucía P18-FR-4314, Ministério da Ciência, Tecnologia, Inovações e Comunicações CZ.02.1.01/0.0/0.0/16_013/0001402, CZ.02.1.01/0.0/0.0/17_049/0008422, CZ.02.1.01/0.0/0.0/18_046/0016010, LM2015038, LM2018102, MSMT CR LTT18004, Programa Operacional Temático Factores de Competitividade, Institut Lagrange de Paris

Published
2021

26. 5.5 years multi-wavelength variability of Mrk 421: evidences of leptonic emission from the radio to TeV

Author

Adrian Biland, Dominik Baack, Roman Iotov, Marvin Beck, Maximilian Noethe, Thomas Bretz, Daniela Dorner, Jens Buss, Michael Blank, Karl Mannheim, Axel Arbet-Engels, Wolfgang Rhode, Amit Shukla, Bernd Schleicher, Matteo Balbo, Vitalii Sliusar, Dominik Elsaesser, Dominik Neise, Manuel Doerr, M. Bulinski, Dorothee Hildebrand, Aleksander Paravac, K. Sedlaczek, K. Bruegge, Laurits Tani, Marc Klinger, Fabian Theissen, and Roland Walter

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Astrophysics of Galaxies (astro-ph.GA), Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, High Energy Physics::Experiment, Multi wavelength, Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Astrophysics of Galaxies
Abstract

Mrk 421 is a high-synchrotron-peaked blazar featuring bright and persistent GeV and TeV emission. We use the longest and densest ongoing unbiased observing campaign obtained at TeV and GeV energies during 5.5 years with the FACT telescope and the Fermi-LAT detector. The contemporaneous multi-wavelength observations were used to characterize the variability of the source and to constrain the underlying physical mechanisms. We study and correlate light curves obtained by nine different instruments from radio to gamma rays and found two significant results. The TeV and X-ray light curves are very well correlated with lag, if any, shorter than a day. The GeV light curve varies independently and accurately leads the variations observed at long wavelengths, in particular in the radio band. We find that the observations match the predictions of leptonic models and suggest that the physical conditions vary along the jet, when the emitting region moves outwards., PoS: Proceedings of Science, 354, ISSN:1824-8039, Proceedings of High Energy Phenomena in Relativistic Outflows VII PoS (HEPRO VII9)

Published
2020

27. Studies on the response of a water-Cherenkov detector of the Pierre Auger Observatory to atmospheric muons using an RPC hodoscope

Author

A. Zepeda, Pedro Assis, H. Martinez, A. Etchegoyen, Dariusz Gora, Bjarni Pont, Alan Coleman, B. Tome, Peter Hansen, F. Guarino, John Matthews, Peter Buchholz, S. J. Saffi, D. Lo Presti, S. J. De Jong, B. García, R. López, Karen S. Caballero-Mora, G. Cataldi, V. Scherini, Martin Erdmann, G. Matthiae, J. de Jesús, Frank G. Schröder, Antonio Bueno, A. Streich, Gioacchino Alex Anastasi, M. Wirtz, Thomas Hebbeker, Sergio Dasso, Tristan Sudholz, P. Abreu, D. Ravignani, Roger W Clay, Marco Aglietta, Marko Zavrtanik, E. Santos, Jarryd A. Day, G. De Mauro, F. Riehn, Marina Scornavacche, Alexandra Saftoiu, Tiina Suomijarvi, F. Pedreira, Raul Sarmento, Felix Schlüter, Martin Vacula, J. Rautenberg, Q. Luce, Gualberto Avila, Martín Miguel Freire, Fabian Gobbi, Jiri Blazek, Lorenzo Caccianiga, Denis Stanca, I. Lhenry-Yvon, Miroslav Pech, M. Pothast, Markus Roth, D. Nitz, A.C. Cobos Cerutti, J. R. T. de Mello Neto, Paul Sommers, A. Blanco, Marcus Niechciol, B. Vargas Cárdenas, J. Pallotta, L. R. Wiencke, G. Marsella, F. Sánchez, Heino Falcke, Maximilian Stadelmaier, Jesús Peña-Rodríguez, Carla Bleve, Rodrigo Guedes Lang, B. Andrada, P. Horvath, Isabel Goos, D. Heck, John Farmer, Jonathan Biteau, A. Insolia, M. Kleifges, A.D. Supanitsky, J. Pȩkala, Antonio Condorelli, Christine Peters, Maria-Teresa Dova, M. R. Hampel, Valerio Verzi, J. Vicha, A. M. Botti, Niraj Dhital, P. Tobiska, Sofia Andringa, Julian Kemp, Luis Villaseñor, R. Conceição, A. Weindl, S. Querchfeld, Miroslav Hrabovský, T. Huege, M. del Río, Nicolás González, Jeffrey Brack, A.L. Garcia Vegas, M. Schimp, Marvin Gottowik, Maria Rita Coluccia, Maximilian Reininghaus, M.A. Leigui de Oliveira, Olaf Scholten, Gaia Silli, Humberto Ibarguen Salazar, D. Mockler, L. Bonneau Arbeletche, A. Di Matteo, Eric Mayotte, A. Haungs, A. Filipčič, G. Torralba Elipe, I. Valiño, Olena Tkachenko, M. I. Micheletti, B. C. Manning, P. Ruehl, Ralf Ulrich, M. Gómez Berisso, L. Valore, B. Wundheiler, L. Lopes, Roberto Mussa, J. Šupík, Carlo Ventura, F. Sarazin, Jaime Alvarez-Muñiz, Alexandru Gherghel-Lascu, David Schmidt, S. Schröder, Italo Epicoco, S. Petrera, Marc Weber, Charles Timmermans, Hernán Asorey, R.C. dos Anjos, R.C. Shellard, Adriana Vásquez-Ramírez, J. F. Valdés Galicia, M. Palatka, Mario Buscemi, Jörg R. Hörandel, P. Mantsch, J. Hulsman, Julien Manshanden, Dusan Mandat, Lukáš Vaclavek, H. J. Mathes, I. De Mitri, Stanislav Michal, G. Mancarella, François Montanet, G. Golup, B. Keilhauer, Sullivan Marafico, Vladimir Lenok, L. Perrone, Francesco Fenu, Ladislav Chytka, Gaetano Salina, Hernan Wahlberg, Miguel Mostafa, Violet M. Harvey, Andres Travaini, E. Varela, J.D. Sanabria Gomez, D. Harari, L. Nožka, J. Chudoba, S. J. Sciutto, J. Rodriguez Rojo, Fridtjof Feldbusch, Marcel Köpke, M. Platino, C. M. Schäfer, Maria Giller, R. Squartini, Alfred Müller, Marco Giammarchi, Juan Miguel Carceller, P. Savina, Eleonora Guido, W. Rodrigues de Carvalho, Flavia Gesualdi, Alex Kääpä, Enrique Zas, A. Parra, Alena Bakalova, J. Stasielak, Massimo Mastrodicasa, R. M. de Almeida, Teresa Bister, E. De Vito, R.J. Barreira Luz, Alina Mihaela Badescu, Dalibor Nosek, Fernando Contreras, Brian Fick, Samo Stanič, Giovanni Consolati, Cristina Galea, P. Ristori, M. Trini, K. Choi, Martina Bohacova, G. Medina-Tanco, A. Tapia, Octavian Sima, A. Cancio, H. Gemmeke, R. Halliday, Nataliia Borodai, M. Unger, M. L. Díaz Castro, G. Farrar, M.P. Panetta, Petr Schovanek, Juan Pablo Gongora, Christian Sarmiento-Cano, Francesca Zuccarello, Luis A. Anchordoqui, I. Allekotte, M. J. Roncoroni, Valerio Pirronello, H. Schieler, Q. Dorosti, Philipp Papenbreer, C. J. Todero Peixoto, Karl-Heinz Kampert, L. Calcagni, Kai Daumiller, Antonella Castellina, A. C. Fauth, F. Salamida, A. Yushkov, A. Fuster, A. Puyleart, L. Nellen, Zbigniew Szadkowski, Michael Prouza, Corinne Berat, Carla Bonifazi, Rodrigo Pelayo, Denise Boncioli, D. Melo, Stijn Buitink, M. Risse, V. Novotny, Trent D. Grubb, A. Taboada, Jose A. Bellido, C. Morello, Rossella Caruso, Fabio Convenga, A. Lucero, Fernando Catalani, Caterina Trimarelli, M. A. Muller, Juan Manuel Figueira, H. Wilczyński, Roberta Colalillo, P.F. Gómez Vitale, I.D. Vergara Quispe, A. G. Mariazzi, A. Aab, R. Sato, Peter L. Biermann, G. P. Guedes, Toshihiro Fujii, Paolo Privitera, Jakub Juryšek, G. Kukec Mezek, Alessio Gorgi, M. E. Bertaina, A. Menshikov, P. Travnicek, J. Debatin, Orazio Zapparrata, Carola Dobrigkeit, M. Muzio, Steffen Hahn, Juan Carlos D'Olivo, T. Pierog, Esteban Roulet, Justin M. Albury, Alan Watson, M. Perlin, Mihai Niculescu-Oglinzanu, J. Alvarez Castillo, Matias Tueros, Luis A. Nunez, Piera Luisa Ghia, Jeffrey A. Johnsen, B. L. Lago, Günter Sigl, P. Stassi, Radomir Smida, A. Machado Payeras, Paula Gina Isar, Fernando Gollan, E. M. Santos, R. Alves Batista, Bruce R. Dawson, P.O. Mazur, V. de Souza, K.-H. Becker, M. Pimenta, P.R. Araújo Ferreira, Tobias Winchen, Florian Lukas Briechle, Max Malacari, J. Perez Armand, Claudio Galelli, Jose Chinellato, Ioana Caracas, A. Letessier-Selvon, Lorenzo Cazon, A. van Vliet, David Wittkowski, Danielle LaHurd, Olivier Deligny, Tomáš Fodran, R. Lorek, M. Urban, W. M. Namasaka, A. C. Rovero, Ugo Giaccari, Alexandru Balaceanu, M. Suárez-Durán, Carla Aramo, Julien Souchard, D. Martello, M. Ziolkowski, O. Martínez Bravo, K. Mulrey, Silvia Mollerach, N. Fazzini, Ioana Codrina Maris, Jonas Glombitza, F. C. T. Barbato, D. Zavrtanik, Serguei Vorobiov, G. C. Hill, Jorge F. Soriano, Ralph Engel, Marcos Cerda, J. Ridky, Darko Veberič, J. Kleinfeller, Carlos Escobar, Kevin-Druis Merenda, M. Schimassek, C. Hojvat, Jan Ebr, Jacco Vink, H.O. Klages, A. A. Nucita, G. Parente, Fabrizia Canfora, L. Zehrer, J. de Oliveira, Alejandro Almela, Thomas Bretz, V. Rizi, Corbin Covault, Lino Miramonti, D. de Oliveira Franco, Xavier Bertou, Aab, A., Abreu, P., Aglietta, M., Albury, J. M., Allekotte, I., Almela, A., Castillo, J. Alvarez, Alvarez-Muñiz, J., Batista, R. Alve, Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Ferreira, P. R. Araújo, Asorey, H., Assis, P., Avila, G., Badescu, A. M., Bakalova, A., Balaceanu, A., Barbato, F., Luz, R. J. Barreira, Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Bister, T., Biteau, J., Blanco, A., Blazek, J., Bleve, C., Boháčová, M., Boncioli, D., Bonifazi, C., Arbeletche, L. Bonneau, Borodai, N., Botti, A. M., Brack, J., Bretz, T., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero-Mora, K. S., Caccianiga, L., Calcagni, L., Cancio, A., Canfora, F., Caracas, I., Carceller, J. M., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Cerda, M., Chinellato, J. A., Choi, K., Chudoba, J., Chytka, L., Clay, R. W., Cerutti, A. C. Cobo, Colalillo, R., Coleman, A., Coluccia, M. R., Conceição, R., Condorelli, A., Consolati, G., Contreras, F., Convenga, F., Covault, C. E., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., de Almeida, R. M., de Jesús, J., de Jong, S. J., Mauro, G. De, Neto, J. R. T. de Mello, Mitri, I. De, de Oliveira, J., Franco, D. de Oliveira, de Souza, V., Vito, E. De, Debatin, J., Río, M. del, Deligny, O., Dhital, N., Matteo, A. Di, Castro, M. L. Díaz, Dobrigkeit, C., D'Olivo, J. C., Dorosti, Q., Anjos, R. C. do, Dova, M. T., Ebr, J., Engel, R., Epicoco, I., Erdmann, M., Escobar, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Fick, B., Figueira, J. M., Filipčič, A., Fodran, T., Freire, M. M., Fujii, T., Fuster, A., Galea, C., Galelli, C., García, B., Vegas, A. L. Garcia, Gemmeke, H., Gesualdi, F., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., Glombitza, J., Gobbi, F., Gollan, F., Golup, G., Berisso, M. Gómez, Vitale, P. F. Gómez, Gongora, J. P., González, N., Goos, I., Góra, D., Gorgi, A., Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Hahn, S., Halliday, R., Hampel, M. R., Hansen, P., Harari, D., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Hill, G. C., Hojvat, C., Hörandel, J. R., Horvath, P., Hrabovský, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Johnsen, J. A., Jurysek, J., Kääpä, A., Kampert, K. H., Keilhauer, B., Kemp, J., Klages, H. O., Kleifges, M., Kleinfeller, J., Köpke, M., Mezek, G. Kukec, Lago, B. L., Lahurd, D., Lang, R. G., de Oliveira, M. A. Leigui, Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Presti, D. Lo, Lopes, L., López, R., Lorek, R., Luce, Q., Lucero, A., Payeras, A. Machado, Malacari, M., Mancarella, G., Mandat, D., Manning, B. C., Manshanden, J., Mantsch, P., Marafico, S., Mariazzi, A. G., Mariş, I. C., Marsella, G., Martello, D., Martinez, H., Bravo, O. Martínez, Mastrodicasa, M., Mathes, H. J., Matthews, J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina-Tanco, G., Melo, D., Menshikov, A., Merenda, K. -D., Michal, S., Micheletti, M. I., Miramonti, L., Mockler, D., Mollerach, S., Montanet, F., Morello, C., Mostafá, M., Müller, A. L., Muller, M. A., Mulrey, K., Mussa, R., Muzio, M., Namasaka, W. M., Nellen, L., Niculescu-Oglinzanu, M., Niechciol, M., Nitz, D., Nosek, D., Novotny, V., Nožka, L., Nucita, A, Núñez, L. A., Palatka, M., Pallotta, J., Panetta, M. P., Papenbreer, P., Parente, G., Parra, A., Pech, M., Pedreira, F., Pȩkala, J., Pelayo, R., Peña-Rodriguez, J., Armand, J. Perez, Perlin, M., Perrone, L., Peters, C., Petrera, S., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Pont, B., Pothast, M., Privitera, P., Prouza, M., Puyleart, A., Querchfeld, S., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Ristori, P., Rizi, V., de Carvalho, W. Rodrigue, Rojo, J. Rodriguez, Roncoroni, M. J., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Salina, G., Gomez, J. D. Sanabria, Sánchez, F., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Savina, P., Schäfer, C. M., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schlüter, F., Schmidt, D., Scholten, O., Schovánek, P., Schröder, F. G., Schröder, S., Sciutto, S. J., Scornavacche, M., Shellard, R. C., Sigl, G., Silli, G., Sima, O., Šmída, R., Sommers, P., Soriano, J. F., Souchard, J., Squartini, R., Stadelmaier, M., Stanca, D., Stanič, S., Stasielak, J., Stassi, P., Streich, A., Suárez-Durán, M., Sudholz, T., Suomijärvi, T., Supanitsky, A. D., Šupík, J., Szadkowski, Z., Taboada, A., Tapia, A., Timmermans, C., Tkachenko, O., Tobiska, P., Peixoto, C. J. Todero, Tomé, B., Elipe, G. Torralba, Travaini, A., Travnicek, P., Trimarelli, C., Trini, M., Tueros, M., Ulrich, R., Unger, M., Urban, M., Vaclavek, L., Vacula, M., Galicia, J. F. Valdé, Valiño, I., Valore, L., Vliet, A. van, Varela, E., Cárdenas, B. Varga, Vásquez-Ramírez, A., Veberič, D., Ventura, C., Quispe, I. D. Vergara, Verzi, V., Vicha, J., Villaseñor, L., Vink, J., Vorobiov, S., Wahlberg, H., Watson, A. A., Weber, M., Weindl, A., Wiencke, L., Wilczyński, H., Winchen, T., Wirtz, M., Wittkowski, D., Wundheiler, B., Yushkov, A., Zapparrata, O., Zas, E., Zavrtanik, D., Zavrtanik, M., Zehrer, L., Zepeda, A., Ziolkowski, M., Zuccarello, F., Castillo, J. A., Alvarez-Muniz, J., Batista, R. A., Ferreira, P. R. A., Luz, R. J. B., Bohacova, M., Arbeletche, L. B., Cerutti, A. C. C., Conceicao, R., De Almeida, R. M., De Jesus, J., De Jong, S. J., Mauro, G. D., Neto, J. R. T. D. M., De Mitri, I., De Oliveira, J., De Oliveira Franco, D., De Souza, V., De Vito, E., Del Rio, M., Di Matteo, A., Castro, M. L. D., Dos Anjos, R. C., Filipcic, A., Garcia, B., Vegas, A. L. G., Berisso, M. G., Vitale, P. F. G., Gonzalez, N., Gora, D., Horandel, J. R., Hrabovsky, M., Kaapa, A., Kopke, M., Mezek, G. K., De Oliveira, M. A. L., Presti, D. L., Lopez, R., Payeras, A. M., Maris, I. C., Bravo, O. M., Mostafa, M., Muller, A. L., Nozka, L., Nucita, A., Nunez, L. A., Pkala, J., Pena-Rodriguez, J., Armand, J. P., De Carvalho, W. R., Rojo, J. R., Gomez, J. D. S., Sanchez, F., Schafer, C. M., Schluter, F., Schovanek, P., Schroder, F. G., Schroder, S., Smida, R., Stanic, S., Suarez-Duran, M., Suomijarvi, T., Supik, J., Peixoto, C. J. T., Tome, B., Elipe, G. T., Galicia, J. F. V., Valino, I., Vliet, A. V., Cardenas, B. V., Vasquez-Ramirez, A., Veberic, D., Quispe, I. D. V., Villasenor, L., Wilczynski, H., High Energy Astrophys. & Astropart. Phys (API, FNWI), Research unit Astroparticle Physics, Physics, Elementary Particle Physics, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Institut de Physique Nucléaire d'Orsay (IPNO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Pierre Auger, Aab A., Abreu P., Aglietta M., Albury J.M., Allekotte I., Almela A., Castillo J.A., Alvarez-Muniz J., Batista R.A., Anastasi G.A., Anchordoqui L., Andrada B., Andringa S., Aramo C., Ferreira P.R.A., Asorey H., Assis P., Avila G., Badescu A.M., Bakalova A., Balaceanu A., Barbato F., Luz R.J.B., Becker K.H., Bellido J.A., Berat C., Bertaina M.E., Bertou X., Biermann P.L., Bister T., Biteau J., Blanco A., Blazek J., Bleve C., Bohacova M., Boncioli D., Bonifazi C., Arbeletche L.B., Borodai N., Botti A.M., Brack J., Bretz T., Briechle F.L., Buchholz P., Bueno A., Buitink S., Buscemi M., Caballero-Mora K.S., Caccianiga L., Calcagni L., Cancio A., Canfora F., Caracas I., Carceller J.M., Caruso R., Castellina A., Catalani F., Cataldi G., Cazon L., Cerda M., Chinellato J.A., Choi K., Chudoba J., Chytka L., Clay R.W., Cerutti A.C.C., Colalillo R., Coleman A., Coluccia M.R., Conceicao R., Condorelli A., Consolati G., Contreras F., Convenga F., Covault C.E., Dasso S., Daumiller K., Dawson B.R., Day J.A., De Almeida R.M., De Jesus J., De Jong S.J., Mauro G.D., Neto J.R.T.D.M., De Mitri I., De Oliveira J., De Oliveira Franco D., De Souza V., De Vito E., Debatin J., Del Rio M., Deligny O., Dhital N., Di Matteo A., Castro M.L.D., Dobrigkeit C., D'Olivo J.C., Dorosti Q., Dos Anjos R.C., Dova M.T., Ebr J., Engel R., Epicoco I., Erdmann M., Escobar C.O., Etchegoyen A., Falcke H., Farmer J., Farrar G., Fauth A.C., Fazzini N., Feldbusch F., Fenu F., Fick B., Figueira J.M., Filipcic A., Fodran T., Freire M.M., Fujii T., Fuster A., Galea C., Galelli C., Garcia B., Vegas A.L.G., Gemmeke H., Gesualdi F., Gherghel-Lascu A., Ghia P.L., Giaccari U., Giammarchi M., Giller M., Glombitza J., Gobbi F., Gollan F., Golup G., Berisso M.G., Vitale P.F.G., Gongora J.P., Gonzalez N., Goos I., Gora D., Gorgi A., Gottowik M., Grubb T.D., Guarino F., Guedes G.P., Guido E., Hahn S., Halliday R., Hampel M.R., Hansen P., Harari D., Harvey V.M., Haungs A., Hebbeker T., Heck D., Hill G.C., Hojvat C., Horandel J.R., Horvath P., Hrabovsky M., Huege T., Hulsman J., Insolia A., Isar P.G., Johnsen J.A., Jurysek J., Kaapa A., Kampert K.H., Keilhauer B., Kemp J., Klages H.O., Kleifges M., Kleinfeller J., Kopke M., Mezek G.K., Lago B.L., Lahurd D., Lang R.G., De Oliveira M.A.L., Lenok V., Letessier-Selvon A., Lhenry-Yvon I., Presti D.L., Lopes L., Lopez R., Lorek R., Luce Q., Lucero A., Payeras A.M., Malacari M., Mancarella G., Mandat D., Manning B.C., Manshanden J., Mantsch P., Marafico S., Mariazzi A.G., Maris I.C., Marsella G., Martello D., Martinez H., Bravo O.M., Mastrodicasa M., Mathes H.J., Matthews J., Matthiae G., Mayotte E., Mazur P.O., Medina-Tanco G., Melo D., Menshikov A., Merenda K.-D., Michal S., Micheletti M.I., Miramonti L., Mockler D., Mollerach S., Montanet F., Morello C., Mostafa M., Muller A.L., Muller M.A., Mulrey K., Mussa R., Muzio M., Namasaka W.M., Nellen L., Niculescu-Oglinzanu M., Niechciol M., Nitz D., Nosek D., Novotny V., Nozka L., Nucita A., Nunez L.A., Palatka M., Pallotta J., Panetta M.P., Papenbreer P., Parente G., Parra A., Pech M., Pedreira F., Pkala J., Pelayo R., Pena-Rodriguez J., Armand J.P., Perlin M., Perrone L., Peters C., Petrera S., Pierog T., Pimenta M., Pirronello V., Platino M., Pont B., Pothast M., Privitera P., Prouza M., Puyleart A., Querchfeld S., Rautenberg J., Ravignani D., Reininghaus M., Ridky J., Riehn F., Risse M., Ristori P., Rizi V., De Carvalho W.R., Rojo J.R., Roncoroni M.J., Roth M., Roulet E., Rovero A.C., Ruehl P., Saffi S.J., Saftoiu A., Salamida F., Salazar H., Salina G., Gomez J.D.S., Sanchez F., Santos E.M., Santos E., Sarazin F., Sarmento R., Sarmiento-Cano C., Sato R., Savina P., Schafer C.M., Scherini V., Schieler H., Schimassek M., Schimp M., Schluter F., Schmidt D., Scholten O., Schovanek P., Schroder F.G., Schroder S., Sciutto S.J., Scornavacche M., Shellard R.C., Sigl G., Silli G., Sima O., Smida R., Sommers P., Soriano J.F., Souchard J., Squartini R., Stadelmaier M., Stanca D., Stanic S., Stasielak J., Stassi P., Streich A., Suarez-Duran M., Sudholz T., Suomijarvi T., Supanitsky A.D., Supik J., Szadkowski Z., Taboada A., Tapia A., Timmermans C., Tkachenko O., Tobiska P., Peixoto C.J.T., Tome B., Elipe G.T., Travaini A., Travnicek P., Trimarelli C., Trini M., Tueros M., Ulrich R., Unger M., Urban M., Vaclavek L., Vacula M., Galicia J.F.V., Valino I., Valore L., Vliet A.V., Varela E., Cardenas B.V., Vasquez-Ramirez A., Veberic D., Ventura C., Quispe I.D.V., Verzi V., Vicha J., Villasenor L., Vink J., Vorobiov S., Wahlberg H., Watson A.A., Weber M., Weindl A., Wiencke L., Wilczynski H., Winchen T., Wirtz M., Wittkowski D., Wundheiler B., Yushkov A., Zapparrata O., Zas E., Zavrtanik D., Zavrtanik M., Zehrer L., Zepeda A., Ziolkowski M., and Zuccarello F.

Subjects
Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, Astronomy, 01 natural sciences, 030218 nuclear medicine & medical imaging, law.invention, 0302 clinical medicine, law, Observatory, atmosphere [muon], Instrumentation, physics.ins-det, Mathematical Physics, Large detector-systems performance, Physics, Instrumentation et méthodes en physique, Performance of high energy physics detectors, Data reduction methods, Large detector systems for particle and astroparticle physics, Detector, Settore FIS/01 - Fisica Sperimentale, Astrophysics::Instrumentation and Methods for Astrophysics, resistive plate chamber, Instrumentation and Detectors (physics.ins-det), trajectory [muon], Auger, observatory, muon: atmosphere, Astrophysics - Instrumentation and Methods for Astrophysics, atmosphere [showers], Cherenkov detector, air, Cherenkov counter: water, Astrophysics::High Energy Astrophysical Phenomena, UHE [cosmic radiation], FOS: Physical sciences, Cosmic ray, muon: trajectory, Nuclear physics, 03 medical and health sciences, Hodoscope, Data reduction method, 0103 physical sciences, Calibration, High Energy Physics, ddc:610, cosmic radiation: UHE, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Instrumentation and Methods for Astrophysics (astro-ph.IM), Zenith, Ciencias Exactas, Pierre Auger Observatory, showers: atmosphere, 010308 nuclear & particles physics, water [Cherenkov counter], hodoscope, Física, Autres mathématiques, stability, calibration, Data reduction methods, Large detector systems for particle and astroparticle physics, Large detector-systems performance, Performance of High Energy Physics Detectors, Experimental High Energy Physics, Large detector systems for particle and astroparticle physic, High Energy Physics::Experiment, RAIOS CÓSMICOS, astro-ph.IM
Abstract

Extensive air showers, originating from ultra-high energy cosmic rays, have been successfully measured through the use of arrays of water-Cherenkov detectors (WCDs). Sophisticated analyses exploiting WCD data have made it possible to demonstrate that shower simulations, based on different hadronic-interaction models, cannot reproduce the observed number of muons at the ground. The accurate knowledge of the WCD response to muons is paramount in establishing the exact level of this discrepancy. In this work, we report on a study of the response of a WCD of the Pierre Auger Observatory to atmospheric muons performed with a hodoscope made of resistive plate chambers (RPCs), enabling us to select and reconstruct nearly 600 thousand single muon trajectories with zenith angles ranging from 0º to 55º. Comparison of distributions of key observables between the hodoscope data and the predictions of dedicated simulations allows us to demonstrate the accuracy of the latter at a level of 2%. As the WCD calibration is based on its response to atmospheric muons, the hodoscope data are also exploited to show the long-term stability of the procedure., La lista completa de autores que integran el documento puede consultarse en el archivo., Facultad de Ciencias Exactas, Instituto de Física La Plata

Published
2020
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28. A 3-Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic-Ray Observatory

Author

B. García, M. L. Díaz Castro, G. Farrar, R. López, Karen S. Caballero-Mora, Francesca Zuccarello, Hernan Wahlberg, Q. Luce, Jose Chinellato, P. H. Nguyen, Martin Erdmann, Octavian Sima, J. Kleinfeller, H. J. Mathes, Z. Zong, G. Matthiae, R. R. Prado, F. Diogo, E. M. Santos, M. Schauer, A. Streich, Gioacchino Alex Anastasi, Stanislav Michal, A. Taboada, A. Letessier-Selvon, A. Parra, Antonio Bueno, Daniel Kuempel, M. Wirtz, Isabel Goos, Lorenzo Cazon, R. M. de Almeida, Kevin-Druis Merenda, D. Heck, G. P. Guedes, Roger W Clay, A. van Vliet, Frank G. Schröder, Toshihiro Fujii, P. Ristori, M. del Río, Bruce R. Dawson, Tim Huege, M. Trini, P.F. Gómez Vitale, Gualberto Avila, P.O. Mazur, David Wittkowski, J. Rodriguez Rojo, Jakub Juryšek, J. Debatin, Ivone F. M. Albuquerque, Angela V. Olinto, G. Salina, Danielle LaHurd, Olivier Deligny, Charles Timmermans, Lukas Middendorf, Fridtjof Feldbusch, Ioana Codrina Maris, M. I. Micheletti, Antonio Condorelli, R. Lorek, Giuseppe De Mauro, J. F. Valdés Galicia, G. C. Hill, Ugo Giaccari, Jorge F. Soriano, Enrique Zas, A. Cancio, Ralph Engel, Rodrigo Pelayo, Q. Dorosti, J. Ridky, Stijn Buitink, Christine Peters, M. Scornavacche, M. Zavrtanik, M. Schimp, M. Risse, Juan Carlos D'Olivo, T. Pierog, Justin M. Albury, Max Malacari, Lili Yang, Markus Roth, I. Allekotte, John Farmer, Piotr Homola, Fernando Contreras, E.M. Holt, Giovanni Consolati, B. C. Manning, Jonathan Blazek, R. Ramos-Pollan, L. Nellen, Piera Luisa Ghia, M. Josebachuili, C. Morello, A. Tapia, Jonathan Biteau, Dariusz Gora, Maria-Teresa Dova, Giovanni Marsella, D. Nosek, Luis A. Anchordoqui, Benedikt Zimmermann, Rúben Conceição, E. Santos, Alessio Gorgi, A. C. Fauth, Vladimir Lenok, L. Perrone, M. A. Leigui de Oliveira, A.M. van den Berg, Darko Veberič, G. Torralba Elipe, Philipp Papenbreer, G. Parente, Fabrizia Canfora, A. Aab, R. Krause, L. Valore, G. Morlino, Hernán Asorey, A. Bridgeman, Esteban Roulet, Petr Travnicek, Carla Bonifazi, S. J. Saffi, Alan Coleman, Trent D. Grubb, Jose A. Bellido, Carola Dobrigkeit, L. Zehrer, Thomas Harrison, D. Melo, R. Legumina, G. Kukec Mezek, M. J. Roncoroni, D. Nitz, Nicolas Martin Gonzalez, Peter L. Biermann, R.C. dos Anjos, L. A. S. Pereira, M.P. Panetta, Petr Schovanek, A. Puyleart, Corinne Berat, M. Giller, S. Baur, M. Stolpovskiy, Juan Manuel Figueira, Roberta Colalillo, M. Palatka, Jan Pękala, A. G. Mariazzi, M. Perlin, Luis Villaseñor, Alan Watson, M. E. Bertaina, A. Menshikov, F. Pedreira, J. Phuntsok, A. Weindl, Raul Sarmento, Paolo Privitera, D. Lo Presti, S. J. De Jong, Patricia María Hansen, Marvin Gottowik, N. Kemmerich, Martina Bohacova, K.-H. Becker, M. Pimenta, Eric Mayotte, Jeffrey A. Johnsen, S. Quinn, Xavier Bertou, Felix Schlüter, Mihai Niculescu-Oglinzanu, A. Zepeda, L. R. Wiencke, I.D. Vergara Quispe, J. Alvarez Castillo, P. Ruehl, Pedro Assis, Maximilian Reininghaus, M. Schimassek, J. de Oliveira, Alejandro Almela, C. Hojvat, Marco Giammarchi, Jan Ebr, Fabian Gobbi, Jarryd A. Day, A. Etchegoyen, David Schmidt, A. M. Botti, Roberto Mussa, M. Gómez Berisso, R. C. Shellard, Juan Pablo Gongora, Günter Sigl, Tobias Winchen, R. Sato, Florian Lukas Briechle, Denis Stanca, P. Stassi, Paul Sommers, Radomir Smida, F. Guarino, John Matthews, A. Blanco, O. C. Lippmann, A.C. Cobos Cerutti, B. Vargas Cárdenas, T. Suomijärvi, Peter Buchholz, J. Pallotta, C. Sarmiento-Cano, Jacco Vink, Thomas Bretz, H.O. Klages, Corbin Covault, J. R. T. de Mello Neto, Miroslav Hrabovský, M. Urban, M. Mastrodicasa, Matias Tueros, François Montanet, Lourenco Lopes, Mario Buscemi, B. L. Lago, S. Schröder, M. J. Cooper, F. Sánchez, V. de Souza, A. C. Rovero, Niraj Dhital, J. Rautenberg, C. Bleve, M. Wiedeński, Marco Aglietta, Dusan Mandat, I. Valiño, Matías Rolf Hampel, Alexandru Balaceanu, A. Haungs, Francesco Fenu, A. Kuotb Awad, S. G. Blaess, Lino Miramonti, A. A. Nucita, Jaime Alvarez-Muñiz, Jesús Peña-Rodríguez, P. Abreu, B. Mitrica, D. Ravignani, Heino Falcke, V. Novotny, Alexandru Gherghel-Lascu, Eleonora Guido, Rossella Caruso, A. Lucero, Fernando Catalani, S. Mathys, Luis A. Nunez, I. Jandt, Ralf Ulrich, Marcio Aparecido Muller, M. Suárez-Durán, Carla Aramo, Jörg R. Hörandel, P. Mantsch, J. Vicha, Z. Szadkowski, Daniela Mockler, Vincenzo Rizi, Julien Souchard, D. Martello, I. Lhenry-Yvon, Miroslav Pech, M. Ziolkowski, M. Platino, F.O. de Oliveira Salles, P. Savina, G. Golup, Paula Gina Isar, Maria Rita Coluccia, Bruno Daniel, G. Mancarella, B. Keilhauer, Pavel Horvath, W. Rodrigues de Carvalho, Marcus Niechciol, Silvia Mollerach, O. Martínez Bravo, Julian Kemp, Rodrigo Guedes Lang, Belén Andrada, S. J. Sciutto, P. van Bodegom, S. Müller, Juan Miguel Carceller, Alex Kääpä, S. Querchfeld, Nataliia Borodai, N. Fazzini, Jonas Glombitza, F. C. T. Barbato, A. Fuster, Sofia Andringa, H. Gemmeke, M. Unger, A. D. Supanitsky, J. Šupík, Carlo Ventura, Andrej Dundovic, Lorenzo Caccianiga, B. Wundheiler, Andres Travaini, Gregory R Snow, E. Varela, J.D. Sanabria Gomez, J. Chudoba, H. Schieler, Karl-Heinz Kampert, Ladislav Chytka, L. Calcagni, Kai Daumiller, Antonella Castellina, Alena Bakalova, J. Stasielak, S. Coutu, Gaia Silli, P. Heimann, Serguei Vorobiov, A. Filipčič, Federico Suarez, O. A. Taborda, C. Porowski, H. Martinez, F. Sarazin, Marcos Cerda, Denise Boncioli, G. Cataldi, V. Scherini, Valerio Verzi, B. Tome, Alexandra Saftoiu, Thomas Hebbeker, S. Petrera, Marc Weber, Sergio Dasso, Tristan Sudholz, Ivan De Mitri, Martín Miguel Freire, Jeffrey Brack, Olaf Scholten, Humberto Ibarguen Salazar, F. Riehn, Miguel Mostafa, C. O. Escobar, A. Insolia, M. Kleifges, D. Zavrtanik, A. López Casado, Samo Stanič, Dariusz Glas, Bjarni Pont, R.J. Barreira Luz, Johannes Schumacher, Violet M. Harvey, D. Harari, F. Salamida, A. Yushkov, L.P. Ferreyro, Alina Mihaela Badescu, M. Prouza, R. Squartini, Alfred Müller, G. Medina-Tanco, R. Halliday, J. Hulsman, J. Poh, Valerio Pirronello, C. J. Todero Peixoto, L. Noža, H. Wilczyński, Aab A., Abreu P., Aglietta M., Albuquerque I.F.M., Albury J.M., Allekotte I., Almela A., Alvarez Castillo J., Alvarez-Muniz J., Anastasi G.A., Anchordoqui L., Andrada B., Andringa S., Aramo C., Asorey H., Assis P., Avila G., Badescu A.M., Bakalova A., Balaceanu A., Barbato F., Barreira Luz R.J., Baur S., Becker K.H., Bellido J.A., Berat C., Bertaina M.E., Bertou X., Biermann P.L., Biteau J., Blaess S.G., Blanco A., Blazek J., Bleve C., Bohacova M., Boncioli D., Bonifazi C., Borodai N., Botti A.M., Brack J., Bretz T., Bridgeman A., Briechle F.L., Buchholz P., Bueno A., Buitink S., Buscemi M., Caballero-Mora K.S., Caccianiga L., Calcagni L., Cancio A., Canfora F., Carceller J.M., Caruso R., Castellina A., Catalani F., Cataldi G., Cazon L., Cerda M., Chinellato J.A., Chudoba J., Chytka L., Clay R.W., Cobos Cerutti A.C., Colalillo R., Coleman A., Coluccia M.R., Conceicao R., Condorelli A., Consolati G., Contreras F., Cooper M.J., Coutu S., Covault C.E., Daniel B., Dasso S., Daumiller K., Dawson B.R., Day J.A., de Almeida R.M., de Jong S.J., Mauro G., de Mello Neto J.R.T., Mitri I., de Oliveira J., de Oliveira Salles F.O., de Souza V., Debatin J., del Rio M., Deligny O., Dhital N., Diaz Castro M.L., Diogo F., Dobrigkeit C., D'Olivo J.C., Dorosti Q., dos Anjos R.C., Dova M.T., Dundovic A., Ebr J., Engel R., Erdmann M., Escobar C.O., Etchegoyen A., Falcke H., Farmer J., Farrar G., Fauth A.C., Fazzini N., Feldbusch F., Fenu F., Ferreyro L.P., Figueira J.M., Filipcic A., Freire M.M., Fujii T., Fuster A., Garcia B., Gemmeke H., Gherghel-Lascu A., Ghia P.L., Giaccari U., Giammarchi M., Giller M., Glas D., Glombitza J., Gobbi F., Golup G., Gomez Berisso M., Gomez Vitale P.F., Gongora J.P., Gonzalez N., Goos I., Gora D., Gorgi A., Gottowik M., Grubb T.D., Guarino F., Guedes G.P., Guido E., Halliday R., Hampel M.R., Hansen P., Harari D., Harrison T.A., Harvey V.M., Haungs A., Hebbeker T., Heck D., Heimann P., Hill G.C., Hojvat C., Holt E.M., Homola P., Horandel J.R., Horvath P., Hrabovsky M., Huege T., Hulsman J., Insolia A., Isar P.G., Jandt I., Johnsen J.A., Josebachuili M., Jurysek J., Kaapa A., Kampert K.H., Keilhauer B., Kemmerich N., Kemp J., Klages H.O., Kleifges M., Kleinfeller J., Krause R., Kuempel D., Kukec Mezek G., Kuotb Awad A., Lago B.L., LaHurd D., Lang R.G., Legumina R., Leigui de Oliveira M.A., Lenok V., Letessier-Selvon A., Lhenry-Yvon I., Lippmann O.C., Lo Presti D., Lopes L., Lopez R., Lopez Casado A., Lorek R., Luce Q., Lucero A., Malacari M., Mancarella G., Mandat D., Manning B.C., Mantsch P., Mariazzi A.G., Maris I.C., Marsella G., Martello D., Martinez H., Martinez Bravo O., Mastrodicasa M., Mathes H.J., Mathys S., Matthews J., Matthiae G., Mayotte E., Mazur P.O., Medina-Tanco G., Melo D., Menshikov A., Merenda K.-D., Michal S., Micheletti M.I., Middendorf L., Miramonti L., Mitrica B., Mockler D., Mollerach S., Montanet F., Morello C., Morlino G., Mostafa M., Muller A.L., Muller M.A., Muller S., Mussa R., Nellen L., Nguyen P.H., Niculescu-Oglinzanu M., Niechciol M., Nitz D., Nosek D., Novotny V., Noza L., Nucita A., Nunez L.A., Olinto A., Palatka M., Pallotta J., Panetta M.P., Papenbreer P., Parente G., Parra A., Pech M., Pedreira F., Pekala J., Pelayo R., Pena-Rodriguez J., Pereira L.A.S., Perlin M., Perrone L., Peters C., Petrera S., Phuntsok J., Pierog T., Pimenta M., Pirronello V., Platino M., Poh J., Pont B., Porowski C., Prado R.R., Privitera P., Prouza M., Puyleart A., Querchfeld S., Quinn S., Ramos-Pollan R., Rautenberg J., Ravignani D., Reininghaus M., Ridky J., Riehn F., Risse M., Ristori P., Rizi V., Rodrigues de Carvalho W., Rodriguez Rojo J., Roncoroni M.J., Roth M., Roulet E., Rovero A.C., Ruehl P., Saffi S.J., Saftoiu A., Salamida F., Salazar H., Salina G., Sanabria Gomez J.D., Sanchez F., Santos E.M., Santos E., Sarazin F., Sarmento R., Sarmiento-Cano C., Sato R., Savina P., Schauer M., Scherini V., Schieler H., Schimassek M., Schimp M., Schluter F., Schmidt D., Scholten O., Schovanek P., Schroder F.G., Schroder S., Schumacher J., Sciutto S.J., Scornavacche M., Shellard R.C., Sigl G., Silli G., Sima O., Smida R., Snow G.R., Sommers P., Soriano J.F., Souchard J., Squartini R., Stanca D., Stanic S., Stasielak J., Stassi P., Stolpovskiy M., Streich A., Suarez F., Suarez-Duran M., Sudholz T., Suomijarvi T., Supanitsky A.D., Supik J., Szadkowski Z., Taboada A., Taborda O.A., Tapia A., Timmermans C., Todero Peixoto C.J., Tome B., Torralba Elipe G., Travaini A., Travnicek P., Trini M., Tueros M., Ulrich R., Unger M., Urban M., Valdes Galicia J.F., Valino I., Valore L., van Bodegom P., van den Berg A.M., van Vliet A., Varela E., Vargas Cardenas B., Veberic D., Ventura C., Vergara Quispe I.D., Verzi V., Vicha J., Villasenor L., Vink J., Vorobiov S., Wahlberg H., Watson A.A., Weber M., Weindl A., Wiedenski M., Wiencke L., Wilczynski H., Winchen T., Wirtz M., Wittkowski D., Wundheiler B., Yang L., Yushkov A., Zas E., Zavrtanik D., Zavrtanik M., Zehrer L., Zepeda A., Zimmermann B., Ziolkowski M., Zong Z., Zuccarello F., Aab, A., Abreu, P., Aglietta, M., Albuquerque, I. F. M., Albury, J. M., Allekotte, I., Almela, A., Alvarez Castillo, J., Alvarez-Muniz, J., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Asorey, H., Assis, P., Avila, G., Badescu, A. M., Bakalova, A., Balaceanu, A., Barbato, F., Barreira Luz, R. J., Baur, S., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Biteau, J., Blaess, S. G., Blanco, A., Blazek, J., Bleve, C., Bohacova, M., Boncioli, D., Bonifazi, C., Borodai, N., Botti, A. M., Brack, J., Bretz, T., Bridgeman, A., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero-Mora, K. S., Caccianiga, L., Calcagni, L., Cancio, A., Canfora, F., Carceller, J. M., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Cerda, M., Chinellato, J. A., Chudoba, J., Chytka, L., Clay, R. W., Cobos Cerutti, A. C., Colalillo, R., Coleman, A., Coluccia, M. R., Conceicao, R., Condorelli, A., Consolati, G., Contreras, F., Cooper, M. J., Coutu, S., Covault, C. E., Daniel, B., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., de Almeida, R. M., de Jong, S. J., Mauro, G., de Mello Neto, J. R. T., Mitri, I., de Oliveira, J., de Oliveira Salles, F. O., de Souza, V., Debatin, J., del Rio, M., Deligny, O., Dhital, N., Diaz Castro, M. L., Diogo, F., Dobrigkeit, C., D'Olivo, J. C., Dorosti, Q., dos Anjos, R. C., Dova, M. T., Dundovic, A., Ebr, J., Engel, R., Erdmann, M., Escobar, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Ferreyro, L. P., Figueira, J. M., Filipcic, A., Freire, M. M., Fujii, T., Fuster, A., Garcia, B., Gemmeke, H., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., Glas, D., Glombitza, J., Gobbi, F., Golup, G., Gomez Berisso, M., Gomez Vitale, P. F., Gongora, J. P., Gonzalez, N., Goos, I., Gora, D., Gorgi, A., Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Halliday, R., Hampel, M. R., Hansen, P., Harari, D., Harrison, T. A., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Hill, G. C., Hojvat, C., Holt, E. M., Homola, P., Horandel, J. R., Horvath, P., Hrabovsky, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Jandt, I., Johnsen, J. A., Josebachuili, M., Jurysek, J., Kaapa, A., Kampert, K. H., Keilhauer, B., Kemmerich, N., Kemp, J., Klages, H. O., Kleifges, M., Kleinfeller, J., Krause, R., Kuempel, D., Kukec Mezek, G., Kuotb Awad, A., Lago, B. L., Lahurd, D., Lang, R. G., Legumina, R., Leigui de Oliveira, M. A., Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Lippmann, O. C., Lo Presti, D., Lopes, L., Lopez, R., Lopez Casado, A., Lorek, R., Luce, Q., Lucero, A., Malacari, M., Mancarella, G., Mandat, D., Manning, B. C., Mantsch, P., Mariazzi, A. G., Maris, I. C., Marsella, G., Martello, D., Martinez, H., Martinez Bravo, O., Mastrodicasa, M., Mathes, H. J., Mathys, S., Matthews, J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina-Tanco, G., Melo, D., Menshikov, A., Merenda, K. -D., Michal, S., Micheletti, M. I., Middendorf, L., Miramonti, L., Mitrica, B., Mockler, D., Mollerach, S., Montanet, F., Morello, C., Morlino, G., Mostafa, M., Muller, A. L., Muller, M. A., Muller, S., Mussa, R., Nellen, L., Nguyen, P. H., Niculescu-Oglinzanu, M., Niechciol, M., Nitz, D., Nosek, D., Novotny, V., Noza, L., Nucita, A., Nunez, L. A., Olinto, A., Palatka, M., Pallotta, J., Panetta, M. P., Papenbreer, P., Parente, G., Parra, A., Pech, M., Pedreira, F., Pekala, J., Pelayo, R., Pena-Rodriguez, J., Pereira, L. A. S., Perlin, M., Perrone, L., Peters, C., Petrera, S., Phuntsok, J., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Poh, J., Pont, B., Porowski, C., Prado, R. R., Privitera, P., Prouza, M., Puyleart, A., Querchfeld, S., Quinn, S., Ramos-Pollan, R., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Ristori, P., Rizi, V., Rodrigues de Carvalho, W., Rodriguez Rojo, J., Roncoroni, M. J., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Salina, G., Sanabria Gomez, J. D., Sanchez, F., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Savina, P., Schauer, M., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schluter, F., Schmidt, D., Scholten, O., Schovanek, P., Schroder, F. G., Schroder, S., Schumacher, J., Sciutto, S. J., Scornavacche, M., Shellard, R. C., Sigl, G., Silli, G., Sima, O., Smida, R., Snow, G. R., Sommers, P., Soriano, J. F., Souchard, J., Squartini, R., Stanca, D., Stanic, S., Stasielak, J., Stassi, P., Stolpovskiy, M., Streich, A., Suarez, F., Suarez-Duran, M., Sudholz, T., Suomijarvi, T., Supanitsky, A. D., Supik, J., Szadkowski, Z., Taboada, A., Taborda, O. A., Tapia, A., Timmermans, C., Todero Peixoto, C. J., Tome, B., Torralba Elipe, G., Travaini, A., Travnicek, P., Trini, M., Tueros, M., Ulrich, R., Unger, M., Urban, M., Valdes Galicia, J. F., Valino, I., Valore, L., van Bodegom, P., van den Berg, A. M., van Vliet, A., Varela, E., Vargas Cardenas, B., Veberic, D., Ventura, C., Vergara Quispe, I. D., Verzi, V., Vicha, J., Villasenor, L., Vink, J., Vorobiov, S., Wahlberg, H., Watson, A. A., Weber, M., Weindl, A., Wiedenski, M., Wiencke, L., Wilczynski, H., Winchen, T., Wirtz, M., Wittkowski, D., Wundheiler, B., Yang, L., Yushkov, A., Zas, E., Zavrtanik, D., Zavrtanik, M., Zehrer, L., Zepeda, A., Zimmermann, B., Ziolkowski, M., Zong, Z., Zuccarello, F., Physics, ITA, and Research unit Astroparticle Physics

Subjects
010504 meteorology & atmospheric sciences, Astronomy, Field of view, 010502 geochemistry & geophysics, 01 natural sciences, 7. Clean energy, Auger, lcsh:QB1-991, Observatory, ultraviolet, Storm, ddc:550, UHE Cosmic Rays, time resolution, Cosmic-ray observatory, Physics, lcsh:QE1-996.5, astro-ph, Geology, width [beam], Ionosphere, lcsh:Astronomy, UHE [cosmic radiation], Environmental Science (miscellaneous), horizon, Lightning, ddc:530, High Energy Physics, 0105 earth and related environmental sciences, fluorescence [detector], background, Física, sensitivity, optics, lcsh:Geology, Elves, UV fluorescence detectors, Thunderstorm, 13. Climate action, Experimental High Energy Physics, network, General Earth and Planetary Sciences, Elves
Abstract

The time and location of the 1,598 verified and reconstructed elves, used for the analysis showcased in this paper, are publicly available on the website of the Pierre Auger Observatory (https://www.auger.org/ index.php/science/data). We wish to thank the World Wide Lightning Location Network (http://wwlln.net), a collaboration among over 50 universities and institutions, for providing the lightning location data used in this paper. We acknowledge Robert Marshall for providing one of the most advanced elve simulations to the public, a key tool in understanding the elves observed by the Pierre Auger Observatory. The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargüe., Elves are a class of transient luminous events, with a radial extent typically greater than 250 km, that occur in the lower ionosphere above strong electrical storms. We report the observation of 1,598 elves, from 2014 to 2016, recorded with unprecedented time resolution (100 ns) using the fluorescence detector (FD) of the Pierre Auger Cosmic-Ray Observatory. The Auger Observatory is located in the Mendoza province of Argentina with a viewing footprint for elve observations of 3 · 106 km2, reaching areas above the Pacific and Atlantic Oceans, as well as the Córdoba region, which is known for severe convective thunderstorms. Primarily designed for ultrahigh energy cosmic-ray observations, the Auger FD turns out to be very sensitive to the ultraviolet emission in elves. The detector features modified Schmidt optics with large apertures resulting in a field of view that spans the horizon, and year-round operation on dark nights with low moonlight background, when the local weather is favorable. The measured light profiles of 18% of the elve events have more than one peak, compatible with intracloud activity. Within the 3-year sample, 72% of the elves correlate with the far-field radiation measurements of the World Wide Lightning Location Network. The Auger Observatory plans to continue operations until at least 2025, including elve observations and analysis. To the best of our knowledge, this observatory is the only facility on Earth that measures elves with year-round operation and full horizon coverage., Argentina—Comisión Nacional de Energía Atómica; Agencia Nacional de Promoción Científica y Tecnológica (ANPCyT); Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET); Gobierno de la Provincia de Mendoza; Municipalidad de Malargüe; and NDM Holdings and Valle Las Leñas, in gratitude for their continuing cooperation over land access; Australia—the Australian Research Council; Brazil—Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq); Financiadora de Estudos e Projetos (FINEP); Fundação de Amparo à Pesquisa do Estado de Rio de Janeiro (FAPERJ); São Paulo Research Foundation (FAPESP) Grants 2010/07359-6 and 1999/05404-3; Ministério da Ciência, Tecnologia, Inovações e Comunicações (MCTIC); Czech Republic—Grants MSMT CRLTT18004, LO1305, LM2015038, and CZ.02.1.01/0.0/0.0/16_013/0001402; France—Centre de Calcul IN2P3/CNRS; Centre National de la Recherche Scientifique (CNRS); Conseil Régional Ile-de-France; Département Physique Nucléaire et Corpusculaire (PNC-IN2P3/CNRS); Département Sciences de l'Univers (SDU-INSU/CNRS); Institut Lagrange de Paris (ILP) Grant LABEX ANR-10-LABX-63 within the Investissements d'Avenir Programme Grant ANR-11-IDEX-0004-02; Germany—Bundesministerium für Bildung und Forschung (BMBF); Deutsche Forschungsgemeinschaft (DFG); Finanzministerium Baden-Württemberg; Helmholtz Alliance for Astroparticle Physics (HAP); Helmholtz-Gemeinschaft. Deutscher Forschungszentren (HGF); Ministerium für Innovation, Wissenschaft und Forschung des Landes Nordrhein-Westfalen; Ministerium für Wissenschaft, Forschung und Kunst des Landes Baden-Württemberg; Italy—Istituto Nazionale di Fisica Nucleare (INFN); Istituto Nazionale di Astrofisica (INAF); Ministero dell'Istruzione, dell'Universitá e della Ricerca (MIUR); CETEMPS Center of Excellence; Ministero degli Affari Esteri (MAE); México—Consejo Nacional de Ciencia y Tecnología (CONACYT)167733; Universidad Nacional Autónoma de México (UNAM); PAPIIT DGAPA-UNAM; The Netherlands—Ministry of Education, Culture and Science; Netherlands Organisation for Scientific Research (NWO); Dutch National e-Infrastructure with the support of SURF Cooperative; Poland—National Centre for Research and Development, Grant ERA-NET-ASPERA/02/11; National Science Centre, Grants 2013/08/M/ST9/00322, 2016/23/B/ST9/01635, and HARMONIA 5–2013/10/M/ST9/00062, UMO-2016/22/M/ST9/00198; Portugal—Portuguese national funds and FEDER funds within Programa Operacional Factores de Competitividade through Fundação para a Ciência e a Tecnologia (COMPETE); Romania—Romanian Ministry of Research and InnovationCNCS/CCCDI-UESFISCDI, projects PN-III-P1-1.2-PCCDI-2017- 0839/19PCCDI/2018, PN-III-P2-2.1-PED-2016-1922, PN-III-P2-2.1-PED-2016-1659, and PN18090102 within PNCDI III; Slovenia—Slovenian Research Agency; Spain—Comunidad de Madrid; Fondo Europeo de Desarrollo Regional (FEDER) funds; Ministerio de Economía y Competitividad; Xunta de Galicia; European Community 7th Framework Program Grant FP7-PEOPLE-2012-IEF-328826; USA—Department of Energy, Contracts DE-AC02-07CH11359, DE-FR02-04ER41300, DE-FG02-99ER41107, and DE-SC0011689; National Science Foundation, Grant 0450696; The Grainger Foundation; Marie Curie-IRSES/EPLANET; European Particle Physics Latin American Network; European Union 7th Framework Program, Grant PIRSES-2009-GA-246806; and UNESCO.

Published
2020

29. Reconstruction of events recorded with the surface detector of the Pierre Auger Observatory

Author

Roberto Mussa, M. I. Micheletti, B. Tome, François Montanet, M. Schimassek, Frank G. Schröder, Peter Hansen, F. Guarino, John Matthews, Ioana Codrina Maris, Peter Buchholz, C. Hojvat, G. C. Hill, Jorge F. Soriano, Vladimir Lenok, Ralph Engel, L. Perrone, Jan Ebr, J. Ridky, Denis Stanca, A. Aab, Brian Fick, Eleonora Guido, Luis Villaseñor, John Farmer, Marco Aglietta, Markus Roth, Lorenzo Caccianiga, Julien Manshanden, Andres Travaini, E. Varela, H. J. Mathes, Maximilian Reininghaus, J.D. Sanabria Gomez, L. Nellen, B. Vargas Cárdenas, Maria-Teresa Dova, Jacco Vink, H.O. Klages, P. Savina, W. Rodrigues de Carvalho, Bjarni Pont, Stanislav Michal, C. Morello, Miroslav Pech, T. Suomijärvi, J. Pallotta, Alena Bakalova, M. Pothast, Pavel Horvath, B. L. Lago, Ralf Ulrich, A. M. Botti, Dusan Mandat, M. L. Díaz Castro, Teresa Bister, Valerio Verzi, M. R. Hampel, Valerio Pirronello, Niraj Dhital, J. Rodriguez Rojo, I. Valiño, Marvin Gottowik, Peter L. Biermann, Jeffrey A. Johnsen, A. A. Nucita, B. Andrada, Fridtjof Feldbusch, L. Calcagni, C. J. Todero Peixoto, Carla Bleve, Rodrigo Guedes Lang, Eric Mayotte, M. Gómez Berisso, G. Farrar, R. C. Shellard, Francesca Zuccarello, K. Choi, Matias Tueros, Sofia Andringa, Paula Gina Isar, F. Riehn, Marina Scornavacche, Paolo Privitera, Kai Daumiller, Günter Sigl, Paul Sommers, A. Blanco, L. Nožka, Enrique Zas, Fernando Contreras, Fred Sarazin, G. De Mauro, Mario Buscemi, Luis A. Anchordoqui, P. Tobiska, A. C. Fauth, Nataliia Borodai, Philipp Papenbreer, Jonathan Biteau, Nicolás González, T. Huege, R.J. Barreira Luz, Petr Travnicek, M. Schimp, F. Sánchez, Antonio Condorelli, Christine Peters, Luis A. Nunez, H. Wilczyński, M. Zavrtanik, P. Stassi, Jörg R. Hörandel, Darko Veberič, R.C. dos Anjos, Radomir Smida, Adriana Vásquez-Ramírez, A. Machado Payeras, Carla Bonifazi, M. Palatka, B. C. Manning, Jose A. Bellido, Isabel Goos, Jeffrey Brack, Olaf Scholten, Trent D. Grubb, Christian Sarmiento-Cano, Humberto Ibarguen Salazar, Fabio Convenga, Martin Vacula, Marcus Niechciol, D. Heck, A.L. Garcia Vegas, R. Squartini, E. De Vito, Giovanni Consolati, M. A. Muller, Alfred Müller, A. Di Matteo, A. Taboada, M. del Río, I. Lhenry-Yvon, Juan Manuel Figueira, Jesús Peña-Rodríguez, Francesco Fenu, B. Wundheiler, A. Puyleart, Corinne Berat, M. Giller, Roberta Colalillo, Fernando Gollan, Maria Rita Coluccia, A. G. Mariazzi, Heino Falcke, A. Fuster, J. Vicha, S. Querchfeld, Gaia Silli, I.D. Vergara Quispe, P.F. Gómez Vitale, D. Nosek, M.P. Panetta, Miguel Mostafa, Petr Schovanek, G. Medina-Tanco, R. Halliday, Charles Timmermans, V. de Souza, Olena Tkachenko, Martina Bohacova, A. Filipčič, F. Salamida, Hernán Asorey, A. Yushkov, G. Matthiae, Antonio Bueno, E. Santos, J. Šupík, Carlo Ventura, Hernan Wahlberg, D. Melo, A. Tapia, Juan Pablo Gongora, G. Torralba Elipe, H. Gemmeke, J. Rautenberg, Gualberto Avila, S. Petrera, Marc Weber, Q. Luce, G. P. Guedes, Toshihiro Fujii, G. Marsella, Dariusz Gora, Ladislav Chytka, Massimo Mastrodicasa, L. Valore, M. Unger, D. Mockler, A. Parra, P. Ruehl, Samo Stanič, A. Weindl, E. M. Santos, Maximilian Stadelmaier, R. Sato, G. Golup, J. F. Valdés Galicia, I. De Mitri, Jakub Juryšek, J. Debatin, A. Bridgeman, Alan Coleman, V. Novotny, J. Hulsman, Rossella Caruso, A. Lucero, Fernando Catalani, David Schmidt, S. Schröder, S. J. Saffi, R. Alves Batista, Bruce R. Dawson, Caterina Trimarelli, Italo Epicoco, Steffen Hahn, P. Ristori, P.O. Mazur, Juan Carlos D'Olivo, T. Pierog, D. Lo Presti, Sullivan Marafico, M. Trini, M. A. Leigui de Oliveira, Xavier Bertou, A. Zepeda, Violet M. Harvey, D. Harari, Esteban Roulet, Pedro Assis, H. Martinez, S. J. De Jong, A. Etchegoyen, Justin M. Albury, Pierre Billoir, F. Pedreira, Marco Giammarchi, Raul Sarmento, Jarryd A. Day, A. Saftoiu, Felix Schlüter, A. Cancio, J. Stasielak, Fabian Gobbi, Piera Luisa Ghia, A.C. Cobos Cerutti, Thomas Hebbeker, Sergio Dasso, Tristan Sudholz, Alina Mihaela Badescu, Cristina Galea, Martín Miguel Freire, M. Prouza, J. R. T. de Mello Neto, I. Allekotte, M. J. Roncoroni, L. Bonneau Arbeletche, Denise Boncioli, R. M. de Almeida, Jose Chinellato, Rodrigo Pelayo, Stijn Buitink, Ioana Caracas, A. Letessier-Selvon, Lorenzo Cazon, Alessio Gorgi, Orazio Zapparrata, Carola Dobrigkeit, M. Muzio, A. van Vliet, David Wittkowski, G. Salina, Danielle LaHurd, Olivier Deligny, Tomáš Fodran, R. Lorek, Ugo Giaccari, Alan Watson, M. Perlin, Mihai Niculescu-Oglinzanu, J. Alvarez Castillo, Julian Kemp, R. Conceição, Miroslav Hrabovský, A. Haungs, P. Mantsch, Z. Szadkowski, Alex Kääpä, Octavian Sima, L. Lopes, Jaime Alvarez-Muñiz, H. Schieler, Alexandru Gherghel-Lascu, Q. Dorosti, Lukáš Vaclavek, G. Mancarella, B. Keilhauer, André Schulz, Karl-Heinz Kampert, S. J. Sciutto, Juan Miguel Carceller, Antonella Castellina, D. Nitz, M. Risse, L. R. Wiencke, Jonathan Blazek, C. M. Schäfer, G. Parente, Fabrizia Canfora, L. Zehrer, J. de Oliveira, Alejandro Almela, Thomas Bretz, Corbin Covault, G. Kukec Mezek, Lino Miramonti, M. E. Bertaina, D. de Oliveira Franco, A. Menshikov, P. Abreu, D. Ravignani, Marcel Köpke, M. Platino, Max Malacari, J. Perez Armand, Claudio Galelli, K.-H. Becker, M. Pimenta, P.R. Araújo Ferreira, Tobias Winchen, Florian Lukas Briechle, Silvia Mollerach, B. García, N. Fazzini, Jonas Glombitza, F. C. T. Barbato, R. López, Karen S. Caballero-Mora, Martin Erdmann, J. de Jesús, A. Streich, Gioacchino Alex Anastasi, M. Wirtz, J. Chudoba, Roger W Clay, G. Cataldi, V. Scherini, Serguei Vorobiov, A. Insolia, M. Kleifges, D. Zavrtanik, A.D. Supanitsky, J. Pȩkala, Flavia Gesualdi, Marcos Cerda, M. Urban, W. M. Namasaka, A. C. Rovero, Alexandru Balaceanu, M. Suárez-Durán, Carla Aramo, Vincenzo Rizi, Julien Souchard, D. Martello, M. Ziolkowski, O. Martínez Bravo, K. Mulrey, J. Kleinfeller, Carlos Escobar, Kevin-Druis Merenda, Aab, A., Abreu, P., Aglietta, M., Albury, J. M., Allekotte, I., Almela, A., Castillo, J. A., Alvarez-Muñiz, J., Batista, R. A., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Ferreira, P. R. A., Asorey, H., Assis, P., Avila, G., Badescu, A. M., Bakalova, A., Balaceanu, A., Barbato, F., Luz, R. J. B., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Billoir, P., Bister, T., Biteau, J., Blanco, A., Blazek, J., Bleve, C., Bohacova, M., Boncioli, D., Bonifazi, C., Arbeletche, L. B., Borodai, N., Botti, A. M., Brack, J., Bretz, T., Bridgeman, A., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero-Mora, K. S., Caccianiga, L., Calcagni, L., Cancio, A., Canfora, F., Caracas, I., Carceller, J. M., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Cerda, M., Chinellato, J. A., Choi, K., Chudoba, J., Chytka, L., Clay, R. W., Cerutti, A. C. C., Colalillo, R., Coleman, A., Coluccia, M. R., Conceicao, R., Condorelli, A., Consolati, G., Contreras, F., Convenga, F., Covault, C. E., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., De Almeida, R. M., De Jesus, J., De Jong, S. J., Mauro, G. D., Neto, J. R. T. D. M., Mitri, I. D., De Oliveira, J., Franco, D. D. O., De Souza, V., Vito, E. D., Debatin, J., Rio, M. D., Deligny, O., Dhital, N., Matteo, A. D., Castro, M. L. D., Dobrigkeit, C., D'Olivo, J. C., Dorosti, Q., Anjos, R. C. D., Dova, M. T., Ebr, J., Engel, R., Epicoco, I., Erdmann, M., Escobar, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Fick, B., Figueira, J. M., Filipcic, A., Fodran, T., Freire, M. M., Fujii, T., Fuster, A., Galea, C., Galelli, C., Garcia, B., Vegas, A. L. G., Gemmeke, H., Gesualdi, F., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., Glombitza, J., Gobbi, F., Gollan, F., Golup, G., Berisso, M. G., Vitale, P. F. G., Gongora, J. P., Gonzalez, N., Goos, I., Gora, D., Gorgi, A., Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Hahn, S., Halliday, R., Hampel, M. R., Hansen, P., Harari, D., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Hill, G. C., Hojvat, C., Horandel, J. R., Horvath, P., Hrabovsky, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Johnsen, J. A., Jurysek, J., Kaapa, A., Kampert, K. H., Keilhauer, B., Kemp, J., Klages, H. O., Kleifges, M., Kleinfeller, J., Kopke, M., Mezek, G. K., Lago, B. L., Lahurd, D., Lang, R. G., De Oliveira, M. A. L., Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Presti, D. L., Lopes, L., Lopez, R., Lorek, R., Luce, Q., Lucero, A., Payeras, A. M., Malacari, M., Mancarella, G., Mandat, D., Manning, B. C., Manshanden, J., Mantsch, P., Marafico, S., Mariazzi, A. G., Maris, I. C., Marsella, G., Martello, D., Martinez, H., Bravo, O. M., Mastrodicasa, M., Mathes, H. J., Matthews, J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina-Tanco, G., Melo, D., Menshikov, A., Merenda, K. -D., Michal, S., Micheletti, M. I., Miramonti, L., Mockler, D., Mollerach, S., Montanet, F., Morello, C., Mostafa, M., Muller, A. L., Muller, M. A., Mulrey, K., Mussa, R., Muzio, M., Namasaka, W. M., Nellen, L., Niculescu-Oglinzanu, M., Niechciol, M., Nitz, D., Nosek, D., Novotny, V., Nozka, L., Nucita, A., Nuñez, L. A., Palatka, M., Pallotta, J., Panetta, M. P., Papenbreer, P., Parente, G., Parra, A., Pech, M., Pedreira, F., Pkala, J., Pelayo, R., Peña-Rodriguez, J., Armand, J. P., Perlin, M., Perrone, L., Peters, C., Petrera, S., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Pont, B., Pothast, M., Privitera, P., Prouza, M., Puyleart, A., Querchfeld, S., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Ristori, P., Rizi, V., De Carvalho, W. R., Rojo, J. R., Roncoroni, M. J., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Salina, G., Gomez, J. D. S., Sanchez, F., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Savina, P., Schafer, C., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schluter, F., Schmidt, D., Scholten, O., Schovanek, P., Schroder, F. G., Schroder, S., Schulz, A., Sciutto, S. J., Scornavacche, M., Shellard, R. C., Sigl, G., Silli, G., Sima, O., Smida, R., Sommers, P., Soriano, J. F., Souchard, J., Squartini, R., Stadelmaier, M., Stanca, D., Stanic, S., Stasielak, J., Stassi, P., Streich, A., Suarez-Duran, M., Sudholz, T., Suomijarvi, T., Supanitsky, A. D., Supik, J., Szadkowski, Z., Taboada, A., Tapia, A., Timmermans, C., Tkachenko, O., Tobiska, P., Peixoto, C. J. T., Tome, B., Elipe, G. T., Travaini, A., Travnicek, P., Trimarelli, C., Trini, M., Tueros, M., Ulrich, R., Unger, M., Urban, M., Vaclavek, L., Vacula, M., Galicia, J. F. V., Valiño, I., Valore, L., Vliet, A. V., Varela, E., Cardenas, B. V., Vasquez-Ramirez, A., Veberic, D., Ventura, C., Quispe, I. D. V., Verzi, V., Vicha, J., Villaseñor, L., Vink, J., Vorobiov, S., Wahlberg, H., Watson, A. A., Weber, M., Weindl, A., Wiencke, L., Wilczynski, H., Winchen, T., Wirtz, M., Wittkowski, D., Wundheiler, B., Yushkov, A., Zapparrata, O., Zas, E., Zavrtanik, D., Zavrtanik, M., Zehrer, L., Zepeda, A., Ziolkowski, M., Zuccarello, F., Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut de Physique Nucléaire d'Orsay (IPNO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Pierre Auger, Research unit Astroparticle Physics, Physics, Elementary Particle Physics, Aab A., Abreu P., Aglietta M., Albury J.M., Allekotte I., Almela A., Castillo J.A., Alvarez-Muñiz J., Batista R.A., Anastasi G.A., Anchordoqui L., Andrada B., Andringa S., Aramo C., Ferreira P.R.A., Asorey H., Assis P., Avila G., Badescu A.M., Bakalova A., Balaceanu A., Barbato F., Luz R.J.B., Becker K.H., Bellido J.A., Berat C., Bertaina M.E., Bertou X., Biermann P.L., Billoir P., Bister T., Biteau J., Blanco A., Blazek J., Bleve C., Bohacova M., Boncioli D., Bonifazi C., Arbeletche L.B., Borodai N., Botti A.M., Brack J., Bretz T., Bridgeman A., Briechle F.L., Buchholz P., Bueno A., Buitink S., Buscemi M., Caballero-Mora K.S., Caccianiga L., Calcagni L., Cancio A., Canfora F., Caracas I., Carceller J.M., Caruso R., Castellina A., Catalani F., Cataldi G., Cazon L., Cerda M., Chinellato J.A., Choi K., Chudoba J., Chytka L., Clay R.W., Cerutti A.C.C., Colalillo R., Coleman A., Coluccia M.R., Conceicao R., Condorelli A., Consolati G., Contreras F., Convenga F., Covault C.E., Dasso S., Daumiller K., Dawson B.R., Day J.A., De Almeida R.M., De Jesus J., De Jong S.J., Mauro G.D., Neto J.R.T.D.M., Mitri I.D., De Oliveira J., Franco D.D.O., De Souza V., Vito E.D., Debatin J., Rio M.D., Deligny O., Dhital N., Matteo A.D., Castro M.L.D., Dobrigkeit C., D'Olivo J.C., Dorosti Q., Anjos R.C.D., Dova M.T., Ebr J., Engel R., Epicoco I., Erdmann M., Escobar C.O., Etchegoyen A., Falcke H., Farmer J., Farrar G., Fauth A.C., Fazzini N., Feldbusch F., Fenu F., Fick B., Figueira J.M., Filipcic A., Fodran T., Freire M.M., Fujii T., Fuster A., Galea C., Galelli C., Garcia B., Vegas A.L.G., Gemmeke H., Gesualdi F., Gherghel-Lascu A., Ghia P.L., Giaccari U., Giammarchi M., Giller M., Glombitza J., Gobbi F., Gollan F., Golup G., Berisso M.G., Vitale P.F.G., Gongora J.P., Gonzalez N., Goos I., Gora D., Gorgi A., Gottowik M., Grubb T.D., Guarino F., Guedes G.P., Guido E., Hahn S., Halliday R., Hampel M.R., Hansen P., Harari D., Harvey V.M., Haungs A., Hebbeker T., Heck D., Hill G.C., Hojvat C., Horandel J.R., Horvath P., Hrabovsky M., Huege T., Hulsman J., Insolia A., Isar P.G., Johnsen J.A., Jurysek J., Kaapa A., Kampert K.H., Keilhauer B., Kemp J., Klages H.O., Kleifges M., Kleinfeller J., Kopke M., Mezek G.K., Lago B.L., Lahurd D., Lang R.G., De Oliveira M.A.L., Lenok V., Letessier-Selvon A., Lhenry-Yvon I., Presti D.L., Lopes L., Lopez R., Lorek R., Luce Q., Lucero A., Payeras A.M., Malacari M., Mancarella G., Mandat D., Manning B.C., Manshanden J., Mantsch P., Marafico S., Mariazzi A.G., Maris I.C., Marsella G., Martello D., Martinez H., Bravo O.M., Mastrodicasa M., Mathes H.J., Matthews J., Matthiae G., Mayotte E., Mazur P.O., Medina-Tanco G., Melo D., Menshikov A., Merenda K.-D., Michal S., Micheletti M.I., Miramonti L., Mockler D., Mollerach S., Montanet F., Morello C., Mostafa M., Muller A.L., Muller M.A., Mulrey K., Mussa R., Muzio M., Namasaka W.M., Nellen L., Niculescu-Oglinzanu M., Niechciol M., Nitz D., Nosek D., Novotny V., Nozka L., Nucita A., Nuñez L.A., Palatka M., Pallotta J., Panetta M.P., Papenbreer P., Parente G., Parra A., Pech M., Pedreira F., Pkala J., Pelayo R., Peña-Rodriguez J., Armand J.P., Perlin M., Perrone L., Peters C., Petrera S., Pierog T., Pimenta M., Pirronello V., Platino M., Pont B., Pothast M., Privitera P., Prouza M., Puyleart A., Querchfeld S., Rautenberg J., Ravignani D., Reininghaus M., Ridky J., Riehn F., Risse M., Ristori P., Rizi V., De Carvalho W.R., Rojo J.R., Roncoroni M.J., Roth M., Roulet E., Rovero A.C., Ruehl P., Saffi S.J., Saftoiu A., Salamida F., Salazar H., Salina G., Gomez J.D.S., Sanchez F., Santos E.M., Santos E., Sarazin F., Sarmento R., Sarmiento-Cano C., Sato R., Savina P., Schafer C., Scherini V., Schieler H., Schimassek M., Schimp M., Schluter F., Schmidt D., Scholten O., Schovanek P., Schroder F.G., Schroder S., Schulz A., Sciutto S.J., Scornavacche M., Shellard R.C., Sigl G., Silli G., Sima O., Smida R., Sommers P., Soriano J.F., Souchard J., Squartini R., Stadelmaier M., Stanca D., Stanic S., Stasielak J., Stassi P., Streich A., Suarez-Duran M., Sudholz T., Suomijarvi T., Supanitsky A.D., Supik J., Szadkowski Z., Taboada A., Tapia A., Timmermans C., Tkachenko O., Tobiska P., Peixoto C.J.T., Tome B., Elipe G.T., Travaini A., Travnicek P., Trimarelli C., Trini M., Tueros M., Ulrich R., Unger M., Urban M., Vaclavek L., Vacula M., Galicia J.F.V., Valiño I., Valore L., Vliet A.V., Varela E., Cardenas B.V., Vasquez-Ramirez A., Veberic D., Ventura C., Quispe I.D.V., Verzi V., Vicha J., Villaseñor L., Vink J., Vorobiov S., Wahlberg H., Watson A.A., Weber M., Weindl A., Wiencke L., Wilczynski H., Winchen T., Wirtz M., Wittkowski D., Wundheiler B., Yushkov A., Zapparrata O., Zas E., Zavrtanik D., Zavrtanik M., Zehrer L., Zepeda A., Ziolkowski M., Zuccarello F., and High Energy Astrophys. & Astropart. Phys (API, FNWI)

Subjects
Physics::Instrumentation and Detectors, Astronomy, primary [cosmic radiation], 01 natural sciences, 030218 nuclear medicine & medical imaging, Auger, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), 0302 clinical medicine, surface [detector], Observatory, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Data Processing, Large detector systems for particle and astroparticle physics, Large detector-systems performance, Performance of High Energy Physics Detectors, Instrumentation, Mathematical Physics, Largedetector-systems performance, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, astro-ph.HE, Instrumentation et méthodes en physique, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, cascade, observatory, Cascade, ddc:620, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, atmosphere [showers], air, Astrophysics::High Energy Astrophysical Phenomena, water, FOS: Physical sciences, Cosmic ray, Atmosphere, 03 medical and health sciences, Optics, 0103 physical sciences, High Energy Physics, 14. Life underwater, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], ddc:610, Instrumentation and Methods for Astrophysics (astro-ph.IM), Zenith, Engineering & allied operations, Pierre Auger Observatory, showers: atmosphere, 010308 nuclear & particles physics, business.industry, hep-ex, detector: surface, Autres mathématiques, cosmic radiation: primary, Cherenkov counter, Experimental High Energy Physics, Large detector systems for particle and astroparticle physic, High Energy Physics::Experiment, business, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], RAIOS CÓSMICOS, astro-ph.IM
Abstract

Cosmic rays arriving at Earth collide with the upper parts of the atmosphere, thereby inducing extensive air showers. When secondary particles from the cascade arrive at the ground, they are measured by surface detector arrays. We describe the methods applied to the measurements of the surface detector of the Pierre Auger Observatory to reconstruct events with zenith angles less than 60 using the timing and signal information recorded using the water-Cherenkov detector stations. In addition, we assess the accuracy of these methods in reconstructing the arrival directions of the primary cosmic ray particles and the sizes of the induced showers., Argentina - Comisión Nacional de Energía Atómica, Argentina - Agencia Nacional de Promoción Científica y Tecnológica (ANPCyT), Argentina - Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET), Argentina - Gobierno de la Provincia de Mendoza, Argentina - Municipalidad de Malargue, Argentina - NDM Holdings, Argentina - Valle Las Lenas, Australia - Australian Research Council, National Council for Scientific and Technological Development (CNPq), Brazil - Financiadora de Estudos e Projetos (FINEP), Carlos Chagas Filho Foundation for Research Support of the State of Rio de Janeiro (FAPERJ), Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP) 2019/10151-2 2010/07359-6 1999/05404-3, Brazil - Ministerio da Ciencia, Tecnologia, Inovacoes e Comunicacoes (MCTIC), Czech Republic Grant MSMT CR LTT18004 LM2015038 LM2018102 CZ.02.1.01/0.0/0.0/16_013/0001402 CZ.02.1.01/0.0/0.0/18_046/0016010 CZ.02.1.01/0.0/0.0/17_049/0008422, France - Centre de Calcul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), France - Conseil Regional Ile-de-France, France - Departement Physique Nucleaire et Corpusculaire (PNC-IN2P3/CNRS), France - Departement Sciences de l'Univers (SDU-INSU/CNRS), French National Research Agency (ANR) LABEX ANR-10-LABX-63 ANR11-IDEX-0004-02, Federal Ministry of Education & Research (BMBF), German Research Foundation (DFG), Germany - Finanzministerium Baden-Wurttemberg, Germany - Helmholtz Alliance for Astroparticle Physics (HAP), Germany - Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF), Germany - Min-isterium fur Innovation, Wissenschaft und Forschung des Landes Nordrhein-Westfalen, Germany - Ministerium fur Wissenschaft, Forschung und Kunst des Landes Baden-Wurttemberg, Italy - Istituto Nazionale di Fisica Nucleare (INFN), Italy - Istituto Nazionale di Astrofisica (INAF), Italy - Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR), Italy - CETEMPS Center of Excellence, Italy - Ministero degli Affari Esteri (MAE), Consejo Nacional de Ciencia y Tecnología (CONACyT) 167733, México - Universidad Nacional Autónoma de México (UNAM), México - PAPIIT DGAPA-UNAM, The Netherlands - Ministry of Education, Culture and Science, Netherlands Organization for Scientific Research (NWO), The Netherlands - Dutch national e-infrastructure, The Netherlands - SURF Cooperative, Poland - Ministry of Science and Higher Education DIR/WK/2018/11, Poland - National Science Centre 2013/08/M/ST9/00322 2016/23/B/ST9/01635 HARMONIA 52013/10/M/ST9/00062 UMO-2016/22/M/ST9/00198, Portugal - Portuguese national funds, Portugal - FEDER funds within Programa Operacional Factores de Competitividade through Fundacao para a Ciencia e a Tecnologia (COMPETE), Romania - Romanian Ministry of Education and Research, the Program Nucleu within MCI PN19150201/16N/2019 PN19060102, Romania - Romanian Ministry of Education and Research, the Program Nucleu within PNCDI III PN-III-P11.2-PCCDI-2017-0839/19PCCDI/2018, Slovenian Research Agency - Slovenia P1-0031 P1-0385 I0-0033 N1-0111, Spain - Ministerio de Economía, Industria y Competitividad FPA2017-85114-P FPA2017-85197-P, Spain - Xunta de Galicia ED431C 2017/07, Junta de Andalucía SOMM17/6104/UGR, Spain - Feder Funds, Spain - RENATARedNacional Tematica de Astroparticulas FPA2015-68783-REDT, Spain - Maria de MaeztuUnit of Excellence MDM-2016-0692, United States Department of Energy (DOE) DE-AC02-07CH11359 DE-FR02-04ER41300 DEFG02-99ER41107 DE-SC0011689, National Science Foundation (NSF) 0450696, U.S.A. - Grainger Foundation, U.S.A. - Marie Curie-IRSES/EPLANET, U.S.A. - European Particle Physics Latin American Network, U.S.A. - UNESCO

Published
2020
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30. Direct measurement of the muonic content of extensive air showers between $\mathbf { 2\times 10^{17}}$ and $\mathbf {2\times 10^{18}}~$eV at the Pierre Auger Observatory

Author

P. Tobiska, Bjarni Pont, H. J. Mathes, Stanislav Michal, S. Schröder, Italo Epicoco, A. Di Matteo, L. Lopes, B. Wundheiler, Jaime Alvarez-Muñiz, Alexandru Gherghel-Lascu, Lukáš Vaclavek, B. Keilhauer, Ioana Codrina Maris, S. J. Sciutto, J. Rodriguez Rojo, Fridtjof Feldbusch, Alessio Gorgi, D. Melo, G. C. Hill, Juan Miguel Carceller, Jorge F. Soriano, Ralph Engel, Enrique Zas, Orazio Zapparrata, J. Stasielak, L. Calcagni, Kai Daumiller, R. Sato, J. Ridky, Roberto Mussa, Fernando Contreras, Luis Villaseñor, J. Rautenberg, K.-H. Becker, Q. Luce, M. Pimenta, Carola Dobrigkeit, M. Muzio, Maximilian Stadelmaier, Darko Veberič, Maximilian Reininghaus, J. F. Valdés Galicia, I. De Mitri, P.R. Araújo Ferreira, Tobias Winchen, Marvin Gottowik, François Montanet, Alan Watson, M. A. Leigui de Oliveira, M. Perlin, Eric Mayotte, M. Gómez Berisso, Mihai Niculescu-Oglinzanu, J. Alvarez Castillo, Gaia Silli, A. Filipčič, Eleonora Guido, R. C. Shellard, Florian Lukas Briechle, F. Sarazin, T. Huege, Heino Falcke, D. Nitz, A. van Vliet, S. Petrera, L. Nellen, Denise Boncioli, Hernan Wahlberg, P. Abreu, Jeffrey Brack, Olaf Scholten, Mario Buscemi, Marc Weber, Humberto Ibarguen Salazar, R. M. de Almeida, D. Ravignani, J. Vicha, L. R. Wiencke, David Wittkowski, G. Salina, Danielle LaHurd, Olivier Deligny, Lorenzo Caccianiga, C. Morello, Jesús Peña-Rodríguez, E. M. Santos, Dusan Mandat, M. L. Díaz Castro, G. Farrar, R. Squartini, R. Lorek, Ugo Giaccari, Miguel Mostafa, J. Kleinfeller, Bruce R. Dawson, Francesca Zuccarello, B. Tome, P.O. Mazur, Rodrigo Pelayo, K. H. Kampert, Peter L. Biermann, Stijn Buitink, Valerio Verzi, Alfred Müller, A. Aab, Violet M. Harvey, D. Harari, C. M. Schäfer, Jose Chinellato, L. Bonneau Arbeletche, Paolo Privitera, Massimo Mastrodicasa, A. López Casado, Frank G. Schröder, Marcel Köpke, Max Malacari, M. Platino, Samo Stanič, R. Conceição, Miroslav Hrabovský, Julien Manshanden, Ioana Caracas, Kevin-Druis Merenda, A. Letessier-Selvon, Dariusz Gora, Andres Travaini, F. Guarino, John Matthews, Flavia Gesualdi, A. Haungs, J. Perez Armand, Matias Tueros, Alina Mihaela Badescu, Cristina Galea, B. L. Lago, Lorenzo Cazon, E. Varela, Peter Buchholz, J.D. Sanabria Gomez, A. Taboada, M. Prouza, P. Mantsch, G. Matthiae, Z. Szadkowski, A. Parra, R.J. Barreira Luz, Luis A. Nunez, Alan Coleman, Christian Sarmiento-Cano, Marco Aglietta, Marcus Niechciol, S. J. Saffi, G. Medina-Tanco, R. Halliday, P.F. Gómez Vitale, Alena Bakalova, Claudio Galelli, Thomas Hebbeker, Paula Gina Isar, S. Müller, Giovanni Marsella, D. Nosek, E. Santos, F. Riehn, A. Fuster, B. García, Sergio Dasso, Tristan Sudholz, S. Querchfeld, R. López, Karen S. Caballero-Mora, F. Pedreira, Marina Scornavacche, Martín Miguel Freire, Markus Roth, F. Salamida, A. Yushkov, J. Šupík, Carlo Ventura, Raul Sarmento, Jonathan Biteau, Felix Schlüter, Nicolás González, Fabian Gobbi, M. Schimp, G. P. Guedes, Martin Erdmann, Toshihiro Fujii, Ladislav Chytka, G. Cataldi, Antonio Bueno, A. Weindl, P. Ristori, J. de Jesús, B. C. Manning, V. Scherini, Jakub Juryšek, A. Streich, J. Debatin, D. Mockler, David Schmidt, A. Tapia, Gioacchino Alex Anastasi, M. Wirtz, P. Ruehl, Alexandra Saftoiu, A. Puyleart, Corinne Berat, M. Giller, Roger W Clay, G. Kukec Mezek, Steffen Hahn, Juan Carlos D'Olivo, T. Pierog, M. Trini, J. Hulsman, M. E. Bertaina, Esteban Roulet, Justin M. Albury, Francesco Fenu, Valerio Pirronello, H. Gemmeke, A. Menshikov, Denis Stanca, C. J. Todero Peixoto, Piera Luisa Ghia, Miroslav Pech, M. Pothast, Jeffrey A. Johnsen, M. Schimassek, C. Hojvat, Jan Ebr, Pavel Horvath, C. O. Escobar, A. Insolia, H. Wilczyński, Günter Sigl, M. Unger, M. Kleifges, D. Zavrtanik, A.D. Supanitsky, J. Pȩkala, B. Andrada, P. Stassi, A. Cancio, Sofia Andringa, Radomir Smida, A. Machado Payeras, Jacco Vink, V. de Souza, Gualberto Avila, P. Savina, H.O. Klages, M. I. Micheletti, M.P. Panetta, I. Allekotte, M. J. Roncoroni, A. A. Nucita, Ralf Ulrich, B. Vargas Cárdenas, T. Suomijärvi, J. Pallotta, John Farmer, Brian Fick, A. M. Botti, Maria-Teresa Dova, M. R. Hampel, Niraj Dhital, I. Valiño, L. Nožka, Jörg R. Hörandel, R.C. dos Anjos, M. Zavrtanik, Adriana Vásquez-Ramírez, M. Palatka, A. C. Fauth, Giovanni Consolati, Carla Bonifazi, Jose A. Bellido, Fabio Convenga, M. Urban, W. M. Namasaka, A. C. Rovero, Petr Schovanek, Alexandru Balaceanu, M. Suárez-Durán, Carla Aramo, Vincenzo Rizi, I.D. Vergara Quispe, Julien Souchard, D. Martello, M. Ziolkowski, O. Martínez Bravo, Silvia Mollerach, N. Fazzini, Jonas Glombitza, F. C. T. Barbato, J. Chudoba, Serguei Vorobiov, O. A. Taborda, Marcos Cerda, D. Lo Presti, S. J. De Jong, Jarryd A. Day, A.C. Cobos Cerutti, J. R. T. de Mello Neto, W. Rodrigues de Carvalho, Teresa Bister, G. Golup, Nataliia Borodai, K. Choi, Paul Sommers, A. Blanco, F. Sánchez, Antonio Condorelli, Christine Peters, A.L. Garcia Vegas, Luis A. Anchordoqui, Maria Rita Coluccia, Julian Kemp, Philipp Papenbreer, Petr Travnicek, Martina Bohacova, Trent D. Grubb, M. A. Muller, Hernán Asorey, Juan Manuel Figueira, Roberta Colalillo, Giovanni Mancarella, A. G. Mariazzi, Xavier Bertou, A. Zepeda, Juan Pablo Gongora, Pedro Assis, H. Martinez, G. Torralba Elipe, A. Etchegoyen, L. Valore, Alex Kääpä, Patricia María Hansen, Marco Giammarchi, V. Novotny, Octavian Sima, Rossella Caruso, A. Lucero, Fernando Catalani, G. De Mauro, Caterina Trimarelli, H. Schieler, Q. Dorosti, I. Lhenry-Yvon, Antonella Castellina, Vladimir Lenok, L. Perrone, Thomas Bretz, Corbin Covault, Lino Miramonti, D. de Oliveira Franco, Isabel Goos, D. Heck, M. del Río, M. Risse, Jonathan Blazek, Charles Timmermans, G. Parente, Fabrizia Canfora, L. Zehrer, J. de Oliveira, Alejandro Almela, Carla Bleve, Rodrigo Guedes Lang, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), and Pierre Auger

Subjects
Physics and Astronomy (miscellaneous), air, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, UHE [cosmic radiation], Cosmic ray, 01 natural sciences, Auger, detector: fluorescence, Nuclear physics, 5/3, 0103 physical sciences, muon: density, ddc:530, cosmic radiation: UHE, 010306 general physics, Engineering (miscellaneous), Physics, Pierre Auger Observatory, fluorescence [detector], detector [muon], Muon, showers: atmosphere, hybrid, 010308 nuclear & particles physics, muon: detector, Astrophysics::Instrumentation and Methods for Astrophysics, observatory, Air shower, density [muon], 13. Climate action, Content (measure theory), High Energy Physics::Experiment, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Muon detector, atmosphere [showers]
Abstract

The hybrid design of the Pierre Auger Observatory allows for the measurement of the properties of extensive air showers initiated by ultra-high energy cosmic rays with unprecedented precision. By using an array of prototype underground muon detectors, we have performed the first direct measurement, by the Auger Collaboration, of the muon content of air showers between $$2\times 10^{17}$$2×1017 and $$2\times 10^{18}$$2×1018 eV. We have studied the energy evolution of the attenuation-corrected muon density, and compared it to predictions from air shower simulations. The observed densities are found to be larger than those predicted by models. We quantify this discrepancy by combining the measurements from the muon detector with those from the Auger fluorescence detector at $$10^{{17.5}}\, {\mathrm{eV}} $$1017.5eV and $$10^{{18}}\, {\mathrm{eV}} $$1018eV. We find that, for the models to explain the data, an increase in the muon density of $$38\%$$38%$$\pm 4\% (12\%)$$±4%(12%)$$\pm {}^{21\%}_{18\%}$$±18%21% for EPOS-LHC, and of $$50\% (53\%)$$50%(53%)$$\pm 4\% (13\%)$$±4%(13%)$$\pm {}^{23\%}_{20\%}$$±20%23% for QGSJetII-04, is respectively needed.

Published
2020

31. Study of the variable broadband emission of Markarian 501 during the most extreme Swift X-ray activity

Author

Francesco Longo, Yuki Iwamura, Susumu Inoue, L. Nogués, M. I. Martínez, G. Pedaletti, Thomas Bretz, J. Buss, A. Rugliancich, Marina Manganaro, D. Galindo, Merja Tornikoski, Sabrina Einecke, Martin Makariev, Oscar Blanch, C. Leto, Ciro Bigongiari, Adrian Biland, D. Zarić, Andrii Neronov, M. Garczarczyk, Sargis Gasparyan, Konstancja Satalecka, Michele Doro, Marc Ribó, M. Noethe, J. Becerra González, Kazuma Ishio, J. Rico, Christian Fruck, Kyoshi Nishijima, Abelardo Moralejo, E. Moretti, Wolfgang Rhode, Christoph Wendel, Dominik Baack, Satoshi Masuda, Hidetoshi Kubo, Nikola Godinovic, B. Machado de Oliveira Fraga, Alexander Hahn, Manuel Delfino, Daniela Dorner, P. Giammaria, A. Niedzwiecki, Alessio Berti, U. Barres de Almeida, F. Verrecchia, G. Busetto, Lena Linhoff, D. Fidalgo, Damir Lelas, G. Ferrara, Alicia Fattorini, D. Hildebrand, David Paneque, V. A. Acciari, Bernd Schleicher, Gaia Vanzo, M. Peresano, Rodolfo Carosi, M. Perri, Alessandra Lamastra, John Hoang, Marcel Strzys, M. Gaug, Chiara Righi, M. Armas Padilla, D. Ninci, Ana Babić, Michael Blank, Dorota Sobczyńska, D. Dominis Prester, A. De Angelis, Vitaly Neustroev, I. Snidaric, F. Schulz, E. von Willert, D. Guberman, A. Y. Lien, J. Herrera, Juan Abel Barrio, B. Banerjee, J. van Scherpenberg, V. D'Elia, Narek Sahakyan, P. Temnikov, Stefano Ansoldi, R. J. García López, G. Maneva, E. Do Souto Espiñera, B. De Lotto, Elisa Bernardini, Riccardo Paoletti, S. Paiano, Karl Mannheim, Pablo Peñil, A. Shukla, Ivica Puljak, Jose Luis Contreras, D. Neise, Andrea Tramacere, Manuela Mallamaci, A. López-Oramas, Jordi Delgado, V. Fallah Ramazani, Juan Cortina, J. Palacio, P. Colin, R. Walter, J. M. Paredes, F. Di Pierro, Antonio Stamerra, Pratik Majumdar, Camilla Maggio, M. V. Fonseca, Ievgen Vovk, Francesco Dazzi, A. Fernández-Barral, Cosimo Nigro, P. Munar-Adrover, Massimo Persic, Dario Hrupec, L. A. Antonelli, Martin Will, D. Kuveždić, T. Schweizer, F. Leone, Anne Lähteenmäki, Tarek M. Hassan, Fabrizio Tavecchio, Masahiro Teshima, A. Somero, Kari Nilsson, Ll. Font, M. Bulinski, Wlodek Bednarek, Vitalii Sliusar, P. G. Prada Moroni, Junko Kushida, P. Da Vela, E. Prandini, N. Torres-Albà, Joni Tammi, Sebastian Achim Mueller, J. R. Garcia, Giacomo Bonnoli, Manuel Doerr, Stefano Gallozzi, Jose Miguel Miranda, Wrijupan Bhattacharyya, Julian Sitarek, T. Surić, Shimpei Tsujimoto, K. Bruegge, D. Elsaesser, Tomislav Terzić, Jürgen Besenrieder, E. Molina, E. Colombo, Lab Saha, Luca Foffano, Mosè Mariotti, A. Paravac, Saverio Lombardi, M. Nievas Rosillo, M. Minev, M. Balbo, D. Hadasch, R. Mirzoyan, A. Arbet-Engels, K. Sedlaczek, L. Maraschi, Elina Lindfors, Daniel Mazin, Stefan Cikota, M. Vazquez Acosta, Victoria Moreno, Stefano Covino, Tomoki Saito, Giovanni Ceribella, Aaron Dominguez, K. Noda, Sidika Merve Colak, M. López, German Research Foundation, Istituto Nazionale di Fisica Nucleare, Istituto Nazionale di Astrofisica, Swiss National Science Foundation, Japan Society for the Promotion of Science, Ministry of Education, Culture, Sports, Science and Technology (Japan), Croatian Science Foundation, University of Rijeka, Polish National Agency for Academic Exchange, Ministério da Ciência, Tecnologia e Inovação (Brasil), National Aeronautics and Space Administration (US), Department of Energy (US), Commissariat à l'Ènergie Atomique et aux Ènergies Alternatives (France), Centre National de la Recherche Scientifique (France), Institut National de Physique Nucléaire et de Physique des Particules (France), Agenzia Spaziale Italiana, High Energy Accelerator Research Organization (Japan), Japan Aerospace Exploration Agency, Knut and Alice Wallenberg Foundation, Swedish Research Council, Swedish National Space Board, Acciari, V. A., Ansoldi, S., Antonelli, L. A., Babic, A., Banerjee, B., Barres De Almeida, U., Barrio, J. A., Becerra Gonzalez, J., Bednarek, W., Bernardini, E., Berti, A., Besenrieder, J., Bhattacharyya, W., Bigongiari, C., Blanch, O., Bonnoli, G., Busetto, G., Carosi, R., Ceribella, G., Cikota, S., Colak, S. M., Colin, P., Colombo, E., Contreras, J. L., Cortina, J., Covino, S., D'Elia, V., Da Vela, P., Dazzi, F., De Angelis, A., De Lotto, B., Delfino, M., Delgado, J., DI Pierro, F., Do Souto Espinera, E., Dominguez, A., Dominis Prester, D., Doro, M., Fallah Ramazani, V., Fattorini, A., Fernandez-Barral, A., Ferrara, G., Fidalgo, D., Foffano, L., Fonseca, M. V., Font, L., Fruck, C., Galindo, D., Gallozzi, S., Garcia Lopez, R. J., Garczarczyk, M., Gasparyan, S., Gaug, M., Giammaria, P., Godinovic, N., Guberman, D., Hadasch, D., Hahn, A., Hassan, T., Herrera, J., Hoang, J., Hrupec, D., Inoue, S., Ishio, K., Iwamura, Y., Kubo, H., Kushida, J., Kuvecdic, D., Lamastra, A., Lelas, D., Leone, F., Lindfors, E., Lombardi, S., Longo, F., Lopez, M., Lopez-Oramas, A., MacHado De Oliveira Fraga, B., Maggio, C., Majumdar, P., Makariev, M., Mallamaci, M., Maneva, G., Manganaro, M., Maraschi, L., Mariotti, M., Martinez, M., Masuda, S., Mazin, D., Minev, M., Miranda, J. M., Mirzoyan, R., Molina, E., Moralejo, A., Moreno, V., Moretti, E., Munar-Adrover, P., Neustroev, V., Niedzwiecki, A., Nievas Rosillo, M., Nigro, C., Nilsson, K., Ninci, D., Nishijima, K., Noda, K., Nogues, L., Paiano, S., Palacio, J., Paneque, D., Paoletti, R., Paredes, J. M., Pedaletti, G., Penil, P., Peresano, M., Persic, M., Prada Moroni, P. G., Prandini, E., Puljak, I., Garcia, J. R., Ribo, M., Rico, J., Righi, C., Rugliancich, A., Saha, L., Sahakyan, N., Saito, T., Satalecka, K., Schweizer, T., Sitarek, J., Snidaric, I., Sobczynska, D., Somero, A., Stamerra, A., Strzys, M., Suric, T., Tavecchio, F., Temnikov, P., Terzic, T., Teshima, M., Torres-Alba, N., Tsujimoto, S., Van Scherpenberg, J., Vanzo, G., Vazquez Acosta, M., Vovk, I., Will, M., Zaric, D., Arbet-Engels, A., Baack, D., Balbo, M., Biland, A., Blank, M., Bretz, T., Bruegge, K., Bulinski, M., Buss, J., Doerr, M., Dorner, D., Einecke, S., Elsaesser, D., Hildebrand, D., Linhoff, L., Mannheim, K., Mueller, S., Neise, D., Neronov, A., Noethe, M., Paravac, A., Rhode, W., Schleicher, B., Schulz, F., Sedlaczek, K., Shukla, A., Sliusar, V., Von Willert, E., Walter, R., Wendel, C., Tramacere, A., Lien, A., Perri, M., Verrecchia, F., Armas Padilla, M., Leto, C., Lahteenmaki, A., Tornikoski, M., Tammi, J., Department of Electronics and Nanoengineering, Metsähovi Radio Observatory, Aalto-yliopisto, and Aalto University

Subjects
galaxies: active, BL Lacertae objects: individual: Mrk 501, gamma rays: galaxies, X-rays: galaxies, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Flux, Context (language use), Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, 01 natural sciences, Power law, Spectral line, Galaxies: active, Gamma rays: galaxies, individual: Mrk 501 [BL Lacertae objects], 0103 physical sciences, MAGIC (telescope), Blazar, 010303 astronomy & astrophysics, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, galaxie [Gamma rays], 010308 nuclear & particles physics, Gamma ray, Astronomy and Astrophysics, galaxies [X-rays], Crab Nebula, Space and Planetary Science, active [galaxies], galaxies [gamma rays], ddc:520, Física nuclear, High Energy Astrophysical Phenomena, Astrophysics - High Energy Astrophysical Phenomena
Abstract

[Context] Markarian 501 (Mrk 501) is a very high-energy (VHE) gamma-ray blazar located at z = 0:034, which is regularly monitored by a wide range of multi-wavelength instruments, from radio to VHE gamma rays. During a period of almost two weeks in July 2014, the highest X-ray activity of Mrk 501 was observed in -14 years of operation of the Neil Gehrels Swift Gamma-ray Burst Observatory., [Aims] We characterize the broadband variability of Mrk 501 from radio to VHE gamma rays during the most extreme X-ray activity measured in the last 14 years, and evaluate whether it can be interpreted within theoretical scenarios widely used to explain the broadband emission from blazars., [Methods] The emission of Mrk 501 was measured at radio with Metsähovi, at optical–UV with KVA and Swift/UVOT, at X-ray with Swift/XRT and Swift/BAT, at gamma ray with Fermi-LAT, and at VHE gamma rays with the FACT and MAGIC telescopes. The multi-band variability and correlations were quantified, and the broadband spectral energy distributions (SEDs) were compared with predictions from theoretical models., [Results] The VHE emission of Mrk 501 was found to be elevated during the X-ray outburst, with a gamma-ray flux above 0.15 TeV varying from ∼0.5 to ∼2 times the Crab nebula flux. The X-ray and VHE emission both varied on timescales of 1 day and were found to be correlated. We measured a general increase in the fractional variability with energy, with the VHE variability being twice as large as the X-ray variability. The temporal evolution of the most prominent and variable segments of the SED, characterized on a day-by-day basis from 2014 July 16 to 2014 July 31, is described with a one-zone synchrotron self-Compton model with variations in the break energy of the electron energy distribution (EED), and with some adjustments in the magnetic field strength and spectral shape of the EED. These results suggest that the main flux variations during this extreme X-ray outburst are produced by the acceleration and the cooling of the high-energy electrons. A narrow feature at ∼3 TeV was observed in the VHE spectrum measured on 2014 July 19 (MJD 56857.98), which is the day with the highest X-ray flux (>0.3 keV) measured during the entire Swift mission. This feature is inconsistent with the classical analytic functions to describe the measured VHE spectra (power law, log-parabola, and log-parabola with exponential cutoff) at more than 3σ. A fit with a log-parabola plus a narrow component is preferred over the fit with a single log-parabola at more than 4σ, and a dedicated Monte Carlo simulation estimated the significance of this extra component to be larger than 3σ. Under the assumption that this VHE spectral feature is real, we show that it can be reproduced with three distinct theoretical scenarios: (a) a pileup in the EED due to stochastic acceleration; (b) a structured jet with two-SSC emitting regions, with one region dominated by an extremely narrow EED; and (c) an emission from an IC pair cascade induced by electrons accelerated in a magnetospheric vacuum gap, in addition to the SSC emission from a more conventional region along the jet of Mrk 501., The financial support of the German BMBF and MPG, the Italian INFN and INAF, the Swiss National Fund SNF, the ERDF under the Spanish MINECO (FPA2015-69818-P, FPA2012-36668, FPA2015-68378-P, FPA2015-69210-C6-2-R, FPA2015-69210-C6-4-R, FPA2015-69210-C6-6-R, AYA2015-71042-P, AYA2016-76012-C3-1-P, ESP2015-71662-C2-2-P, FPA2017-90566-REDC), and the Japanese JSPS and MEXT is gratefully acknowledged. This work was also supported by the Spanish Centro de Excelencia “Severo Ochoa” SEV-2016-0588 and SEV-2015-0548, and Unidad de Excelencia “María de Maeztu” MDM-2014-0369, by the Croatian Science Foundation (HrZZ) Project IP-2016-06-9782 and the University of Rijeka Project 13.12.1.3.02, by the DFG Collaborative Research Centers SFB823/C4 and SFB876/C3, the Polish National Research Centre grant UMO-2016/22/M/ST9/00382 and by the Brazilian MCTIC, CNPq and FAPERJ. The Fermi-LAT Collaboration acknowledges generous ongoing support from a number of agencies and institutes that have supported both the development and the operation of the LAT as well as scientific data analysis. These include the National Aeronautics and Space Administration and the Department of Energy in the United States, the Commissariat à l’Energie Atomique and the Centre National de la Recherche Scientifique/Institut National de Physique Nucléaire et de Physique des Particules in France, the Agenzia Spaziale Italiana and the Istituto Nazionale di Fisica Nucleare in Italy, the Ministry of Education, Culture, Sports, Science and Technology (MEXT), High Energy Accelerator Research Organization (KEK) and Japan Aerospace Exploration Agency (JAXA) in Japan, and the K. A. Wallenberg Foundation, the Swedish Research Council and the Swedish National Space Board in Sweden. Additional support for science analysis during the operations phase is gratefully acknowledged from the Instituto Nazionale di Astrofisica in Italy and the Centre National d’Études Spatiales in France. The important contributions from ETH Zurich grants ETH-10.08-2 and ETH-27.12-1 as well as the funding by the Swiss SNF and the German BMBF (Ver-bundforschung Astro-und Astroteilchenphysik) and HAP (Helmoltz Alliance for Astroparticle Physics) are gratefully acknowledged. Part of this work is supported by Deutsche Forschungsgemeinschaft (DFG) within the Collaborative Research Center SFB 876, project C3. We thank the Instituto de Astrofisica de Canarias for allowing us to operate the telescope at the Observatorio del Roque de los Muchachos in La Palma, the Max-Planck-Institut fur Physik for providing us with the mount of the former HEGRA CT3 telescope, and the MAGIC Collaboration for their support. JBG acknowledges the support of the Viera y Clavijo program funded by ACIISI and ULL. C. W. is grateful for the support by the project “Promotion inklusive” of the Universität zu Köln and the German Bundesmin-isterium für Arbeit und Soziales. This publication makes use of data obtained at Metsähovi Radio Observatory, operated by Aalto University, Finland.

Published
2020

32. Long-term multi-band photometric monitoring of Mrk 501

Author

Bernd Schleicher, Adrian Biland, Dorothee Hildebrand, Dominik Elsaesser, Jens Buss, Daniela Dorner, Laura Eisenberger, Alison Mitchell, Adelina Kalenski, Axel Arbet-Engels, Karl Mannheim, Matteo Balbo, Aleksander Paravac, Dominik Baack, Roland Walter, Roman Iotov, Maximilian Noethe, Dominik Neise, Thomas Bretz, Wolfgang Rhode, and Vitalii Sliusar

Subjects
Photon, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, 01 natural sciences, law.invention, Telescope, law, 0103 physical sciences, Blazar, 010303 astronomy & astrophysics, Cherenkov radiation, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, 010308 nuclear & particles physics, Computer Science::Information Retrieval, Compton scattering, Astronomy and Astrophysics, Light curve, Astrophysics - Astrophysics of Galaxies, Synchrotron, 3. Good health, 13. Climate action, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Precession, High Energy Physics::Experiment, Astrophysics - High Energy Astrophysical Phenomena
Abstract

Radio-to-TeV observations of the bright nearby (z=0.034) blazar Markarian 501 (Mrk 501), performed from December 2012 to April 2018, are used to study the emission mechanisms in its relativistic jet. We examined the multi-wavelength variability and the correlations of the light curves obtained by eight different instruments, including the First G-APD Cherenkov Telescope (FACT), observing Mrk 501 in very high-energy (VHE) gamma-rays at TeV energies. We identified individual TeV and X-ray flares and found a sub-day lag between variability in these two bands. Simultaneous TeV and X-ray variations with almost zero lag are consistent with synchrotron self-Compton (SSC) emission, where TeV photons are produced through inverse Compton scattering. The characteristic time interval of 5-25 days between TeV flares is consistent with them being driven by Lense-Thirring precession., 10 pages, 11 figures, Astronomy and astrophysics pre-print. arXiv admin note: text overlap with arXiv:2101.10651

Published
2021

33. Mirror position determination for the alignment of Cherenkov Telescopes

Author

Dominik Baack, Michael Blank, Sabrina Einecke, Sebastian Achim Mueller, Karl Mannheim, A. Dmytriiev, Daniela Dorner, Adrian Biland, Gareth Hughes, Matthias Bergmann, Lena Linhoff, R. Walter, Aleksander Paravac, D. Hildebrand, Julia Thaele, Felicitas Pauss, K. Bruegge, Jens Buss, Thomas Bretz, Wolfgang Rhode, Maximilian Noethe, Fabian Temme, Andrii Neronov, Dominik Neise, Christina Hempfling, M. Domke, J. Adam, Max Ludwig Ahnen, A. Shukla, and Matteo Balbo

Subjects
Point spread function, Nuclear and High Energy Physics, Facet (geometry), Mirror image, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Curved mirror, IACT, 01 natural sciences, law.invention, Telescope, Optics, law, 0103 physical sciences, Image sensor, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, Instrumentation, Cherenkov radiation, Physics, 010308 nuclear & particles physics, business.industry, Astrophysics::Instrumentation and Methods for Astrophysics, Computer Science::Computer Vision and Pattern Recognition, Astrophysics - Instrumentation and Methods for Astrophysics, business
Abstract

Imaging Atmospheric Cherenkov Telescopes (IACTs) need imaging optics with large apertures to map the faint Cherenkov light emitted in extensive air showers onto their image sensors. Segmented reflectors fulfill these needs using mass produced and light weight mirror facets. However, as the overall image is the sum of the individual mirror facet images, alignment is important. Here we present a method to determine the mirror facet positions on a segmented reflector in a very direct way. Our method reconstructs the mirror facet positions from photographs and a laser distance meter measurement which goes from the center of the image sensor plane to the center of each mirror facet. We use our method to both align the mirror facet positions and to feed the measured positions into our IACT simulation. We demonstrate our implementation on the 4 m First Geiger-mode Avalanche Cherenkov Telescope (FACT)., 11 figures, small ray tracing performance simulation, and implementation demonstration

Published
2017

34. Atmospheric Cherenkov Telescopes as a Potential Veto Array for Neutrino Astronomy

Author

Thomas Bretz, D. Rysewyk, J. Auffenberg, Tyce DeYoung, M. U. Nisa, Christopher Wiebusch, Merlin Schaufel, and Dirk Lennarz

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), Physics, 010308 nuclear & particles physics, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Detector, High Energy Physics::Phenomenology, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Astronomy, Astronomy and Astrophysics, 01 natural sciences, IceCube Neutrino Observatory, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), Air shower, 0103 physical sciences, High Energy Physics::Experiment, Neutrino astronomy, Neutrino, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, Cherenkov radiation
Abstract

The IceCube Neutrino Observatory has revealed the existence of sources of high-energy astrophysical neutrinos. However, identification of the sources is challenging because astrophysical neutrinos are difficult to separate from the background of atmospheric neutrinos produced in cosmic-ray-induced particle cascades in the atmosphere. The efficient detection of air showers in coincidence with detected neutrinos can greatly reduce those backgrounds and increase the sensitivity of neutrino telescopes. Imaging Air Cherenkov Telescopes (IACTs) are sensitive to gamma-ray-induced (and cosmic-ray-induced) air showers in the 50 GeV to 50 TeV range, and can therefore be used as background-identifiers for neutrino observatories. This paper describes the feasibility of an array of small scale, wide field-of-view, cost-effective IACTs as an air shower veto for neutrino astronomy. A surface array of 250 to 750 telescopes would significantly improve the performance of a cubic kilometer-scale detector like IceCube, at a cost of a few percent of the original investment. The number of telescopes in the array can be optimized based on astronomical and geometrical considerations., 33 pages, 10 figures. Published by Astropart. Phys

Published
2019

35. HAWC’s Eye - Implementing hybrid detection at the HAWC Gamma-Ray Observatory

Author

Jesús Martínez-Castro, Ruben Alfaro, Thomas Bretz, Jan Audehm, Y. Perez, Ibrahim Torres, José Miguel Serna, Maria Magdalena González, Merlin Schaufel, and Arturo Iriarte

Subjects
Physics, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, media_common.quotation_subject, Astrophysics::Instrumentation and Methods for Astrophysics, Gamma ray, Fresnel lens, law.invention, Telescope, Silicon photomultiplier, Sky, Observatory, law, Angular resolution, Cherenkov radiation, media_common, Remote sensing
Abstract

Combining a compact imaging air-Cherenkov telescope with the High-Altitude Water Cherenkov Gamma-Ray Observatory (HAWC) promises significant improvements in energy resolution, angular resolution and background suppression. The HAWC Observatory is an extensive air-shower array located in the state of Puebla, Mexico, sensitive at TeV energies continuously monitors two steradians of the sky. An improved sensitivity has the power to significantly increase the number of monitored sources. Triangulation by a compact air-Cherenkov telescope in a hybrid setup overcomes ambiguities on the height of the shower core if measured only with a ground array. A Cherenkov telescope prototype featuring a 50 cm Fresnel lens and a camera with 61 semi-conductor photosensors (SiPM) was commissioned and temporarily installed at the HAWC site in summer 2017. For the first time, hybrid events were recorded and the energy threshold and other basic properties of the telescope were measured and compared with simulations. Results of this campaign will be presented.

Published
2019

36. Air Shower Measurement with a SiPM Based Scintillator Detector

Author

Julian Kemp, Thomas Hebbeker, Thomas Bretz, Johannes Schumacher, Lukas Middendorf, and Christine Peters

Subjects
Pierre Auger Observatory, Physics, Photomultiplier, Optics, Silicon photomultiplier, Air shower, Physics::Instrumentation and Detectors, business.industry, Dynamic range, Detector, Biasing, Scintillator, business
Abstract

We developed an optical module based on silicon photomultipliers (SiPMs) designed for a wide variety of applications especially in scintillator detectors and laboratory measurements. To test the module, a Scintillator Surface Detector developed for AugerPrime, the upgrade of the Pierre Auger Observatory, was modified and is operating in the Argentinean Pampas. It is the first SiPM based scintillator detector successfully measuring air showers induced by ultra-high energy cosmic rays. The main goal of the development was exploiting the advantages of SiPMs compared to conventional photomultiplier tubes, specifically their mechanical and optical robustness, their high photon detection efficiency and their lower operating voltage. Two SiPMs are read out in parallel and equipped with light guides to increase the sensitive area. Their signal is split into three independent gain stages to exploit the full dynamic range from a breakdown of a single SiPM cell to a simultaneous breakdown of all cells. The bias voltage supply, which corrects for the temperature, is integrated into the module, and it is powered and controlled through a USB connection. This setup guarantees an easy usage of the module in many applications. We present the module and will show results from the field measurements.

Published
2019

37. FACT - Probing the Periodicity of Mrk 421 and Mrk 501

Author

Matteo Balbo, Dominik Elsaesser, Daniela Dorner, Axel Arbet-Engels, M. Bulinski, K. Sedlaczek, Adrian Biland, Amit Shukla, Aleksander Paravac, Roland Walter, Dorothee Hildebrand, Thomas Bretz, Andrii Neronov, Dominik Neise, Wolfgang Rhode, Elan von Willert, Sebastian Achim Mueller, Karl Mannheim, Vitalii Sliusar, Bernd Schleicher, Marc Klinger, Fabian Theissen, Laurits Tani, Michael Blank, Manuel Doerr, K. Bruegge, Marvin Beck, Dominik Baack, Roman Iotov, Maximilian Noethe, and Jens Buss

Subjects
Physics, Active galactic nucleus, Astrophysics::High Energy Astrophysical Phenomena, Gamma ray, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Light curve, Accretion (astrophysics), law.invention, Telescope, Crab Nebula, law, Blazar, Astrophysics::Galaxy Astrophysics, Fermi Gamma-ray Space Telescope
Abstract

Markarian 421 and Markarian 501 are Active Galactic Nuclei and two of the most prominent sources of very high energetic gamma rays. In contrast to the predominantly stable Crab Nebula, the two blazars have extremely variable gamma-ray fluxes. Those could be caused by erratic accretion flow instabilities, but also by processes leading to quasi periodic oscillations (QPOs). Recently, hints of such a QPO of Mrk 501 with a period of about 322 days have been observed with the Large Area Telescope on-board of the Fermi satellite at GeV energies featuring global and local significances of the signal above 99%. The First G-APD Cherenkov Telescope (FACT) has monitored a small sample of known TeV gamma-ray sources including Mrk 421 and Mrk 501 over the last seven years. Therefore, it is ideally suited for periodicity studies of Active Galactic Nuclei, as they require unbiased and continuous long-term observations. Based on measurements of the well-known gamma-ray flux originating from the Crab Nebula, corrections to the measured light curves are applied. In total, 2500~hours of data for each of the two blazars have been analysed using the Lomb-Scargle algorithm. The resulting periodogram of Mrk 501 shows a hint of QPO with a similar period as the one observed by Fermi/LAT., PoS: Proceedings of Science, 358, ISSN:1824-8039, Proceedings of 36th International Cosmic Ray Conference (ICRC 2019)

Published
2019

38. Fluorescence light detection with the FAMOUS telescope

Author

Thomas Hebbeker, Christine Peters, Tobias Pan, Paulo Ricardo Araújo Ferreira, Thomas Bretz, Julian Kemp, Adrianna Luz García Vegas, Johannes Schumacher, and Merlin Schaufel

Subjects
Physics, Pierre Auger Observatory, Photomultiplier, Photon, Physics::Instrumentation and Detectors, business.industry, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, law.invention, Telescope, Silicon photomultiplier, Optics, law, Ultra-high-energy cosmic ray, business, Cherenkov radiation
Abstract

The First Auger Multi-pixel photon counter camera for the Observation of Ultra-high-energy air-Showers (FAMOUS) is a telescope developed at the RWTH Aachen University in Germany. Its main goal is to measure photons produced in extensive air showers generated from the interaction of ultra high energy cosmic rays with the Earth's atmosphere. FAMOUS uses Silicon Photomultipliers as photodetection device instead of Photomultiplier tubes used by the fluorescence telescope in the Pierre Auger Observatory. The data acquisition system currently used by FAMOUS is suitable to measure Cherenkov photons. Now we evaluate its capability to detect also fluorescence light which will give information about the energy and the arrival direction of the primary cosmic rays.

Published
2019

39. The Aachen Muon Detector for testing the local production of Scintillating Surface Detectors for AugerPrime

Author

Thomas Hebbeker, A. Garcia, Paulo Ricardo Araújo Ferreira, Julian Kemp, Jorn Schumacher, Thomas Bretz, and Christine Peters

Subjects
Physics, Pierre Auger Observatory, Physics::Instrumentation and Detectors, business.industry, Detector, Scintillator, Chip, Data acquisition, Silicon photomultiplier, Optics, Calibration, High Energy Physics::Experiment, business, Image resolution
Abstract

The prototype of the Aachen Muon Detector was designed as an alternative for the upcoming upgrade (AugerPrime) of Scintillating Surface Detectors (SSD) for the Pierre Auger Observatory. Due to the successful application of semi-conductor photo sensors (SiPM), two portable detectors with a slightly modified design were built. They are currently applied for testing the local production of SSD detectors. Each of the two detectors consists of eight 30 x 30 x 0.5 cm$^3$ scintillator tiles. The light of each tile is collected by a dedicated wavelength-shifting fiber embedded into the tile and coupled directly to a 1.3 x 1.3 mm$^2$ SiPM. Reading out each channel individually with an EASIROC data acquisition chip provides spatial resolution, muon counting and an amplitude measurement for bright events. The obtained spectrum of minimum ionizing particles is nicely modulated with the single-photon equivalent (p.e.) resolution of the SiPM allowing for a very precise calibration of the system. The use of SiPM provides a very robust solution for a lightweight and portable detector easily applicable to a wide variety of setups.

Published
2019

40. Zenith angle dependence of the cosmic ray rate as measured with Imaging air-Cherenkov Telescopes

Author

Thomas Bretz

Subjects
Physics, 010308 nuclear & particles physics, Aperture, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Astronomy and Astrophysics, Cosmic ray, 01 natural sciences, Computational physics, law.invention, Core (optical fiber), Telescope, Cardinal point, law, 0103 physical sciences, Astrophysics - Instrumentation and Methods for Astrophysics, 010303 astronomy & astrophysics, Image resolution, Instrumentation and Methods for Astrophysics (astro-ph.IM), Zenith, Cherenkov radiation
Abstract

The rate of extensive air-showers observed with imaging air-Cherenkov telescopes is zenith angle dependent. This effect originates from the increasing geometrical distance of the observed shower to the telescope with increasing zenith distance. This paper investigates how this alters the observed image and how this affects the trigger rate as a function of zenith angle. The discussed effects include the change of Cherenkov light yield, of absorption in the atmosphere, of photon density at the aperture and of the image size at the focal plane of the telescope. Based on a simple model for the atmosphere and well-known first principles on the development of extensive air-showers, the zenith angle dependence is expressed analytically. The assumption that most light is emitted from the shower core and mathematical approximations allow to derive an analytical expression describing the zenith angle dependence well with only three free parameters which are directly linked with the underlying physics. This suggests further investigations about how these fit parameters are linked to the properties of the atmosphere and the instrument. Using data published by the First G-APD Cherenkov Telescope, a good match of the fit functions with the data is obtained. For the trigger rate of cosmic rays, the obtained parameters are consistent with the naive expectation., Comment: accepted

Published
2019
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41. AMS-100: The Next Generation Magnetic Spectrometer in Space -- An International Science Platform for Physics and Astrophysics at Lagrange Point 2

Author

Michael Wlochal, M. Czupalla, Philipp Mertsch, Henning Gast, L. Spies, S. Schael, P. von Doetinchem, Bernd Dachwald, C. Maña, P. S. Marrocchesi, J. Berdugo, A. Schultz von Dratzig, Waclaw Karpinski, J. Zimmermann, Davide Uglietti, Kai-Uwe Schröder, T. Kirn, Michael Schluse, Igor V. Moskalenko, Carmine Senatore, A. Atanasyan, Thomas Bretz, M. Duranti, S. P. Wakely, Thomas Andreas Schervan, and K. Lübelsmeyer

Subjects
FLUX, Antimatter, Nuclear and High Energy Physics, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Dark matter, Lagrangian point, FOS: Physical sciences, Cosmic-ray knee, Cosmic ray, ddc:500.2, Radiation, Cosmic rays, High-energy, gamma-rays, Multi-messenger astrophysics, DARK-MATTER, GAMMA-RAYS, PAMELA, ANTIPROTONS, PARTICLES, PROTONS, TRACKER, 01 natural sciences, Article, Optics, Rigidity (electromagnetism), 0103 physical sciences, 010306 general physics, 010303 astronomy & astrophysics, Instrumentation, Instrumentation and Methods for Astrophysics (astro-ph.IM), Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Spectrometer, business.industry, high-energy gamma-rays, Magnet, business, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract

The next generation magnetic spectrometer in space, AMS-100, is designed to have a geometrical acceptance of $100\,\mathrm{m}^2\,\mathrm{sr}$ and to be operated for at least ten years at the Sun-Earth Lagrange Point 2. Compared to existing experiments, it will improve the sensitivity for the observation of new phenomena in cosmic rays, and in particular in cosmic antimatter, by at least a factor of 1000. The magnet design is based on high temperature superconductor tapes, which allow the construction of a thin solenoid with a homogeneous magnetic field of 1 Tesla inside. The inner volume is instrumented with a silicon tracker reaching a maximum detectable rigidity of 100 TV and a calorimeter system that is 70 radiation lengths deep, equivalent to four nuclear interaction lengths, which extends the energy reach for cosmic-ray nuclei up to the PeV scale, i.e. beyond the cosmic-ray knee. Covering most of the sky continuously, AMS-100 will detect high-energy gamma rays in the calorimeter system and by pair conversion in the thin solenoid, reconstructed with excellent angular resolution in the silicon tracker., Comment: 26 pages, 15 figures, to be submitted to Nuclear Instruments and Methods in Physics Research Section A. Corresponding author: Stefan Schael

Published
2019
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42. Fractional Variability: a Tool to Study Blazar Variability

Author

Sergej Grischagin, Dominik Elsaesser, F. Schulz, Dorothee Hildebrand, Adrian Biland, M. Bulinski, Vitalii Sliusar, Aleksander Paravac, Thomas Bretz, Matteo Balbo, Bernd Schleicher, Lena Linhoff, Axel Arbet-Engels, Andrii Neronov, Dominik Neise, Roland Walter, Wolfgang Rhode, Elan von Willert, Sebastian Achim Mueller, K. Bruegge, Michael Blank, Manuel Doerr, K. Sedlaczek, Daniela Dorner, Amit Shukla, Karl Mannheim, Dominik Baack, Maximilian Noethe, Jens Buss, Balbo, Matteo, Dorner, Daniela, Neronov, Andrii, Sliusar, Vitalii, and Walter, Roland

Subjects
Complete data, Active galactic nucleus, lcsh:Astronomy, Electromagnetic spectrum, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics, Radiation, Blazar, 01 natural sciences, lcsh:QB1-991, 0103 physical sciences, Range (statistics), ddc:530, Variability, 010303 astronomy & astrophysics, Physics, Active galactic nuclei, 010308 nuclear & particles physics, Astronomy and Astrophysics, Light curve, Aktiver galaktischer Kern, Fractional variability, Blazars, Variabilität, ddc:520
Abstract

Active Galactic Nuclei emit radiation over the whole electromagnetic spectrum up to TeV energies. Blazars are one subtype with their jets pointing towards the observer. One of their typical features is extreme variability on timescales, from minutes to years. The fractional variability is an often used parameter for investigating the degree of variability of a light curve. Different detection methods and sensitivities of the instruments result in differently binned data and light curves with gaps. As they can influence the physics interpretation of the broadband variability, the effects of these differences on the fractional variability need to be studied. In this paper, we study the systematic effects of completeness in time coverage and the sampling rate. Using public data from instruments monitoring blazars in various energy ranges, we study the variability of the bright TeV blazars Mrk 421 and Mrk 501 over the electromagnetic spectrum, taking into account the systematic effects, and compare our findings with previous results. Especially in the TeV range, the fractional variability is higher than in previous studies, which can be explained by the much longer (seven years compared to few weeks) and more complete data sample., Galaxies, 7 (2)

Published
2019

43. Science Case for a Wide Field-of-View Very-High-Energy Gamma-Ray Observatory in the Southern Hemisphere

Author

Harm Schoorlemmer, J. C. Arteaga-Velázquez, M. J. Martínez González, A. J. S. Smith, Mosè Mariotti, O. Tibolla, Sergio Dasso, Jose A. Bellido, M. Seglar-Arroyo, L. Nellen, P. Cristofari, F. Schüssler, R. Arceo, S. Coutiño de León, Arturo Iriarte, J. M. Alvarez, Marcos Santander, Chad Brisbois, Nissim Illich Fraija, Michael DuVernois, E. de Oña Wilhelmi, R. D. Parsons, Samridha Kunwar, A. Carosi, A. Pichel, Jose Andres Garcia-Gonzalez, A. Carramiñana, Samuel Timothy Spencer, E. Pueschel, H. Martínez-Huerta, E. Tabachnick, J. P. Harding, Thomas Weisgarber, Henrike Fleischhack, J. L. Rodriguez, C. Alvarez, E. Prandini, E. De la Fuente, S. Y. BenZvi, B. Vallage, T. K. Sako, R. López-Coto, K. Link, Hao Zhou, Ibrahim Torres, F.O. de Oliveira Salles, R. Alfaro, P. M. Chadwick, J. G. Gonzalez, S. Procureur, Aion Viana, Miguel Mostafa, A. Haungs, A. Sandoval, Julien Lefaucheur, A. Zepeda, P. Huentemeyer, A. C. Rovero, Edna Ruiz-Velasco, B. Patricelli, Sarah Kaufmann, R. Yang, Gavin Rowell, Kristi Engel, J-F. Glicenstein, D. Hoyos, Juan Carlos Diaz-Velez, V. de Souza, J. A. Goodman, Armelle Jardin-Blicq, T. Sako, J.-P. Lenain, Pooja Surajbali, A.M. Taylor, F. Werner, Konstancja Satalecka, Stefan Funk, Paolo Desiati, Jim Hinton, Quentin Piel, Halim Ashkar, R. Wischnewski, Daniela Dorner, Sabrina Casanova, V. Joshi, G. Di Sciascio, Thomas Bretz, Francois Brun, A. M. Brown, Karen S. Caballero-Mora, A. Nayerhoda, R. White, Jesús Martínez-Castro, H. A. Ayala Solares, Andrea Albert, Colas Rivière, Binita Hona, K. Kawata, Andreas Reisenegger, Jason John Watson, Brenda Dingus, V. Marandon, and Garret Cotter

Subjects
Physics, 010308 nuclear & particles physics, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, Gamma ray, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Particle accelerator, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, Cherenkov Telescope Array, 7. Clean energy, 01 natural sciences, Galaxy, law.invention, Air shower, 13. Climate action, law, Observatory, Sky, 0103 physical sciences, 010303 astronomy & astrophysics, media_common
Abstract

We outline the science motivation for SGSO, the Southern Gamma-Ray Survey Observatory. SGSO will be a next-generation wide field-of-view gamma-ray survey instrument, sensitive to gamma-rays in the energy range from 100 GeV to hundreds of TeV. Its science topics include unveiling galactic and extragalactic particle accelerators, monitoring the transient sky at very high energies, probing particle physics beyond the Standard Model, and the characterization of the cosmic ray flux. SGSO will consist of an air shower detector array, located in South America. Due to its location and large field of view, SGSO will be complementary to other current and planned gamma-ray observatories such as HAWC, LHAASO, and CTA.

Published
2019

44. An integrated general purpose SiPM based optical module with a high dynamic range

Author

Johannes Schumacher, Darko Veberič, Radomir Smida, Thomas Bretz, J. Kemp, Ralph Engel, T. Hebbeker, Lukas Middendorf, and Christine Peters

Subjects
Photomultiplier, Materials science, Physics - Instrumentation and Detectors, 010308 nuclear & particles physics, business.industry, Dynamic range, Physics, Detector, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), Scintillator, 01 natural sciences, Particle detector, Silicon photomultiplier, Upgrade, 0103 physical sciences, Scintillation counter, Optoelectronics, ddc:530, ddc:610, 010306 general physics, business, Instrumentation, Mathematical Physics
Abstract

Silicon photomultipliers (SiPMs) are semiconductor-based light-sensors offering a high gain, a mechanically and optically robust design and high photon detection efficiency. Due to these characteristics, they started to replace conventional photomultiplier tubes in many applications in recent years. This paper presents an optical module based on SiPMs designed for the application in scintillators as well as lab measurements. The module hosts the SiPM bias voltage supply and three pre-amplifiers with different gain levels to exploit the full dynamic range of the SiPMs. Two SiPMs, read-out in parallel, are equipped with light guides to increase the sensitive area. The light guides are optimized for the read-out of wavelength shifting fibers as used in many plastic scintillator detectors. The optical and electrical performance of the module is characterized in detail in laboratory measurements. Prototypes have been installed and tested in a modified version of the Scintillator Surface Detector developed for AugerPrime, the upgrade of the Pierre Auger Observatory. The SiPM module is operated in the Argentinian Pampas and first data proves its usability in such harsh environments., 32 pages, 28 figures, submitted to JINST

Published
2018

45. Single Photon Extraction for FACT’s SiPMs allows for Novel IACT Event Representation

Author

J. Oberkirch, Anton Dmytriiev, Adrian Biland, Dominik Baack, L. Kortmann, Felicitas Pauss, Michael Blank, K. Bruegge, Max Mahlke, Aleksander Paravac, Sabrina Einecke, Lena Linhoff, Daniela Dorner, Matteo Balbo, Roland Walter, Amit Shukla, Julia Thaele, Tina Herbst, Andrii Neronov, Karl Mannheim, Dominik Neise, Sebastian Achim Mueller, Bernd Schleicher, Fabian Temme, F. Schulz, Dorothee Hildebrand, Dominik Elsaesser, Jens Buss, Thomas Bretz, Maximilian Noethe, Wolfgang Rhode, Vitalii Sliusar, Christina Hempfling, J. Adam, and Max Ludwig Ahnen

Subjects
Physics, Photomultiplier, Photon, Pixel, business.industry, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, IACT, law.invention, Telescope, Optics, Silicon photomultiplier, Air shower, law, business, Cherenkov radiation
Abstract

Imaging Atmospheric Cherenkov Telescopes provide large gamma-ray collection areas > 10^4 m^2 and successfully probe the high energetic gamma-ray sky by observing extensive air showers during the night. The First G-APD Cherenkov Telescope (FACT) explores silicon based photoelectric converters (called G-APDs or SiPMs) which provide more observation time with strong moonlight, a more stable photon gain over years of observations, and mechanically simpler imaging cameras. So far, the signal extraction methods used for FACT originate from sensors with no intrinsic quantized responses like photomultiplier tubes. This standard signal extraction is successfully used for the long time monitoring of the gamma-ray flux of bright blazars. However, we now challenge our classic signal extraction and explore single photon extraction methods to take advantage of the highly stable and quantized single photon responses of FACT's SiPM sensors. Instead of having one main pulse with one arrival time and one photon equivalent extracted for each pixel, we extract the arrival times of all individual photons in a pixel’s time line which opens up a new dimension in time for representing extensive air showers with an IACT. In this contribution, we will introduce our novel IACT event representation which is a list of single photon arrival times for each pixel (Photon-Stream). We will discuss our single photon extractor, its performance and its limitations. We will present example events where we identify individual, single air shower Cherenkov photons in the pool of individual, single night sky background photons., PoS: Proceedings of Science, 301, ISSN:1824-8039, Proceedings of the 35th International Cosmic Ray Conference (ICRC 2017)

Published
2018
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46. Higher Order Temperature Dependence of SiPM used in FACT

Author

Thomas Bretz, Michael Blank, Matteo Balbo, Anton Dmytriiev, F. Schulz, J. Oberkirch, L. Kortmann, Adrian Biland, Lena Linhoff, Felicitas Pauss, Wolfgang Rhode, Andrii Neronov, Dominik Neise, Sabrina Einecke, Jens Buss, Dorothee Hildebrand, Karl Mannheim, Christina Hempfling, Daniela Dorner, Vitalii Sliusar, J. Adam, Dominik Elsaesser, Max Ludwig Ahnen, Tina Herbst, Aleksander Paravac, Maximilian Noethe, Fabian Temme, Amit Shukla, Dominik Baack, Julia Thaele, Sebastian Achim Mueller, Bernd Schleicher, Max Mahlke, and K. Bruegge

Subjects
Physics, business.industry, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Photodetector, Cosmic ray, IACT, law.invention, Telescope, Wavelength, Optics, Silicon photomultiplier, law, Calibration, business, Cherenkov radiation
Abstract

Solid state photosensors, usually called SiPM or G-APD, seem ideal devices to be used in Imaging Atmospheric Cherenkov Telescopes (IACT). Nevertheless, their temperature dependence poses questions about their suitability in the harsh environment intrinsic to the operation of IACTs. While detailed measurements in the laboratory are possible with some sample sensors, limited data about the performance and uniformity of large samples exist. The First G-APD Cherenkov Telescope (FACT) is pioneering the usage of SiPMs for IACTs. Its camera consists of 1440 SiPMs and it is operated since October 2011 each night when observation conditions permit. Using no temperature stabilization system for the sensors, their temperature is closely coupled to the outside temperature that can change by more than 20 ∘C. While the strong temperature dependence of the gain of the sensors was shown to be easily compensated by adapting the applied voltage, there could also be higher order temperature dependencies of parameters like optical cross-talk, after-pulsing and wavelength dependent photon-detection efficiency. While external calibration devices could be used, one would have to proof that these devices do not have their own temperature dependencies. Instead, we use the constant flux of high energetic cosmic ray particles as calibration device. Their measured flux can depend on variable absorption and scattering of Cherenkov light e.g. due to dust and clouds, as well as on seasonal variations of the atmosphere. Nevertheless, using data sets where the temperature drastically changed within short time periods, we show that temperature dependencies of FACT, including the SiPMs, are well under control., PoS: Proceedings of Science, 301, ISSN:1824-8039, Proceedings of the 35th International Cosmic Ray Conference (ICRC 2017)

Published
2018
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47. FACT – Performance of the First Cherenkov Telescope Observing with SiPMs

Author

F. Schulz, Anton Dmytriiev, Karl Mannheim, Thomas Bretz, J. Oberkirch, Wolfgang Rhode, Adrian Biland, Max Mahlke, Lena Linhoff, Dominik Elsaesser, Sabrina Einecke, Sebastian Achim Mueller, Aleksander Paravac, Dominik Baack, Christina Hempfling, J. Adam, Max Ludwig Ahnen, K. Bruegge, Tina Herbst, Roland Walter, Michael Blank, Matteo Balbo, Daniela Dorner, Andrii Neronov, Dominik Neise, Felicitas Pauss, Bernd Schleicher, Vitalii Sliusar, Amit Shukla, Julia Thaele, Jens Buss, Fabian Temme, L. Kortmann, Maximilian Noethe, and Dorothee Hildebrand

Subjects
Physics, Physics::Instrumentation and Detectors, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, Cosmic distance ladder, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Context (language use), First light, law.invention, Telescope, Crab Nebula, Sky, law, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Blazar, Cherenkov radiation, media_common
Abstract

The First G-APD Cherenkov Telescope (FACT) is pioneering the usage of silicon photo mul- tipliers (SiPMs also known as G-APDs) for the imaging atmospheric Cherenkov technique. It is located at the Observatorio Roque de los Muchachos on the Canary island of La Palma. Since first light in October 2011, it is monitoring bright TeV blazars in the northern sky. By now, FACT is the only imaging atmospheric Cherenkov telescope operating with S I PMs on a nightly basis. Over the course of the last five years, FACT has been demonstrating their reliability and excel- lent performance. Moreover, their robustness allowed for an increase of the duty cycle including nights with strong moon light without the need for UV-filters. In this contribution, we will present the performance of the first Cherenkov telescope using solid state photo sensors, which was determined in analysis of data from Crab Nebula, the so called standard candle in gamma-ray astronomy. The presented analysis chain utilizes modern data mining methods and unfolding techniques to obtain the energy spectrum of this source. The characteristical results of such an analysis will be reported providing, e. g., the angular and energy resolution of FACT, as well as, the energy spectrum of the Crab Nebula. Furthermore, these results are discussed in the context of the performance of coexisting Cherenkov telescopes., PoS: Proceedings of Science, 301, ISSN:1824-8039, Proceedings of the 35th International Cosmic Ray Conference (ICRC 2017)

Published
2018
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48. MAGIC detection of short-term variability of the high-peaked BL Lac object 1ES 0806+524

Author

A. De Angelis, A. Treves, Vitaly Neustroev, R. Zanin, Adrian Biland, J. Rico, G. Maneva, Dario Hrupec, Thomas Bretz, M. Palatiello, Dario Gasparrini, I. Lozano, M. A. Lopez, A. González Muñoz, Louis Antonelli, Walter Max-Moerbeck, Diego F. Torres, Jelena Aleksić, R. López-Coto, X. Paredes-Fortuny, A. Niedzwiecki, D. Nakajima, Julian Sitarek, Francesco Dazzi, A. Fernández-Barral, Patrick Vogler, P. Munar-Adrover, J. M. Paredes, J. Kushida, Jose Luis Contreras, Masahiro Teshima, Ivica Puljak, Filippo D'Ammando, Daniela Dorner, K. Mallot, Wolfgang Rhode, Pierre Colin, R. J. García López, Elina Lindfors, A. Sillanpää, Juan Abel Barrio, David Paneque, Juan Cortina, C. Fruck, M. Gaug, D. Fidalgo, T. Toyama, Antonio Stamerra, Daniel Mazin, Takashi Saito, J. Krause, W. Bednarek, J. Herrera, B. De Lotto, Fabrizio Tavecchio, Julia Thaele, S. N. Shore, K. Berger, Ll. Font, Koji Noda, Reiko Orito, Elisa Bernardini, J. Hose, I. Snidaric, J. L. Richards, D. Elsaesser, E. de Oña Wilhelmi, Francesco Longo, H. Takami, Abelardo Moralejo, K. Nishijima, F. Di Pierro, C. Delgado Mendez, D. Dominis Prester, T. Steinbring, Massimo Persic, Yusuke Konno, Juri Poutanen, E. Lorenz, M. Hayashida, Stefano Covino, G. De Caneva, M. V. Fonseca, Kari Nilsson, K. Kodani, Y. Hanabata, K. Saito, G. Bonnoli, Talvikki Hovatta, M. Will, Marc Ribó, D. Tescaro, P. Antoranz, Konstancja Satalecka, R. Reinthal, P. Temnikov, Michele Doro, M. L. Knoetig, S. Buson, Razmik Mirzoyan, Hidetoshi Kubo, P. G. Prada Moroni, D. Garrido Terrats, Damir Lelas, V. Scalzotto, Nikola Godinovic, Benito Marcote, Dorota Sobczyńska, Oscar Blanch, Ana Babić, P. Da Vela, Stefano Ansoldi, T. Schweizer, Riccardo Paoletti, E. Prandini, F. Borracci, Alessandro Carosi, D. Hadasch, Jose Miguel Miranda, C. Schultz, V. Scapin, Anthony C. S. Readhead, M. Strzys, L. Maraschi, B. Biasuzzi, Tomislav Terzić, D. Galindo, M. I. Martínez, P. Bangale, Sabrina Einecke, S. R. Gozzini, J. Rodriguez Garcia, M. Makariev, U. Menzel, W. Idec, E. Colombo, L. O. Takalo, Mosè Mariotti, A.-K. Overkemping, Saverio Lombardi, Hanna Kellermann, K. Frantzen, V. Kadenius, S. Bonnefoy, S. Paiano, Karl Mannheim, D. Eisenacher, E. Carmona, Markus Garczarczyk, Alicia López-Oramas, Natalia Lewandowska, A. La Barbera, M. Nievas Rosillo, J. Becerra González, Aalto-yliopisto, Aalto University, Aleksi , J., Ansoldi, Stefano, Antonelli, L. A., Antoranz, P., Babic, A., Bangale, P., Barrio, J. A., Becerra Gonzalez, J., Bednarek, W., Bernardini, E., Biasuzzi, B., Biland, A., Blanch, O., Bonnefoy, S., Bonnoli, G., Borracci, F., Bretz, T., Carmona, E., Carosi, A., Colin, P., Colombo, E., Contreras, J. L., Cortina, J., Covino, S., Da Vela, P., Dazzi, F., De Angelis, A., De Caneva, G., De Lotto, B., de Ona Wilhelmi, E., Delgado Mendez, C., Di Pierro, F., Dominis Prester, D., Dorner, D., Doro, M., Einecke, S., Eisenacher, D., Elsaesser, D., Fernandez Barral, A., Fidalgo, D., Fonseca, M. V., Font, L., Frantzen, K., Fruck, C., Galindo, D., Garcia Lopez, R. J., Garczarczyk, M., Garrido Terrats, D., Gaug, M., Godinovi , N., Gonzalez Munoz, A., Gozzini, S. R., Hadasch, D., Hanabata, Y., Hayashida, M., Herrera, J., Hose, J., Hrupec, D., Idec, W., Kadenius, V., Kellermann, H., Knoetig, M. L., Kodani, K., Konno, Y., Krause, J., Kubo, H., Kushida, J., La Barbera, A., Lelas, D., Lewandowska, N., Lindfors, E., Lombardi, S., Longo, Francesco, Lopez, M., Lopez Coto, R., Lopez Oramas, A., Lorenz, E., Lozano, I., Makariev, M., Mallot, K., Maneva, G., Mannheim, K., Maraschi, L., Marcote, B., Mariotti, M., Martinez, M., Mazin, D., Menzel, U., Miranda, J. M., Mirzoyan, R., Moralejo, A., Munar Adrover, P., Nakajima, D., Neustroev, V., Niedzwiecki, A., Nievas Rosillo, M., Nilsson, K., Nishijima, K., Noda, K., Orito, R., Overkemping, A., Paiano, S., Palatiello, M., Paneque, D., Paoletti, R., Paredes, J. M., Paredes Fortuny, X., Persic, M., Poutanen, J., Prada Moroni, P. G., Prandini, E., Puljak, I., Reinthal, R., Rhode, W., Ribo, M., Rico, J., Rodriguez Garcia, J., Saito, T., Saito, K., Satalecka, K., Scalzotto, V., Scapin, V., Schultz, C., Schweizer, T., Shore, S. N., Sillanpaa, A., Sitarek, J., Snidaric, I., Sobczynska, D., Stamerra, A., Steinbring, T., Strzys, M., Takalo, L., Takami, H., Tavecchio, F., Temnikov, P., Terzi , T., Tescaro, D., Teshima, M., Thaele, J., Torres, D. F., Toyama, T., Treves, A., Vogler, P., Will, M., Zanin, R., Berger, K., Buson, S., D'Ammando, F., Gasparrini, D., Hovatta, T., Max Moerbeck, W., Readhead, A., and Richards, J.

Subjects
radiation mechanisms: non-thermal, galaxies: active, BL Lacertae objects: individual: 1ES 0806+524, galaxies: jets, gamma rays: galaxies, Astrophysics::High Energy Astrophysical Phenomena, astro-ph.GA, galaxies: active, jets [galaxies], Flux, FOS: Physical sciences, radiation mechanisms: non-thermal, BL Lacertae objects: individual: 1ES 0806+524, galaxies: jets, gamma rays: galaxies, individual: 1ES 0806+524 [BL Lacertae objects], Astrophysics, law.invention, law, MAGIC (telescope), Blazar, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), astro-ph.HE, ta115, ta213, Compton scattering, Astronomy, Astronomy and Astrophysics, non-thermal [radiation mechanisms], non-thermal, galaxies: active, BL Lacertae objects: individual: 1ES 0806+524, galaxies: jets, gamma rays: galaxies [radiation mechanisms], Astrophysics - Astrophysics of Galaxies, Galaxies: active, Galaxies: jets, Gamma rays: galaxies, Radiation mechanisms: non-thermal, Space and Planetary Science, Crab Nebula, Astrophysics of Galaxies (astro-ph.GA), active [galaxies], galaxies [gamma rays], ddc:520, Spectral energy distribution, Astrophysics - High Energy Astrophysical Phenomena, BL Lac object, Flare
Abstract

Monthly notices of the Royal Astronomical Society 451(1), 739 - 750 (2015). doi:10.1093/mnras/stv895, The high-frequency-peaked BL Lac (HBL) 1ES 0806+524 (z = 0.138) was discovered in very high energy (VHE) γ-rays in 2008. Until now, the broad-band spectrum of 1ES 0806+524 has been only poorly characterized, in particular at high energies. We analysed multiwavelength observations from γ-rays to radio performed from 2011 January to March, which were triggered by the high activity detected at optical frequencies. These observations constitute the most precise determination of the broad-band emission of 1ES 0806+524 to date. The stereoscopic Major Atmospheric Gamma-Ray Imaging Cherenkov (MAGIC) observations yielded a γ-ray signal above 250 GeV of (3.7 ± 0.7) per cent of the Crab Nebula flux with a statistical significance of 9.9σ. The multiwavelength observations showed significant variability in essentially all energy bands, including a VHE γ-ray flare that lasted less than one night, which provided unprecedented evidence for short-term variability in 1ES 0806+524. The spectrum of this flare is well described by a power law with a photon index of 2.97 ± 0.29 between ∼150 GeV and 1 TeV and an integral flux of (9.3 ± 1.9) per cent of the Crab nebula flux above 250 GeV. The spectrum during the non-flaring VHE activity is compatible with the only available VHE observation performed in 2008 with VERITAS when the source was in a low optical state. The broad-band spectral energy distribution can be described with a one-zone synchrotron self-Compton model with parameters typical for HBLs, indicating that 1ES 0806+524 is not substantially different from the HBLs previously detected., Published by Oxford Univ. Press, Oxford

Published
2015

49. Measuring the Optical Point Spread Function of FACT Using the Cherenkov Camera

Author

Max Mahlke, Fabian Temme, Daniela Dorner, J. Oberkirch, Max Ludwig Ahnen, Adrian Biland, Amit Shukla, Felicitas Pauss, Michael Blank, Vitalii Sliusar, Lena Linhoff, Aleksander Paravac, F. Schulz, Dominik Baack, Bernd Schleicher, L. Kortmann, Sebastian Achim Mueller, Anton Dmytriiev, Roland Walter, K. Bruegge, Christina Hempfling, J. Adam, Matteo Balbo, Thomas Bretz, Dorothee Hildebrand, Maximilian Noethe, Sabrina Einecke, Jens Buss, Julia Thaele, Wolfgang Rhode, Tina Herbst, Andrii Neronov, Dominik Neise, Dominik Elsaesser, and Karl Mannheim

Subjects
Physics, Point spread function, Pixel, business.industry, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Field of view, Reflector (antenna), IACT, law.invention, Radio telescope, Telescope, Optics, law, Astrophysics::Earth and Planetary Astrophysics, business, Cherenkov radiation
Abstract

FACT, the First G-APD Cherenkov Telescope, is an Imaging Air Cherenkov Telescope (IACT) operating since 2011 at the Observatorio del Roque de los Muchachos on the Canary Island of La Palma. As typical for IACTs, its reflector is comprised of smaller mirror facets and not protected by a dome. In the case of FACT, 30 hexagonal facets form a total mirror area of 9.5 m 2 . Hence, it is crucial to monitor the optical properties of this system and realign the facets if necessary. Up to now, measuring the Point Spread Function of FACT required human interaction to mount a screen and an optical camera. In this contribution, a new method to measure the optical Point Spread Function using directly the Cherenkov camera of the telescope is presented. Inspired by the method radio telescopes use to determine their resolution, the telescope is pointed towards a fixed position on the trajectory of a star. During the star’s passage through the field of view, the camera is read out using a fixed rate. In each event, the pedestal variance is determined for each pixel. This value is directly correlated with the amount of night sky background light a pixel received. Translating the time of the measurement to the position of the star in the camera enables to determine the optical point spread function from this measurement. As the measurement is done for each pixel along the trajectory of the star, the Point Spread Function can be determined not only for the camera center but for the entire field of view. In this contribution, the new method will also be compared with the existing methods of determining the optical Point Spread Function: direct measurement with an optical camera and the width of Muon ring events, PoS: Proceedings of Science, 301, ISSN:1824-8039

Published
2017

50. On improving composition measurements by combining compact Cherenkov telescopes with ground based detectors

Author

Aatif Waza, Christopher Wiebusch, Thomas Bretz, Martin Rongen, and J. Auffenberg

Subjects
Physics, Physics::Instrumentation and Detectors, business.industry, Astrophysics::High Energy Astrophysical Phenomena, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, Limiting, Galaxy, Optics, Particle, Outflow, business, Astrophysics::Galaxy Astrophysics, Energy (signal processing), Cherenkov radiation
Abstract

The cosmic ray knee is generally understood as marking the limiting energy of galactic accelerators and/or the onset of increasing outflow of particles from the galaxy. Detailed measurements of the cosmic ray composition are needed to support this prediction. The model and detector systematics of these measurements can be reduced with shower-by-shower based measurements employing independent detection techniques. Here we discuss the potential of compact imaging air Cherenkov telescopes to contribute to the composition measurement in interplay with ground based particle detectors.

Published
2017

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