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1. Prospects for realtime characterization of core-collapse supernova and neutrino properties

Author: Bendahman, Meriem, Goos, Isabel, Coelho, Joao, Bugli, Matteo, Coleiro, Alexis, Hedri, Sonia El, Foglizzo, Thierry, Franco, Davide, Guilet, Jérôme, Kouchner, Antoine, Raynaud, Raphaël, and Tayalati, Yahya
Subjects: Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Experiment
Abstract: Core-collapse supernovae (CCSNe) offer extremely valuable insights into the dynamics of galaxies. Neutrino time profiles from CCSNe, in particular, could reveal unique details about collapsing stars and particle behavior in dense environments. However, CCSNe in our galaxy and the Large Magellanic Cloud are rare and only one supernova neutrino observation has been made so far. To maximize the information obtained from the next Galactic CCSN, it is essential to combine analyses from multiple neutrino experiments in real time and transmit any relevant information to electromagnetic facilities within minutes. Locating the CCSN, in particular, is challenging, requiring disentangling CCSN localization information from observational features associated with the properties of the supernova progenitor and the physics of the neutrinos. Yet, being able to estimate the progenitor distance from the neutrino signal would be of great help for the optimisation of the electromagnetic follow-up campaign that will start soon after the propagation of the neutrino alert. Existing CCSN distance measurement algorithms based on neutrino observations hence rely on the assumption that neutrino properties can be described by the Standard Model. This paper presents a swift and robust approach to extract CCSN and neutrino physics information, leveraging diverse next-generation neutrino detectors to counteract potential measurement biases from Beyond the Standard Model effects., Comment: 37 pages, 19 figures
Published: 2023

2. The Athena X-ray Integral Field Unit: a consolidated design for the system requirement review of the preliminary definition phase

Author: Barret, Didier, Albouys, Vincent, Herder, Jan-Willem den, Piro, Luigi, Cappi, Massimo, Huovelin, Juhani, Kelley, Richard, Mas-Hesse, J. Miguel, Paltani, Stéphane, Rauw, Gregor, Rozanska, Agata, Svoboda, Jiri, Wilms, Joern, Yamasaki, Noriko, Audard, Marc, Bandler, Simon, Barbera, Marco, Barcons, Xavier, Bozzo, Enrico, Ceballos, Maria Teresa, Charles, Ivan, Costantini, Elisa, Dauser, Thomas, Decourchelle, Anne, Duband, Lionel, Duval, Jean-Marc, Fiore, Fabrizio, Gatti, Flavio, Goldwurm, Andrea, Hartog, Roland den, Jackson, Brian, Jonker, Peter, Kilbourne, Caroline, Korpela, Seppo, Macculi, Claudio, Mendez, Mariano, Mitsuda, Kazuhisa, Molendi, Silvano, Pajot, François, Pointecouteau, Etienne, Porter, Frederick, Pratt, Gabriel W., Prêle, Damien, Ravera, Laurent, Sato, Kosuke, Schaye, Joop, Shinozaki, Keisuke, Skup, Konrad, Soucek, Jan, Thibert, Tanguy, Vink, Jacco, Webb, Natalie, Chaoul, Laurence, Raulin, Desi, Simionescu, Aurora, Torrejon, Jose Miguel, Acero, Fabio, Branduardi-Raymont, Graziella, Ettori, Stefano, Finoguenov, Alexis, Grosso, Nicolas, Kaastra, Jelle, Mazzotta, Pasquale, Miller, Jon, Miniutti, Giovanni, Nicastro, Fabrizio, Sciortino, Salvatore, Yamaguchi, Hiroya, Beaumont, Sophie, Cucchetti, Edoardo, D'Andrea, Matteo, Eckart, Megan, Ferrando, Philippe, Kammoun, Elias, Lotti, Simone, Mesnager, Jean-Michel, Natalucci, Lorenzo, Peille, Philippe, de Plaa, Jelle, Ardellier, Florence, Argan, Andrea, Bellouard, Elise, Carron, Jérôme, Cavazzuti, Elisabetta, Fiorini, Mauro, Khosropanah, Pourya, Martin, Sylvain, Perry, James, Pinsard, Frederic, Pradines, Alice, Rigano, Manuela, Roelfsema, Peter, Schwander, Denis, Torrioli, Guido, Ullom, Joel, Vera, Isabel, Villegas, Eduardo Medinaceli, Zuchniak, Monika, Brachet, Frank, Cicero, Ugo Lo, Doriese, William, Durkin, Malcom, Fioretti, Valentina, Geoffray, Hervé, Jacques, Lionel, Kirsch, Christian, Smith, Stephen, Adams, Joseph, Gloaguen, Emilie, Hoogeveen, Ruud, van der Hulst, Paul, Kiviranta, Mikko, van der Kuur, Jan, Ledot, Aurélien, van Leeuwen, Bert-Joost, van Loon, Dennis, Lyautey, Bertrand, Parot, Yann, Sakai, Kazuhiro, van Weers, Henk, Abdoelkariem, Shariefa, Adam, Thomas, Adami, Christophe, Aicardi, Corinne, Akamatsu, Hiroki, Alonso, Pablo Eleazar Merino, Amato, Roberta, André, Jérôme, Angelinelli, Matteo, Anon-Cancela, Manuel, Anvar, Shebli, Atienza, Ricardo, Attard, Anthony, Auricchio, Natalia, Balado, Ana, Bancel, Florian, Barusso, Lorenzo Ferrari, Bernard, Vivian, Berrocal, Alicia, Blin, Sylvie, Bonino, Donata, Bonnet, François, Bonny, Patrick, Boorman, Peter, Boreux, Charles, Bounab, Ayoub, Boutelier, Martin, Boyce, Kevin, Brienza, Daniele, Bruijn, Marcel, Bulgarelli, Andrea, Calarco, Simona, Callanan, Paul, Camus, Thierry, Canourgues, Florent, Capobianco, Vito, Cardiel, Nicolas, Castellani, Florent, Cheatom, Oscar, Chervenak, James, Chiarello, Fabio, Clerc, Nicolas, Clerc, Laurent, Cobo, Beatriz, Coeur-Joly, Odile, Coleiro, Alexis, Colonges, Stéphane, Corcione, Leonardo, Coriat, Mickael, Coynel, Alexandre, Cuttaia, Francesco, D'Ai, Antonino, D'anca, Fabio, Dadina, Mauro, Daniel, Christophe, DeNigris, Natalie, Dercksen, Johannes, DiPirro, Michael, Doumayrou, Eric, Dubbeldam, Luc, Dupieux, Michel, Dupourqué, Simon, Durand, Jean Louis, Eckert, Dominique, Eiriz, Valvanera, Ercolani, Eric, Etcheverry, Christophe, Finkbeiner, Fred, Fiocchi, Mariateresa, Fossecave, Hervé, Franssen, Philippe, Frericks, Martin, Gabici, Stefano, Gant, Florent, Gao, Jian-Rong, Gastaldello, Fabio, Genolet, Ludovic, Ghizzardi, Simona, Gil, M Angeles Alcacera, Giovannini, Elisa, Godet, Olivier, Gomez-Elvira, Javier, Gonzalez, Manuel, Gonzalez, Raoul, Gottardi, Luciano, Granat, Dolorès, Gros, Michel, Guignard, Nicolas, Hieltjes, Paul, Hurtado, Adolfo Jesus, Irwin, Kent, Jacquey, Christian, Janiuk, Agnieszka, Jaubert, Jean, Jiménez, Maria, Jolly, Antoine, Jourdan, Thierry, Julien, Sabine, Kedziora, Bartosz, Korb, Andrew, Kreykenbohm, Ingo, König, Ole, Langer, Mathieu, Laudet, Philippe, Laurent, Philippe, Laurenza, Monica, Lesrel, Jean, Ligori, Sebastiano, Lorenz, Maximilian, Luminari, Alfredo, Maffei, Bruno, Maisonnave, Océane, Marelli, Lorenzo, Massonet, Didier, Maussang, Irwin, Melchor, Alejandro Gonzalo, Mer, Isabelle Le, Michalski, Lea, Millerioux, Jean-Pierre, Mineo, Teresa, Minervini, Gabriele, Molin, Alexeï, Monestes, David, Montinaro, Nicola, Mot, Baptiste, Murat, David, Nagayoshi, Kenichiro, Nazé, Yaël, Noguès, Loïc, Pailot, Damien, Panessa, Francesca, Parodi, Luigi, Petit, Pascal, Piconcelli, Enrico, Pinto, Ciro, Plaza, Jose Miguel Encinas, Poyatos, David, Prouvé, Thomas, Ptak, Andy, Puccetti, Simonetta, Puccio, Elena, Ramon, Pascale, Reina, Manuel, Rioland, Guillaume, Rodriguez, Louis, Roig, Anton, Rollet, Bertrand, Roncarelli, Mauro, Roudil, Gilles, Rudnicki, Tomasz, Sanisidro, Julien, Sciortino, Luisa, Silva, Vitor, Sordet, Michael, Soto-Aguilar, Javier, Spizzi, Pierre, Surace, Christian, Sánchez, Miguel Fernández, Taralli, Emanuele, Terrasa, Guilhem, Terrier, Régis, Todaro, Michela, Ubertini, Pietro, Uslenghi, Michela, de Vaate, Jan Geralt Bij, Vaccaro, Davide, Varisco, Salvatore, Varnière, Peggy, Vibert, Laurent, Vidriales, María, Villa, Fabrizio, Vodopivec, Boris Martin, Volpe, Angela, de Vries, Cor, Wakeham, Nicholas, Walmsley, Gavin, Wise, Michael, de Wit, Martin, and Woźniak, Grzegorz
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics
Abstract: The Athena X-ray Integral Unit (X-IFU) is the high resolution X-ray spectrometer, studied since 2015 for flying in the mid-30s on the Athena space X-ray Observatory, a versatile observatory designed to address the Hot and Energetic Universe science theme, selected in November 2013 by the Survey Science Committee. Based on a large format array of Transition Edge Sensors (TES), it aims to provide spatially resolved X-ray spectroscopy, with a spectral resolution of 2.5 eV (up to 7 keV) over an hexagonal field of view of 5 arc minutes (equivalent diameter). The X-IFU entered its System Requirement Review (SRR) in June 2022, at about the same time when ESA called for an overall X-IFU redesign (including the X-IFU cryostat and the cooling chain), due to an unanticipated cost overrun of Athena. In this paper, after illustrating the breakthrough capabilities of the X-IFU, we describe the instrument as presented at its SRR, browsing through all the subsystems and associated requirements. We then show the instrument budgets, with a particular emphasis on the anticipated budgets of some of its key performance parameters. Finally we briefly discuss on the ongoing key technology demonstration activities, the calibration and the activities foreseen in the X-IFU Instrument Science Center, and touch on communication and outreach activities, the consortium organisation, and finally on the life cycle assessment of X-IFU aiming at minimising the environmental footprint, associated with the development of the instrument. Thanks to the studies conducted so far on X-IFU, it is expected that along the design-to-cost exercise requested by ESA, the X-IFU will maintain flagship capabilities in spatially resolved high resolution X-ray spectroscopy, enabling most of the original X-IFU related scientific objectives of the Athena mission to be retained. (abridged)., Comment: 48 pages, 29 figures, Accepted for publication in Experimental Astronomy with minor editing
Published: 2022
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3. SNEWPY: A Data Pipeline from Supernova Simulations to Neutrino Signals

Author: Baxter, Amanda L., BenZvi, Segev, Jaimes, Joahan Castaneda, Coleiro, Alexis, Molla, Marta Colomer, Dornic, Damien, Goldhagen, Tomer, Graf, Anne M., Griswold, Spencer, Habig, Alec, Hill, Remington, Lang, Shunsaku Horiuchi James P. Kneller Rafael F., Lincetto, Massimiliano, Migenda, Jost, Nakamura, Ko, O'Connor, Evan, Renshaw, Andrew, Scholberg, Kate, Uberoi, Navya, and Worlikar, Arkin
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics, High Energy Physics - Phenomenology, Nuclear Theory
Abstract: Current neutrino detectors will observe hundreds to thousands of neutrinos from a Galactic supernovae, and future detectors will increase this yield by an order of magnitude or more. With such a data set comes the potential for a huge increase in our understanding of the explosions of massive stars, nuclear physics under extreme conditions, and the properties of the neutrino. However, there is currently a large gap between supernova simulations and the corresponding signals in neutrino detectors, which will make any comparison between theory and observation very difficult. SNEWPY is an open-source software package which bridges this gap. The SNEWPY code can interface with supernova simulation data to generate from the model either a time series of neutrino spectral fluences at Earth, or the total time-integrated spectral fluence. Data from several hundred simulations of core-collapse, thermonuclear, and pair-instability supernovae is included in the package. This output may then be used by an event generator such as sntools or an event rate calculator such as SNOwGLoBES. Additional routines in the SNEWPY package automate the processing of the generated data through the SNOwGLoBES software and collate its output into the observable channels of each detector. In this paper we describe the contents of the package, the physics behind SNEWPY, the organization of the code, and provide examples of how to make use of its capabilities., Comment: Software available at https://github.com/SNEWS2/snewpy
Published: 2021

4. INTEGRAL reloaded: spacecraft, instruments and ground system

Author: Kuulkers, Erik, Ferrigno, Carlo, Kretschmar, Peter, Alfonso-Garzon, Julia, Baab, Marius, Bazzano, Angela, Belanger, Guillaume, Benson, Ian, Bird, Anthony J., Bozzo, Enrico, Brandt, Soren, Coe, Elliott, Caballero, Isabel, Cangemi, Floriane, Chenevez, Jerome, Cenko, Bradley, Cinar, Nebil, Coleiro, Alexis, De Padova, Stefano, Diehl, Roland, Dietze, Claudia, Domingo, Albert, Drapes, Mark, D'uva, Eleonora, Ehle, Matthias, Ebrero, Jacobo, Edirimanne, Mithrajith, Eismont, Natan A., Finn, Timothy, Fiocchi, Mariateresa, Tomas, Elena Garcia, Gaudenzi, Gianluca, Godard, Thomas, Goldwurm, Andrea, Gotz, Diego, Gouiffes, Christian, Grebenev, Sergei A., Greiner, Jochen, Gros, Aleksandra, Hanlon, Lorraine, Hermsen, Wim, Hernandez, Cristina, Hernanz, Margarita, Huebner, Jutta, Jourdain, Elisabeth, La Rosa, Giovanni, Labanti, Claudio, Laurent, Philippe, Lehanka, Alexander, Lund, Niels, Madison, James, Malzac, Julien, Martin, Jim, Mas-Hesse, J. Miguel, McBreen, Brian, McDonald, Alastair, McEnery, Julie, Mereghetti, Sandro, Natalucci, Lorenzo, Ness, Jan-Uwe, Oxborrow, Carol Anne, Palmer, John, Peschke, Sibylle, Petrucciani, Francesco, Pfeil, Norbert, Reichenbaecher, Michael, Rodi, James, Rodriguez, Jerome, Roques, Jean-Pierre, Donate, Emilio Salazar, Salt, Dave, Sanchez-Fernandez, Celia, Sauvageon, Aymeric, Savchenko, Volodymyr, Sazonov, Sergey Yu., Scaglioni, Stefano, Schartel, Norbert, Siegert, Thomas, Southworth, Richard, Sunyaev, Rashid A., Toma, Liviu, Ubertini, Pietro, Heuvel, Ed P. J. van den, von Kienlin, Andreas, von Krusenstiern, Nikolai, Winkler, Christoph, Wojciech, Hajdas, and Zannoni, Ugo
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Experiment
Abstract: ESA's INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL) was launched on 17 Oct 2002 at 06:41 CEST. Since then, it has been providing long, uninterrupted observations (up to about 47 hr, or 170 ksec, per satellite orbit of 2.7 days) with a large field-of-view (fully coded: 100 deg^2), msec time resolution, keV energy resolution, polarization measurements, as well as additional coverage in the optical. This is realized by two main instruments in the 15 keV to 10 MeV range, the spectrometer SPI (spectral resolution 3 keV at 1.8 MeV) and the imager IBIS (angular resolution 12 arcmin FWHM), complemented by X-ray (JEM-X; 3-35 keV) and optical (OMC; Johnson V-band) monitors. All instruments are co-aligned to simultaneously observe the target region. A particle radiation monitor (IREM) measures charged particle fluxes near the spacecraft. The Anti-coincidence subsystems of the main instruments are also efficient all-sky gamma-ray detectors, which provide omni-directional monitoring above ~75 keV. INTEGRAL can also rapidly (within a couple of hours) re-point and conduct Target of Opportunity observations. INTEGRAL has build an impressive legacy: e.g. discovery of >600 new high-energy sources; first-ever direct detection of 56Ni and 56Co radio-active decay lines from a Type Ia supernova; new insights on positron annihilation in the Galactic bulge and disk; pioneering gamma-ray polarization studies. INTEGRAL is also a successful in multi-messenger astronomy: INTEGRAL found the first prompt electromagnetic radiation in coincidence with a binary neutron star merger. More than 1750 papers based on INTEGRAL data have been published in refereed journals. Here we give a comprehensive update of the satellite status after more than 18 years of operations in a harsh space environment, and an account of the successful Ground Segment., Comment: 29 pages, 20 figures, accepted for publication in special issue of New Astronomy Reviews
Published: 2021

5. The Athena X-ray Integral Field Unit: a consolidated design for the system requirement review of the preliminary definition phase

Author: Barret, Didier, Albouys, Vincent, Herder, Jan-Willem den, Piro, Luigi, Cappi, Massimo, Huovelin, Juhani, Kelley, Richard, Mas-Hesse, J. Miguel, Paltani, Stéphane, Rauw, Gregor, Rozanska, Agata, Svoboda, Jiri, Wilms, Joern, Yamasaki, Noriko, Audard, Marc, Bandler, Simon, Barbera, Marco, Barcons, Xavier, Bozzo, Enrico, Ceballos, Maria Teresa, Charles, Ivan, Costantini, Elisa, Dauser, Thomas, Decourchelle, Anne, Duband, Lionel, Duval, Jean-Marc, Fiore, Fabrizio, Gatti, Flavio, Goldwurm, Andrea, Hartog, Roland den, Jackson, Brian, Jonker, Peter, Kilbourne, Caroline, Korpela, Seppo, Macculi, Claudio, Mendez, Mariano, Mitsuda, Kazuhisa, Molendi, Silvano, Pajot, François, Pointecouteau, Etienne, Porter, Frederick, Pratt, Gabriel W., Prêle, Damien, Ravera, Laurent, Sato, Kosuke, Schaye, Joop, Shinozaki, Keisuke, Skup, Konrad, Soucek, Jan, Thibert, Tanguy, Vink, Jacco, Webb, Natalie, Chaoul, Laurence, Raulin, Desi, Simionescu, Aurora, Torrejon, Jose Miguel, Acero, Fabio, Branduardi-Raymont, Graziella, Ettori, Stefano, Finoguenov, Alexis, Grosso, Nicolas, Kaastra, Jelle, Mazzotta, Pasquale, Miller, Jon, Miniutti, Giovanni, Nicastro, Fabrizio, Sciortino, Salvatore, Yamaguchi, Hiroya, Beaumont, Sophie, Cucchetti, Edoardo, D’Andrea, Matteo, Eckart, Megan, Ferrando, Philippe, Kammoun, Elias, Lotti, Simone, Mesnager, Jean-Michel, Natalucci, Lorenzo, Peille, Philippe, de Plaa, Jelle, Ardellier, Florence, Argan, Andrea, Bellouard, Elise, Carron, Jérôme, Cavazzuti, Elisabetta, Fiorini, Mauro, Khosropanah, Pourya, Martin, Sylvain, Perry, James, Pinsard, Frederic, Pradines, Alice, Rigano, Manuela, Roelfsema, Peter, Schwander, Denis, Torrioli, Guido, Ullom, Joel, Vera, Isabel, Villegas, Eduardo Medinaceli, Zuchniak, Monika, Brachet, Frank, Cicero, Ugo Lo, Doriese, William, Durkin, Malcom, Fioretti, Valentina, Geoffray, Hervé, Jacques, Lionel, Kirsch, Christian, Smith, Stephen, Adams, Joseph, Gloaguen, Emilie, Hoogeveen, Ruud, van der Hulst, Paul, Kiviranta, Mikko, van der Kuur, Jan, Ledot, Aurélien, van Leeuwen, Bert-Joost, van Loon, Dennis, Lyautey, Bertrand, Parot, Yann, Sakai, Kazuhiro, van Weers, Henk, Abdoelkariem, Shariefa, Adam, Thomas, Adami, Christophe, Aicardi, Corinne, Akamatsu, Hiroki, Alonso, Pablo Eleazar Merino, Amato, Roberta, André, Jérôme, Angelinelli, Matteo, Anon-Cancela, Manuel, Anvar, Shebli, Atienza, Ricardo, Attard, Anthony, Auricchio, Natalia, Balado, Ana, Bancel, Florian, Barusso, Lorenzo Ferrari, Bascuñan, Arturo, Bernard, Vivian, Berrocal, Alicia, Blin, Sylvie, Bonino, Donata, Bonnet, François, Bonny, Patrick, Boorman, Peter, Boreux, Charles, Bounab, Ayoub, Boutelier, Martin, Boyce, Kevin, Brienza, Daniele, Bruijn, Marcel, Bulgarelli, Andrea, Calarco, Simona, Callanan, Paul, Campello, Alberto Prada, Camus, Thierry, Canourgues, Florent, Capobianco, Vito, Cardiel, Nicolas, Castellani, Florent, Cheatom, Oscar, Chervenak, James, Chiarello, Fabio, Clerc, Laurent, Clerc, Nicolas, Cobo, Beatriz, Coeur-Joly, Odile, Coleiro, Alexis, Colonges, Stéphane, Corcione, Leonardo, Coriat, Mickael, Coynel, Alexandre, Cuttaia, Francesco, D’Ai, Antonino, D’anca, Fabio, Dadina, Mauro, Daniel, Christophe, Dauner, Lea, DeNigris, Natalie, Dercksen, Johannes, DiPirro, Michael, Doumayrou, Eric, Dubbeldam, Luc, Dupieux, Michel, Dupourqué, Simon, Durand, Jean Louis, Eckert, Dominique, Eiriz, Valvanera, Ercolani, Eric, Etcheverry, Christophe, Finkbeiner, Fred, Fiocchi, Mariateresa, Fossecave, Hervé, Franssen, Philippe, Frericks, Martin, Gabici, Stefano, Gant, Florent, Gao, Jian-Rong, Gastaldello, Fabio, Genolet, Ludovic, Ghizzardi, Simona, Gil, Ma Angeles Alcacera, Giovannini, Elisa, Godet, Olivier, Gomez-Elvira, Javier, Gonzalez, Raoul, Gonzalez, Manuel, Gottardi, Luciano, Granat, Dolorès, Gros, Michel, Guignard, Nicolas, Hieltjes, Paul, Hurtado, Adolfo Jesús, Irwin, Kent, Jacquey, Christian, Janiuk, Agnieszka, Jaubert, Jean, Jiménez, Maria, Jolly, Antoine, Jourdan, Thierry, Julien, Sabine, Kedziora, Bartosz, Korb, Andrew, Kreykenbohm, Ingo, König, Ole, Langer, Mathieu, Laudet, Philippe, Laurent, Philippe, Laurenza, Monica, Lesrel, Jean, Ligori, Sebastiano, Lorenz, Maximilian, Luminari, Alfredo, Maffei, Bruno, Maisonnave, Océane, Marelli, Lorenzo, Massonet, Didier, Maussang, Irwin, Melchor, Alejandro Gonzalo, Le Mer, Isabelle, Millan, Francisco Javier San, Millerioux, Jean-Pierre, Mineo, Teresa, Minervini, Gabriele, Molin, Alexeï, Monestes, David, Montinaro, Nicola, Mot, Baptiste, Murat, David, Nagayoshi, Kenichiro, Nazé, Yaël, Noguès, Loïc, Pailot, Damien, Panessa, Francesca, Parodi, Luigi, Petit, Pascal, Piconcelli, Enrico, Pinto, Ciro, Plaza, Jose Miguel Encinas, Plaza, Borja, Poyatos, David, Prouvé, Thomas, Ptak, Andy, Puccetti, Simonetta, Puccio, Elena, Ramon, Pascale, Reina, Manuel, Rioland, Guillaume, Rodriguez, Louis, Roig, Anton, Rollet, Bertrand, Roncarelli, Mauro, Roudil, Gilles, Rudnicki, Tomasz, Sanisidro, Julien, Sciortino, Luisa, Silva, Vitor, Sordet, Michael, Soto-Aguilar, Javier, Spizzi, Pierre, Surace, Christian, Sánchez, Miguel Fernández, Taralli, Emanuele, Terrasa, Guilhem, Terrier, Régis, Todaro, Michela, Ubertini, Pietro, Uslenghi, Michela, de Vaate, Jan Geralt Bij, Vaccaro, Davide, Varisco, Salvatore, Varnière, Peggy, Vibert, Laurent, Vidriales, María, Villa, Fabrizio, Vodopivec, Boris Martin, Volpe, Angela, de Vries, Cor, Wakeham, Nicholas, Walmsley, Gavin, Wise, Michael, de Wit, Martin, and Woźniak, Grzegorz
Published: 2023
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6. Fink, a new generation of broker for the LSST community

Author: Möller, Anais, Peloton, Julien, Ishida, Emille E. O., Arnault, Chris, Bachelet, Etienne, Blaineau, Tristan, Boutigny, Dominique, Chauhan, Abhishek, Gangler, Emmanuel, Hernandez, Fabio, Hrivnac, Julius, Leoni, Marco, Leroy, Nicolas, Moniez, Marc, Pateyron, Sacha, Ramparison, Adrien, Turpin, Damien, Ansari, Réza, Allam Jr., Tarek, Bajat, Armelle, Biswas, Biswajit, Boucaud, Alexandre, Bregeon, Johan, Campagne, Jean-Eric, Cohen-Tanugi, Johann, Coleiro, Alexis, Dornic, Damien, Fouchez, Dominique, Godet, Olivier, Gris, Philippe, Karpov, Sergey, Gomez-Moran, Ada Nebot, Neveu, Jérémy, Plaszczynski, Stephane, Savchenko, Volodymyr, and Webb, Natalie
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract: Fink is a broker designed to enable science with large time-domain alert streams such as the one from the upcoming Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST). It exhibits traditional astronomy broker features such as automatised ingestion, annotation, selection and redistribution of promising alerts for transient science. It is also designed to go beyond traditional broker features by providing real-time transient classification which is continuously improved by using state-of-the-art Deep Learning and Adaptive Learning techniques. These evolving added values will enable more accurate scientific output from LSST photometric data for diverse science cases while also leading to a higher incidence of new discoveries which shall accompany the evolution of the survey. In this paper we introduce Fink, its science motivation, architecture and current status including first science verification cases using the Zwicky Transient Facility alert stream., Comment: accepted in MNRAS
Published: 2020
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7. Multimessenger observations of counterparts to IceCube-190331A

Author: Krauß, Felicia, Calamari, Emily, Keivani, Azadeh, Coleiro, Alexis, Evans, Phil A., Fox, Derek B., Kennea, Jamie A., Mészáros, Peter, Murase, Kohta, Russell, Thomas D., Santander, Marcos, and Tohuvavohu, Aaron
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: High-energy neutrinos are a promising tool for identifying astrophysical sources of high and ultra-high energy cosmic rays (UHECR). Prospects of detecting neutrinos at high energies ($\gtrsim$TeV) from blazars have been boosted after the recent association of IceCube-170922A and TXS 0506+056. We investigate the high-energy neutrino, IceCube-190331A, a high-energy starting event (HESE) with a high likelihood of being astrophysical in origin. We initiated a Swift/XRT and UVOT tiling mosaic of the neutrino localisation, and followed up with ATCA radio observations, compiling a multiwavelength SED for the most likely source of origin. NuSTAR observations of the neutrino location and a nearby X-ray source were also performed. We find two promising counterpart in the 90% confidence localisation region and identify the brightest as the most likely counterpart. However, no Fermi/LAT $\gamma$-ray source and no prompt Swift/BAT source is consistent with the neutrino event. At this point it is unclear whether any of the counterparts produced IceCube-190331A. We note that the Helix Nebula is also consistent with the position of the neutrino event, and we calculate that associated particle acceleration processes cannot produce the required energies to generate a high-energy HESE neutrino., Comment: 10 pages, 8 figures. Accepted for publication by MNRAS
Published: 2020
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8. Event reconstruction for KM3NeT/ORCA using convolutional neural networks

Author: Aiello, Sebastiano, Albert, Arnauld, Garre, Sergio Alves, Aly, Zineb, Ameli, Fabrizio, Andre, Michel, Androulakis, Giorgos, Anghinolfi, Marco, Anguita, Mancia, Anton, Gisela, Ardid, Miquel, Aublin, Julien, Bagatelas, Christos, Barbarino, Giancarlo, Baret, Bruny, Pree, Suzan Basegmez du, Bendahman, Meriem, Berbee, Edward, Bertin, Vincent, Biagi, Simone, Biagioni, Andrea, Bissinger, Matthias, Boettcher, Markus, Boumaaza, Jihad, Bouta, Mohammed, Bouwhuis, Mieke, Bozza, Cristiano, Branzas, Horea, Bruijn, Ronald, Brunner, Jürgen, Buis, Ernst-Jan, Buompane, Raffaele, Busto, Jose, Caiffi, Barbara, Calvo, David, Capone, Antonio, Carretero, Víctor, Castaldi, Paolo, Celli, Silvia, Chabab, Mohamed, Chau, Nhan, Chen, Andrew, Cherubini, Silvio, Chiarella, Vitaliano, Chiarusi, Tommaso, Circella, Marco, Cocimano, Rosanna, Coelho, Joao, Coleiro, Alexis, Molla, Marta Colomer, Coniglione, Rosa, Coyle, Paschal, Creusot, Alexandre, Cuttone, Giacomo, D'Onofrio, Antonio, Dallier, Richard, de Jong, Maarten, de Jong, Paul, De Palma, Mauro, de Wasseige, Gwenhaël, de Wolf, Els, Di Palma, Irene, Diaz, Antonio, Diego-Tortosa, Dídac, Distefano, Carla, Domi, Alba, Donà, Roberto, Donzaud, Corinne, Dornic, Damien, Dörr, Manuel, Drouhin, Doriane, Eberl, Thomas, Bojaddaini, Imad El, Elsaesser, Dominik, Enzenhöfer, Alexander, Fermani, Paolo, Ferrara, Giovanna, Filipovic, Miroslav, Filippini, Francesco, Fusco, Luigi Antonio, Gabella, Omar, Gal, Tamas, Soto, Alfonso Andres Garcia, Garufi, Fabio, Gatelet, Yoann, Geißelbrecht, Nicole, Gialanella, Lucio, Giorgio, Emidio, Gozzini, Sara Rebecca, Gracia, Rodrigo, Graf, Kay, Grasso, Dario, Grella, Giuseppe, Guidi, Carlo, Hallmann, Steffen, Hamdaoui, Hassane, Heijboer, Aart, Hekalo, Amar, Hernandez-Rey, Juan-Jose, Hofestädt, Jannik, Huang, Feifei, Ibnsalih, Walid Idrissi, Illuminati, Giulia, James, Clancy, Jung, Bouke Jisse, Kadler, Matthias, Kalaczyński, Piotr, Kalekin, Oleg, Katz, Uli, Chowdhury, Nafis Rezwan Khan, Kistauri, Giorgi, Koffeman, Els, Kooijman, Paul, Kouchner, Antoine, Kreter, Michael, Kulikovskiy, Vladimir, Lahmann, Robert, Larosa, Giuseppina, Breton, Remy Le, Leonardi, Ornella, Leone, Francesco, Leonora, Emanuele, Levi, Giuseppe, Lincetto, Massimiliano, Clark, Miles Lindsey, Lipreau, Thomas, Lonardo, Alessandro, Longhitano, Fabio, Coto, Daniel Lopez, Maderer, Lukas, Mańczak, Jerzy, Mannheim, Karl, Margiotta, Annarita, Marinelli, Antonio, Markou, Christos, Martin, Lilian, Martínez-Mora, Juan Antonio, Martini, Agnese, Marzaioli, Fabio, Mastroianni, Stefano, Mazzou, Safaa, Melis, Karel, Miele, Gennaro, Migliozzi, Pasquale, Migneco, Emilio, Mijakowski, Piotr, Palacios, Luis Salvador Miranda, Mollo, Carlos Maximiliano, Morganti, Mauro, Moser, Michael, Moussa, Abdelilah, Muller, Rasa, Musumeci, Mario, Nauta, Lodewijk, Navas, Sergio, Nicolau, Carlo Alessandro, Fearraigh, Brían Ó, Organokov, Mukharbek, Orlando, Angelo, Papalashvili, Gogita, Papaleo, Riccardo, Pastore, Cosimo, Paun, Alice, Pavalas, Gabriela Emilia, Pellegrino, Carmelo, Perrin-Terrin, Mathieu, Piattelli, Paolo, Pieterse, Camiel, Pikounis, Konstantinos, Pisanti, Ofelia, Poirè, Chiara, Popa, Vlad, Post, Maarten, Pradier, Thierry, Pühlhofer, Gerd, Pulvirenti, Sara, Rabyang, Omphile, Raffaelli, Fabrizio, Randazzo, Nunzio, Rapicavoli, Antonio, Razzaque, Soebur, Real, Diego, Reck, Stefan, Riccobene, Giorgio, Richer, Marc, Rivoire, Stephane, Rovelli, Alberto, Greus, Francisco Salesa, Samtleben, Dorothea Franziska Elisabeth, Losa, Agustín Sánchez, Sanguineti, Matteo, Santangelo, Andrea, Santonocito, Domenico, Sapienza, Piera, Schnabel, Jutta, Seneca, Jordan, Sgura, Irene, Shanidze, Rezo, Sharma, Ankur, Simeone, Francesco, Sinopoulou, Anna, Spisso, Bernardino, Spurio, Maurizio, Stavropoulos, Dimitris, Steijger, Jos, Stellacci, Simona Maria, Taiuti, Mauro, Tayalati, Yahya, Tenllado, Enrique, Thakore, Tarak, Tingay, Steven, Tzamariudaki, Ekaterini, Tzanetatos, Dimitrios, Berg, Ad van den, van der Knaap, Frits, van Eijk, Daan, Van Elewyck, Véronique, van Haren, Hans, Vannoye, Godefroy, Vasileiadis, George, Versari, Federico, Viola, Salvatore, Vivolo, Daniele, Wilms, Joern, Wojaczyński, Rafał, Zaborov, Dmitry, Zavatarelli, Sandra, Zegarelli, Angela, Zito, Daniele, Zornoza, Juan-de-Dios, Zúñiga, Juan, and Zywucka, Natalia
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, High Energy Physics - Experiment, Physics - Instrumentation and Detectors
Abstract: The KM3NeT research infrastructure is currently under construction at two locations in the Mediterranean Sea. The KM3NeT/ORCA water-Cherenkov neutrino detector off the French coast will instrument several megatons of seawater with photosensors. Its main objective is the determination of the neutrino mass ordering. This work aims at demonstrating the general applicability of deep convolutional neural networks to neutrino telescopes, using simulated datasets for the KM3NeT/ORCA detector as an example. To this end, the networks are employed to achieve reconstruction and classification tasks that constitute an alternative to the analysis pipeline presented for KM3NeT/ORCA in the KM3NeT Letter of Intent. They are used to infer event reconstruction estimates for the energy, the direction, and the interaction point of incident neutrinos. The spatial distribution of Cherenkov light generated by charged particles induced in neutrino interactions is classified as shower- or track-like, and the main background processes associated with the detection of atmospheric neutrinos are recognized. Performance comparisons to machine-learning classification and maximum-likelihood reconstruction algorithms previously developed for KM3NeT/ORCA are provided. It is shown that this application of deep convolutional neural networks to simulated datasets for a large-volume neutrino telescope yields competitive reconstruction results and performance improvements with respect to classical approaches.
Published: 2020
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9. gSeaGen: the KM3NeT GENIE-based code for neutrino telescopes

Author: Aiello, Sebastiano, Albert, Arnauld, Garre, Sergio Alves, Aly, Zineb, Ameli, Fabrizio, Andre, Michel, Androulakis, Giorgos, Anghinolfi, Marco, Anguita, Mancia, Anton, Gisela, Ardid, Miquel, Aublin, Julien, Bagatelas, Christos, Barbarino, Giancarlo, Baret, Bruny, Pree, Suzan Basegmez du, Bendahman, Meriem, Berbee, Edward, Bertin, Vincent, Biagi, Simone, Biagioni, Andrea, Bissinger, Matthias, Boettcher, Markus, Boumaaza, Jihad, Bourret, Simon, Bouta, Mohammed, Bouwhuis, Mieke, Bozza, Cristiano, Branzas, Horea, Bruchner, Marc, Bruijn, Ronald, Brunner, Jürgen, Buis, Ernst-Jan, Buompane, Raffaele, Busto, Jose, Calvo, David, Capone, Antonio, Carretero, Víctor, Castaldi, Paolo, Celli, Silvia, Chabab, Mohamed, Chau, Nhan, Chen, Andrew, Cherubini, Silvio, Chiarella, Vitaliano, Chiarusi, Tommaso, Circella, Marco, Cocimano, Rosanna, Coelho, Joao, Coleiro, Alexis, Molla, Marta Colomer, Coniglione, Rosa, Corredoira, Imanol, Coyle, Paschal, Creusot, Alexandre, Cuttone, Giacomo, D'Onofrio, Antonio, Dallier, Richard, de Jong, Maarten, de Jong, Paul, De Palma, Mauro, de Wasseige, Gwenhaël, de Wolf, Els, Di Palma, Irene, Diaz, Antonio, Diego-Tortosa, Dídac, Distefano, Carla, Domi, Alba, Donà, Roberto, Donzaud, Corinne, Dornic, Damien, Dörr, Manuel, Drouhin, Doriane, Durocher, Mora, Eberl, Thomas, Bojaddaini, Imad El, Elsaesser, Dominik, Enzenhöfer, Alexander, Fermani, Paolo, Ferrara, Giovanna, Filipovic, Miroslav, Filippini, Francesco, Franco, Antonio, Fusco, Luigi Antonio, Gabella, Omar, Gal, Tamas, Soto, Alfonso Andres Garcia, Garufi, Fabio, Gatelet, Yoann, Geißelbrecht, Nicole, Gialanella, Lucio, Giorgio, Emidio, Gozzini, Sara Rebecca, Gracia, Rodrigo, Graf, Kay, Grasso, Dario, Grégoire, Timothée, Grella, Giuseppe, Guidi, Carlo, Hallmann, Steffen, Hamdaoui, Hassane, Heijboer, Aart, Hekalo, Amar, Hernandez-Rey, Juan-Jose, Hofestädt, Jannik, Ibnsalih, Walid Idrissi, Illuminati, Giulia, James, Clancy, Jung, Bouke Jisse, Kadler, Matthias, Kalaczyński, Piotr, Kalekin, Oleg, Katz, Uli, Chowdhury, Nafis Rezwan Khan, Koffeman, Els, Kooijman, Paul, Kouchner, Antoine, Kreter, Michael, Kulikovskiy, Vladimir, Lahmann, Robert, Larosa, Giuseppina, Breton, Remy Le, Leonardi, Ornella, Leone, Francesco, Leonora, Emanuele, Levi, Giuseppe, Lincetto, Massimiliano, Clark, Miles Lindsey, Lipreau, Thomas, Lonardo, Alessandro, Longhitano, Fabio, Coto, Daniel Lopez, Mańczak, Jerzy, Mannheim, Karl, Margiotta, Annarita, Marinelli, Antonio, Markou, Christos, Martin, Lilian, Martínez-Mora, Juan Antonio, Martini, Agnese, Marzaioli, Fabio, Mastroianni, Stefano, Mazzou, Safaa, Melis, Karel, Miele, Gennaro, Migliozzi, Pasquale, Migneco, Emilio, Mijakowski, Piotr, Palacios, Luis Salvador Miranda, Modebadze, Zurab, Mollo, Carlos Maximiliano, Morganti, Mauro, Moser, Michael, Moussa, Abdelilah, Muller, Rasa, Musumeci, Mario, Nauta, Lodewijk, Navas, Sergio, Nicolau, Carlo Alessandro, Fearraigh, Brían Ó, Organokov, Mukharbek, Orlando, Angelo, Papalashvili, Gogita, Papaleo, Riccardo, Pastore, Cosimo, Paun, Alice, Pavalas, Gabriela Emilia, Pellegrino, Carmelo, Perrin-Terrin, Mathieu, Piattelli, Paolo, Pieterse, Camiel, Pikounis, Konstantinos, Pisanti, Ofelia, Poirè, Chiara, Popa, Vlad, Post, Maarten, Pradier, Thierry, Pühlhofer, Gerd, Pulvirenti, Sara, Quinn, Liam, Rabyang, Omphile, Raffaelli, Fabrizio, Randazzo, Nunzio, Rapicavoli, Antonio, Razzaque, Soebur, Real, Diego, Reck, Stefan, Reubelt, Jonas, Riccobene, Giorgio, Richer, Marc, Rivoire, Stephane, Rovelli, Alberto, Greus, Francisco Salesa, Samtleben, Dorothea Franziska Elisabeth, Losa, Agustín Sánchez, Sanguineti, Matteo, Santangelo, Andrea, Santonocito, Domenico, Sapienza, Piera, Schnabel, Jutta, Sciacca, Virginia, Seneca, Jordan, Sgura, Irene, Shanidze, Rezo, Sharma, Ankur, Simeone, Francesco, Sinopoulou, Anna, Spisso, Bernardino, Spurio, Maurizio, Stavropoulos, Dimitris, Steijger, Jos, Stellacci, Simona Maria, Taiuti, Mauro, Tayalati, Yahya, Tenllado, Enrique, Thakore, Tarak, Tingay, Steven, Tzamariudaki, Ekaterini, Tzanetatos, Dimitrios, Berg, Ad van den, van der Knaap, Frits, van Eijk, Daan, Van Elewyck, Véronique, Vannoye, Godefroy, Vasileiadis, George, Versari, Federico, Viola, Salvatore, Vivolo, Daniele, Wilms, Joern, Wojaczyński, Rafał, Zaborov, Dmitry, Zavatarelli, Sandra, Zegarelli, Angela, Zornoza, Juan-de-Dios, Zúñiga, Juan, and Zywucka, Natalia
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: The gSeaGen code is a GENIE-based application developed to efficiently generate high statistics samples of events, induced by neutrino interactions, detectable in a neutrino telescope. The gSeaGen code is able to generate events induced by all neutrino flavours, considering topological differences between track-type and shower-like events. Neutrino interactions are simulated taking into account the density and the composition of the media surrounding the detector. The main features of gSeaGen are presented together with some examples of its application within the KM3NeT project., Comment: 45 pages, 10 figures
Published: 2020
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10. Combining neutrino experimental light-curves for pointing to the next Galactic Core-Collapse Supernova

Author: Coleiro, Alexis, Molla, Marta Colomer, Dornic, Damien, Lincetto, Massimiliano, and Kulikovskiy, Vladimir
Subjects: Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Experiment
Abstract: The multi-messenger observation of the next galactic core-collapse supernova will shed light on the different physical processes involved in these energetic explosions. Good timing and pointing capabilities of neutrino detectors would help in the search for an electromagnetic or gravitational-wave counterparts. An approach for the determination of the arrival time delay of the neutrino signal at different experiments using a direct detected neutrino light-curve matching is discussed. A simplified supernova model and detector simulation are used for its application. The arrival time delay and its uncertainty between two neutrino detectors are estimated with chi-square and cross-correlation methods. The direct comparison of the detected light-curves offers the advantage to be model-independent. Millisecond time resolution on the arrival time delay at two different detectors is needed. Using the computed time delay between different combinations of currently operational and future detectors, a triangulation method is used to infer the supernova localisation in the sky. The combination of IceCube, Hyper-Kamiokande, JUNO and KM3NeT/ARCA provides a 90% confidence area of 140$\pm$20 deg$^2$. These low-latency analysis methods can be implemented in the SNEWS alert system., Comment: 12 pages, 4 figures, 6 tables, corresponding authors: Marta Colomer Molla and Vladimir Kulikovskiy
Published: 2020
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11. Athena synergies in the multi-messenger and transient universe

Author: Piro, Luigi, Ahlers, Markus, Coleiro, Alexis, Colpi, Monica, de Oña Wilhelmi, Emma, Guainazzi, Matteo, Jonker, Peter G., Namara, Paul Mc, Nichols, David A., O’Brien, Paul, Troja, Eleonora, Vink, Jacco, Aird, James, Amati, Lorenzo, Anand, Shreya, Bozzo, Enrico, Carrera, Francisco J., Fabian, Andrew C., Fryer, Christopher, Hall, Evan, Korobkin, Oleg, Korol, Valeriya, Mangiagli, Alberto, Martínez-Núñez, Silvia, Nissanke, Samaya, Osborne, Julien, Padovani, Paolo, Rossi, Elena M., Ryan, Geoffrey, Sesana, Alberto, Stratta, Giulia, Tanvir, Niel, and van Eerten, Hendrik
Published: 2022
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12. The Power Board of the KM3NeT Digital Optical Module: Design, Upgrade, and Production

Author: Aiello, Sebastiano, primary, Albert, Arnauld, additional, Garre, Sergio, additional, Aly, Zineb, additional, Ambrosone, Antonio, additional, Ameli, Fabrizio, additional, Andre, Michel, additional, Androutsou, Eleni, additional, Anguita, Mancia, additional, Aphecetche, Laurent, additional, Ardid, Miguel, additional, Ardid, Salva, additional, Atmani, Hicham, additional, Aublin, Julien, additional, Badaracco, Francesca, additional, Bailly-Salins, Louis, additional, Bardacova, Zuzana, additional, Baret, Bruny, additional, Bariego, Adriana, additional, Du Pree, Suzan, additional, Becherini, Yvonne, additional, Bendahman, Meriem, additional, Benfenati, Francesco, additional, Benhassi, Marouane, additional, Benoit, David, additional, Berbee, Edward, additional, Bertin, Vincent, additional, Biagi, Simone, additional, Boettcher, Markus, additional, Bonanno, Danilo, additional, Boumaaza, Jihad, additional, Bouta, Mohammed, additional, Bouwhuis, Mieke, additional, Bozza, Cristiano, additional, Bozza, Riccardo, additional, Branzas, Horea, additional, Bretaudeau, Felix, additional, Bruijn, Ronald, additional, Brunner, Jurgen, additional, Bruno, Riccardo, additional, Buis, Ernst, additional, Buompane, Raffaele, additional, Busto, Jose, additional, Caiffi, Barbara, additional, Calvo, David, additional, Campion, Stefano, additional, Capone, Antonio, additional, Carenini, Francesco, additional, Carretero, Víctor, additional, Cartraud, Théophile, additional, Castaldi, Paolo, additional, Cecchini, Vincent, additional, Celli, Silvia, additional, Cerisy, Luc, additional, Chabab, Mohamed, additional, Chadolias, Michael, additional, Champion, Cèdric, additional, Chen, Andrew, additional, Cherubini, Silvio, additional, Chiarusi, Tommaso, additional, Circella, Marco, additional, Cocimano, Rosanna, additional, Coelho, João, additional, Coleiro, Alexis, additional, Colonges, Stephane, additional, Coniglione, Rosa, additional, Coyle, Paschal, additional, Creusot, Alexandre, additional, Cuttone, Giacomo, additional, Dallier, Richard, additional, Darras, Yara, additional, De Benedittis, Antonio, additional, de Jong, Maarten, additional, de Jong, Paul, additional, De Martino, Bianca, additional, de Wolf, Els, additional, Decoene, Valentin, additional, Del Burgo, Riccardo, additional, Del Rosso, Ilaria, additional, Di Cerbo, Umberto, additional, Di Mauro, Letizia, additional, Di Palma, Irene, additional, Diaz, Antonio, additional, Martín, Cristian, additional, Diego-Tortosa, Dídac, additional, Distefano, Carla, additional, Domi, Alba, additional, Donzaud, Corinne, additional, Dornic, Damien, additional, Dörr, Manuel, additional, Drakopoulou, Evangelia, additional, Drouhin, Doriane, additional, Dvornický, Rastislav, additional, Eberl, Thomas, additional, Eckerova, Eliska, additional, Eddymaoui, Ahmed, additional, Eff, Maximilian, additional, El Bojaddaini, Imad, additional, El Hedri, Sonia, additional, Enzenhöfer, Alexander, additional, Ferrara, Giovanna, additional, Filipovic, Miroslav, additional, Filippini, Francesco, additional, Franciotti, Dino, additional, Antonio Fusco, Luigi, additional, Gabella, Omar, additional, Gabriel, Jean-Louis, additional, Gagliardini, Silvia, additional, Gal, Tamas, additional, García Méndez, Juan, additional, Garcia Soto, Alfonso, additional, Oliver, Clara, additional, Geißelbrecht, Nicole, additional, Ghaddari, Houria, additional, Gialanella, Lucio, additional, Gibson, Brad, additional, Giorgio, Emidio, additional, Goos, Isabel, additional, Goswami, Pranjupriya, additional, Goupilliere, Damien, additional, Gozzini, Sara, additional, Gracia, Rodrigo, additional, Graf, Kay, additional, Guidi, Carlo, additional, Guillon, Benoît, additional, Gutiérrez, Miguel, additional, Heijboer, Aart, additional, Hekalo, Amar, additional, Hennig, Lukas, additional, Hernandez-Rey, Juan-Jose, additional, Ibnsalih, Walid, additional, Illuminati, Giulia, additional, Jansweijer, Peter, additional, Jung, Bouke, additional, Kalaczyński, Piotr, additional, Kalekin, Oleg, additional, Katz, Uli, additional, Khatun, Amina, additional, Kistauri, Giorgi, additional, Kopper, Claudio, additional, Kouchner, Antoine, additional, Kueviakoe, Vincent, additional, Kulikovskiy, Vladimir, additional, Kvatadze, Ramaz, additional, Labalme, Marc, additional, Lahmann, Robert, additional, Larosa, Giuseppina, additional, Lastoria, Chiara, additional, Lazo, Alfonso, additional, Le Stum, Sebastien, additional, Lehaut, Grégory, additional, Leonora, Emanuele, additional, Lessing, Nadja, additional, Levi, Giuseppe, additional, Clark, Miles, additional, Litrico, Pietro, additional, Longhitano, Fabio, additional, Mańczak, Jerzy, additional, Majumdar, Jhilik, additional, Malerba, Leonardo, additional, Mamedov, Fadahat, additional, Manfreda, Alberto, additional, Marconi, Martina, additional, Margiotta, Annarita, additional, Marinelli, Antonio, additional, Markou, Christos, additional, Martin, Lilian, additional, Martínez-Mora, Juan, additional, Marzaioli, Fabio, additional, Mastrodicasa, Massimo, additional, Mastroianni, Stefano, additional, Miccichè, Sandra, additional, Miele, Gennaro, additional, Migliozzi, Pasquale, additional, Migneco, Emilio, additional, Minutoli, Saverio, additional, Mitsou, Maria, additional, Mollo, Carlos, additional, Gallegos, Lizeth, additional, Morga, Michele, additional, Moussa, Abdelilah, additional, Mateo, Ivan, additional, Muller, Rasa, additional, Musico, Paolo, additional, Musone, Maria, additional, Musumeci, Mario, additional, Navas, Sergio, additional, Nayerhoda, Amid, additional, Nicolau, Carlo, additional, Nkosi, Bhuti, additional, Fearraigh, Brían, additional, Oliviero, Veronica, additional, Orlando, Angelo, additional, Oukacha, Enzo, additional, Paesani, Daniele, additional, González, Juan, additional, Papalashvili, Gogita, additional, Parisi, Vittorio, additional, Pastor, Emilio, additional, Paun, Alice, additional, Pavalas, Gabriela, additional, Pellegrini, Giuliano, additional, Martinez, Santiago, additional, Perrin-Terrin, Mathieu, additional, Perronnel, Jerome, additional, Pestel, Valentin, additional, Pestes, Rebekah, additional, Piattelli, Paolo, additional, Poirè, Chiara, additional, Popa, Vlad, additional, Pradier, Thierry, additional, Prado, Jorge, additional, Pulvirenti, Sara, additional, Quemener, Gilles, additional, Quiroz, Carlos, additional, Rahaman, Ushak, additional, Randazzo, Nunzio, additional, Randriatoamanana, Richard, additional, Razzaque, Soebur, additional, Rea, Immacolata, additional, Real, Diego, additional, Riccobene, Giorgio, additional, Robinson, Joshua, additional, Romanov, Andrey, additional, Saina, Adrian, additional, Greus, Francisco, additional, Samtleben, Dorothea, additional, Losa, Agustín, additional, Sanfilippo, Simone, additional, Sanguineti, Matteo, additional, Santonastaso, Claudio, additional, Santonocito, Domenico, additional, Sapienza, Piera, additional, Schmelling, Jan-Willem, additional, Schnabel, Jutta, additional, Schumann, Johannes, additional, Schutte, Hester, additional, Seneca, Jordan, additional, Sennan, Nour-Eddine, additional, Setter, Bastian, additional, Sgura, Irene, additional, Shanidze, Rezo, additional, Sharma, Ankur, additional, Shitov, Yury, additional, Šimkovic, Fedor, additional, Simonelli, Andreino, additional, Sinopoulou, Anna, additional, Smirnov, Mikhail, additional, Spisso, Bernardino, additional, Spurio, Maurizio, additional, Stavropoulos, Dimitris, additional, Štekl, Ivan, additional, Taiuti, Mauro, additional, Tayalati, Yahya, additional, Thiersen, Hannes, additional, Melo, Iara, additional, Tragia, Efi, additional, Trocme, Benjamin, additional, Tsourapis, Vasileios, additional, Tzamariudaki, Ekaterini, additional, Vacheret, Antonin, additional, Melchor, Angel, additional, Valsecchi, Veronica, additional, van Beveren, Vincent, additional, van Eeden, Thijs, additional, van Eijk, Daan, additional, Van Elewyck, Véronique, additional, van Haren, Hans, additional, Vannoye, Godefroy, additional, Vasileiadis, George, additional, De Sola, Francisco, additional, Verilhac, Cedric, additional, Veutro, Alessandro, additional, Viola, Salvatore, additional, Vivolo, Daniele, additional, Wilms, Joern, additional, Ramirez, Harold, additional, Zarpapis, Giorgos, additional, Zavatarelli, Sandra, additional, Zegarelli, Angela, additional, Zito, Daniele, additional, de Dios Zornoza, Juan, additional, Zuñiga, Juan, additional, and Zywucka, Natalia, additional
Published: 2024
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13. Spectroscopic identification of INTEGRAL high-energy sources with VLT/ISAAC

Author: Fortin, Francis, Chaty, Sylvain, Coleiro, Alexis, Tomsick, John, and Nitschelm, Christian
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics
Abstract: The INTEGRAL satellite has been observing the gamma-ray sky for 15 years and has detected over 900 X-ray sources of various nature. However, more than 200 of these sources still lack precise identification. Our goal is to reveal the nature of the high-energy sources detected by INTEGRAL. In particular, we want to improve the census of X-ray binaries. Photometry and spectroscopy were performed in July 2012 on 14 INTEGRAL sources in near-infrared at the Very Large Telescope on the European Southern Observatory-UT3 telescope equipped with the ISAAC spectrograph. We used K$_s$ images reaching to a depth of magnitude 18.5 to look for unique counterparts to high-energy detections to check for both extended sources and photometric variability. The analysis of near-infrared spectral features allows us to constrain the nature of these X-ray sources by comparing them to stellar spectra atlases. We present photometric and/or spectroscopic data for 14 sources (IGR J00465$-$4005, IGR J10447$-$6027, IGR J12489$-$6243, IGR J13020$-$6359, IGR J13186$-$6257, IGR J15293$-$5609, IGR J17200$-$3116, IGR J17404$-$3655, IGR J17586$-$2129, IGR J17597$-$2201, IGR J18457+0244, IGR J18532+0416, IGR J19308$+$0530, and IGR J19378$-$0617). We conclude that 5 of these are active galactic nuclei, 5 are cataclysmic variables, 2 are low- or intermediate-mass X-ray binaries, and 2 are Be high-mass X-ray binaries., Comment: 15 pages
Published: 2018
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14. Prospects for realtime characterization of core-collapse supernova and neutrino properties

Author: Bendahman, Meriem, primary, Goos, Isabel, additional, Coelho, Joao A.B., additional, Bugli, Matteo, additional, Coleiro, Alexis, additional, El Hedri, Sonia, additional, Foglizzo, Thierry, additional, Franco, Davide, additional, Guilet, Jérôme, additional, Kouchner, Antoine, additional, Raynaud, Raphaël, additional, and Tayalati, Yahya, additional
Published: 2024
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15. Multiwavelength study of the fast rotating supergiant high-mass X-ray binary IGR J16465-4507

Author: Chaty, Sylvain, LeReun, Audrey, Negueruela, Ignacio, Coleiro, Alexis, Castro, Norberto, Simon-Diaz, Sergio, Heras, Juan Antonio Zurita, Goldoni, Paolo, and Goldwurm, Andrea
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics
Abstract: Since its launch, the X-ray and gamma-ray observatory INTEGRAL satellite has revealed a new class of high-mass X-ray binaries (HMXB) displaying fast flares and hosting supergiant companion stars. Optical and infrared (OIR) observations in a multi-wavelength context are essential to understand the nature and evolution of these newly discovered celestial objects. The goal of this multiwavelength study (from ultraviolet to infrared) is to characterise the properties of IGR J16465-4507, to confirm its HMXB nature and that it hosts a supergiant star. We analysed all OIR, photometric and spectroscopic observations taken on this source, carried out at ESO facilities. Using spectroscopic data, we constrained the spectral type of the companion star between B0.5 and B1 Ib, settling the debate on the true nature of this source. We measured a high rotation velocity of v = 320 +/- 8 km/s from fitting absorption and emission lines in a stellar spectral model. We then built a spectral energy distribution from photometric observations to evaluate the origin of the different components radiating at each energy range. We finally show that, having accurately determined the spectral type of the early-B supergiant in IGR J16465-4507, we firmly support its classification as an intermediate supergiant fast X-ray transient (SFXT)., Comment: A&A in press, 14 pages, 15 tables, 13 figures
Published: 2016
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16. Multi-messenger astronomy with INTEGRAL

Author: Ferrigno, Carlo, Savchenko, Volodymyr, Coleiro, Alexis, Panessa, Francesca, Bazzano, Angela, Bozzo, Enrico, Chenevez, Jérôme, Domingo, Albert, Doyle, Maeve, Goldwurm, Andrea, Götz, Diego, Jourdain, Elisabeth, von Kienlin, Andreas, Kuulkers, Erik, Mereghetti, Sandro, Martin-Carrillo, Antonio, Natalucci, Lorenzo, Onori, Francesca, Rodi, James, Roques, Jean-Pierre, Sánchez-Fernández, Celia, and Ubertini, Pietro
Published: 2021
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17. Herschel observations of dust around the high-mass X-ray binary GX 301-2

Author: Servillat, Mathieu, Coleiro, Alexis, Chaty, Sylvain, Rahoui, Farid, and Heras, Juan Antonio Zurita
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract: We aim at characterising the structure of the gas and dust around the high mass X-ray binary GX 301-2, a highly obscured X-ray binary hosting a hypergiant star and a neutron star, in order to better constrain its evolution. We used Herschel PACS to observe GX 301-2 in the far infrared and completed the spectral energy distribution of the source using published data or catalogs, from the optical to the radio range (0.4 to 4x10^4 micrometer). GX 301-2 is detected for the first time at 70 and 100 micrometer. We fitted different models of circumstellar environments to the data. All tested models are statistically acceptable, and consistent with a hypergiant star at ~3 kpc. We found that the addition of a free-free emission component from the strong stellar wind is required and could dominate the far infrared flux. Through comparisons with similar systems and discussion on the estimated model parameters, we favour a disk-like circumstellar environment of ~8 AU that would enshroud the binary system. The temperature goes down to ~200 K at the edge of the disk, allowing for dust formation. This disk is probably a rimmed viscous disk with an inner rim at the temperature of the dust sublimation temperature (~1500 K). The similarities between the hypergiant GX 301-2, B[e] supergiants and the highly obscured X-ray binaries (in particular IGR J16318-4848) are strengthened. GX 301-2 might represent a transition stage in the evolution of massive stars in binary systems, connecting supergiant B[e] systems to luminous blue variables., Comment: accepted for publication in ApJ (tentatively scheduled for the December 1, 2014, V796 - 2 issue), 15 pages with emulateapj style
Published: 2014
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18. Exploiting synergies between neutrino telescopes for the next galactic core-collapse supernova

Author: Bendahman Meriem, Buellet Anne-Cécile, Bugli Matteo, Coelho Joao, Coleiro Alexis, de Wasseige Gwenhaël, El Hedri Sonia, Foglizzo Thierry, Franco Davide, Goos Isabel, Guilet Jérôme, Kouchner Antoine, Tayalati Yahya, Tonazzo Alessandra, and Volpe Cristina
Subjects: Physics, QC1-999
Abstract: Observing and characterizing the next galactic core-collapse supernova will be a critical step for neutrino experiments. Extracting information about the supernova progenitors and neutrino properties within minutes after an observation will in particular be crucial in order to optimize analysis strategies at other observatories. Moreover, certain classes of progenitors, with strong magnetic ﬁelds, could give rise to gamma-ray bursts but have been underinvestigated to date. In this contribution we propose a strategy to combine results from next-generation neutrino experiments, focusing notably on the determination of the progenitor mass and the neutrino mass ordering. Additionally, we investigate the impact of strong magnetic ﬁelds on neutrino observations, and demonstrate the detectability of the associated eﬀects in upcoming experiments.
Published: 2023
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19. Infrared identification of high-mass X-ray binaries discovered by INTEGRAL

Author: Coleiro, Alexis, Chaty, Sylvain, Heras, Juan A. Zurita, Rahoui, Farid, and Tomsick, John A.
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics
Abstract: Since it started observing the sky, the INTEGRAL satellite has discovered new categories of high mass X-ray binaries (HMXB) in our Galaxy. These observations raise important questions on the formation and evolution of these rare and short-lived objects. We present here new infrared observations from which to reveal or constrain the nature of 15 INTEGRAL sources, which allow us to update and discuss the Galactic HMXB population statistics. After previous photometric and spectroscopic observing campaigns in the optical and near-infrared, new photometry and spectroscopy was performed in the near-infrared with the SofI instrument on the ESO/NTT telescope in 2008 and 2010 on a sample of INTEGRAL sources. These observations, and specifically the detection of certain features in the spectra, allow the identification of these high-energy objects by comparison with published nIR spectral atlases of O and B stars. We present photometric data of nine sources (IGR J10101-5654, IGR J11187-5438, IGR J11435-6109, IGR J14331-6112, IGR J16328-4726, IGR J17200-3116, IGR J17354-3255, IGR J17404-3655, and IGR J17586-2129) and spectroscopic observations of 13 sources (IGR J10101-5654, IGR J11435-6109, IGR J13020-6359, IGR J14331-6112, IGR J14488-5942, IGR J16195-4945, IGR J16318-4848, IGR J16320-4751, IGR J16328-4726, IGR J16418-4532, IGR J17354-3255, IGR J17404-3655, and IGR J17586-2129). Our spectroscopic measurements indicate that: five of these objects are Oe/Be high-mass X-ray binaries (BeHMXB), six are supergiant high-mass X-ray binaries (sgHMXB), and two are sgB[e]. From a statistical point of view, we estimate the proportion of confirmed sgHMXB to be 42% and that of the confirmed BeHMXB to be 49%. The remaining 9% are peculiar HMXB., Comment: Accepted for publication in A&A (in press)
Published: 2013
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20. Herschel observations of INTEGRAL supergiant High Mass X-ray Binaries

Author: Chaty, Sylvain, Coleiro, Alexis, Servillat, Mathieu, Heras, Juan Antonio Zurita, and Rahoui, Farid
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics
Abstract: We present preliminary results on Herschel/PACS mid/far-infrared photometric observations of INTEGRAL supergiant High Mass X-ray Binaries (HMXBs), with the aim of detecting the presence and characterizing the nature of absorbing material (dust and/or cold gas), either enshrouding the whole binary systems, or surrounding the sources within their close environment. These unique observations allow us to better characterize the nature of these HMXBs, to constrain the link with their environment (impact and feedback), and finally to get a better understanding of the formation and evolution of such rare and short-living supergiant HMXBs in our Galaxy., Comment: Proceedings of the 9th INTEGRAL Workshop and celebration of the 10th anniversary of the launch "An INTEGRAL view of the high-energy sky (the first 10 years)", accepted for publication in Proceedings of Science (editors: F. Lebrun, A. Goldwurm and C. Winkler), 4 pages, 2 figures
Published: 2013

21. Herschel views on ultra-luminous X-ray sources

Author: Servillat, Mathieu, Coleiro, Alexis, and Chaty, Sylvain
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Galaxy Astrophysics
Abstract: The nature of ultra-luminous X-ray sources (ULXs), which are off-nuclear extragalactic X-ray sources that exceed the Eddington luminosity for a stellar-mass black hole, is still largely unknown. They might be black hole X-ray binaries in a super-Eddington accretion state, possibly with significant beaming of their emission, or they might harbor a black hole of intermediate mass (10^2 to 10^5 solar masses). Due to the enormous amount of energy radiated, ULXs can have strong interactions with their environment, particularly if the emission is not beamed and if they host a massive black hole. We present early results of a project that uses archival Herschel infrared observations of galaxies hosting bright ULXs in order to constrain the nature of the environment surrounding the ULXs and possible interactions. We already observe a spatial correlation between ULXs and dense clouds of cold material, that will be quantified in subsequent work. Those observations will allow us to test the similarities with the environment of Galactic high mass X-ray binaries. This project will also shed light on the nature of the host galaxies, and the possible factors that could favor the presence of a ULX in a galaxy., Comment: Accepted for publication in Proceedings of Science (INTEGRAL 2012), Eds. A. Goldwurm, F. Lebrun and C. Winkler, based on a presentation at the 9th INTEGRAL Workshop, October 15-19, 2012, Paris, France
Published: 2013

22. Distribution of High-Mass X-ray Binaries in the Milky Way

Author: Coleiro, Alexis and Chaty, Sylvain
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Galaxy Astrophysics, Astrophysics - Solar and Stellar Astrophysics
Abstract: Observations of the high energy sky, particularly with the INTEGRAL satellite, have quadrupled the number of supergiant X-ray Binaries observed in the Galaxy, and revealed new populations of previously hidden High Mass X-ray Binaries (HMXBs), raising new questions about their formation and evolution. The number of detected HMXBs of different types is now high enough to allow us to carry out a statistical analysis of their distribution in the Milky Way. For the first time, we derive the distance and absorption of a sample of HMXBs using a Spectral Energy Distribution fitting procedure, and we examine the correlation with the distribution of Star Forming Complexes (SFCs) in the Galaxy. We show that HMXBs are clustered with SFCs with a typical cluster size of 0.3 +/- 0.05 kpc and a characteristic distance between clusters of 1.7 +/- 0.3 kpc. Furthermore, we present an investigation of the expected offset between the position of spiral arms and HMXBs, allowing us to constrain age and migration distance due to supernova kick for 13 sources. These new methods will allow us to assess the influence of the environment on these high energy objects with unprecedented reliability., Comment: To appear in ApJ, 2013 February 20, vol. 764-2:185; 13 figures, 4 tables
Published: 2012
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23. Distribution of High Mass X-ray Binaries in the Milky Way

Author: Coleiro, Alexis and Chaty, Sylvain
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Galaxy Astrophysics
Abstract: The INTEGRAL satellite, observing the sky at high energy, has quadrupled the number of supergiant X-ray Binaries known in the Galaxy and has revealed new populations of previously hidden High Mass X-ray Binaries. These observations raise new questions about the formation and evolution of these sources. The number of detected sources is now high enough to allow us to carry out a statistical analysis of the distribution of HMXBs in the Milky Way. We derive the distance of each HMXB using a Spectral Energy Distribution fitting procedure, and we examine the correlation with the distribution of star forming complexes (SFCs) in the Galaxy. We show that HMXBs are clustered with SFCs, with a typical size of 0.3 kpc and a characteristic distance between clusters of 1.7 kpc., Comment: 7 pages, 7 figures. Proceedings of ESO workshop "Evolution of Compact Binaries", Vina del Mar (Chile), March 2011
Published: 2011

24. Core-collapse supernovae: from “nu” physics to new physics

Author: Bendahman, Meriem, primary, Barrère, Paul, additional, Buellet, Anne-Cécile, additional, Bugli, Matteo, additional, Coelho, Joao, additional, Coleiro, Alexis, additional, de Wasseige, Gwenhaël, additional, El Hedri, Sonia, additional, Foglizzo, Thierry, additional, Franco, Davide, additional, Goos, Isabel, additional, Guilet, Jérôme, additional, Kouchner, Antoine, additional, Raynaud, Raphaël, additional, and Tayalati, Yahya, additional
Published: 2023
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25. Deciphering the physical properties of the engines of neutrino-emitter blazars

Author: Azzollini, Alessandra, primary, Buson, Sara, additional, Coleiro, Alexis, additional, Fichet de Clairfontaine, Gaëtan, additional, Baghmanyan, Vardan, additional, Pfeiffer, Leonard, additional, Oswald, Lenz, additional, Barbano, Eleonora, additional, Marchesi, Stefano, additional, and Tramacere, Andrea, additional
Published: 2023
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26. The Athena X-ray Integral Field Unit: a consolidated design for the system requirement review of the preliminary definition phase

Author: Universidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Universidad de Alicante. Instituto Universitario de Física Aplicada a las Ciencias y las Tecnologías, Barret, Didier, Albouys, Vincent, den Herder, Jan-Willem, Piro, Luigi, Cappi, Massimo, Huovelin, Juhani, Kelley, Richard, Mas-Hesse, J. Miguel, Paltani, Stéphane, Rauw, Gregor, Rozanska, Agata, Bernard, Vivian, Berrocal, Alicia, Audard, Marc, Blin, Sylvie, Bonino, Donata, Frericks, Martin, Bonnet, François, Bonny, Patrick, Boorman, Peter, Ptak, Andy, Chaoul, Laurence, Boreux, Charles, Bounab, Ayoub, Boutelier, Martin, Boyce, Kevin, Brienza, Daniele, Bandler, Simon, Bruijn, Marcel, Gabici, Stefano, Bulgarelli, Andrea, Calarco, Simona, Raulin, Desi, Gloaguen, Emilie, Callanan, Paul, Prada Campello, Alberto, Camus, Thierry, Canourgues, Florent, Capobianco, Vito, Cardiel, Nicolas, Castellani, Florent, Barbera, Marco, Gant, Florent, Simionescu, Aurora, Cheatom, Oscar, Doumayrou, Eric, Chervenak, James, Chiarello, Fabio, Clerc, Laurent, Clerc, Nicolas, Cobo, Beatriz, Coeur-Joly, Odile, Coleiro, Alexis, Colonges, Stéphane, Torrejon, Jose M., Corcione, Leonardo, Gao, Jian-Rong, Puccetti, Simonetta, Barcons, Xavier, Coriat, Mickael, Coynel, Alexandre, Cuttaia, Francesco, D’Ai, Antonino, D’anca, Fabio, Dadina, Mauro, Acero, Fabio, Daniel, Christophe, Dauner, Lea, DeNigris, Natalie, Puccio, Elena, Gastaldello, Fabio, Dercksen, Johannes, Bozzo, Enrico, DiPirro, Michael, Genolet, Ludovic, Durkin, Malcom, van Leeuwen, Bert-Joost, Charles, Ivan, Ghizzardi, Simona, Alcacera Gil, M. Angeles, Giovannini, Elisa, Ramon, Pascale, Godet, Olivier, Gomez-Elvira, Javier, Gonzalez, Raoul, Gonzalez, Manuel, Gottardi, Luciano, Branduardi-Raymont, Graziella, Granat, Dolorès, Fioretti, Valentina, Gros, Michel, Costantini, Elisa, Guignard, Nicolas, Reina, Manuel, Hieltjes, Paul, Hurtado, Adolfo Jesús, Irwin, Kent, Jacquey, Christian, Ettori, Stefano, Janiuk, Agnieszka, Jaubert, Jean, Jiménez, Maria, Geoffray, Hervé, Jolly, Antoine, Jourdan, Thierry, Rioland, Guillaume, Dauser, Thomas, Julien, Sabine, Kedziora, Bartosz, Finoguenov, Alexis, Korb, Andrew, Kreykenbohm, Ingo, König, Ole, Langer, Mathieu, Laudet, Philippe, Jacques, Lionel, Laurent, Philippe, Rodriguez, Louis, Laurenza, Monica, Lesrel, Jean, Etcheverry, Christophe, Decourchelle, Anne, Ligori, Sebastiano, Lorenz, Maximilian, Luminari, Alfredo, Maffei, Bruno, Maisonnave, Océane, Marelli, Lorenzo, Kirsch, Christian, Roig, Anton, Massonet, Didier, Petit, Pascal, Maussang, Irwin, Melchor, Alejandro Gonzalo, Le Mer, Isabelle, Duband, Lionel, San Millan, Francisco Javier, Millerioux, Jean-Pierre, Mineo, Teresa, Minervini, Gabriele, Molin, Alexeï, Gatti, Flavio, Grosso, Nicolas, Smith, Stephen, Monestes, David, Montinaro, Nicola, Mot, Baptiste, Murat, David, Nagayoshi, Kenichiro, Duval, Jean-Marc, Nazé, Yaël, Noguès, Loïc, Pailot, Damien, Kaastra, Jelle, Rollet, Bertrand, Panessa, Francesca, Adams, Joseph, Parodi, Luigi, Roncarelli, Mauro, Dubbeldam, Luc, Hoogeveen, Ruud, Roudil, Gilles, Rudnicki, Tomasz, Sanisidro, Julien, Mazzotta, Pasquale, Sciortino, Luisa, Silva, Vitor, Sordet, Michael, Soto-Aguilar, Javier, Spizzi, Pierre, Goldwurm, Andrea, Dupieux, Michel, Surace, Christian, Svoboda, Jiri, Fernández Sánchez, Miguel, Miller, Jon, Taralli, Emanuele, Terrasa, Guilhem, Terrier, Régis, Todaro, Michela, Ubertini, Pietro, Uslenghi, Michela, Vaate, Jan Geralt Bijd de, Dupourqué, Simon, Vaccaro, Davide, den Hartog, Roland, Miniutti, Giovanni, van der Hulst, Paul, Varisco, Salvatore, Varnière, Peggy, Vibert, Laurent, Vidriales, María, Villa, Fabrizio, Vodopivec, Boris Martin, Volpe, Angela, Durand, Jean Louis, Vries, Cor de, Nicastro, Fabrizio, Wakeham, Nicholas, Walmsley, Gavin, Kiviranta, Mikko, Jackson, Brian, Wise, Michael, Wit, Martin de, Woźniak, Grzegorz, Jonker, Peter, Kilbourne, Caroline, Eckert, Dominique, Sciortino, Salvatore, Korpela, Seppo, Macculi, Claudio, Mendez, Mariano, Mitsuda, Kazuhisa, van der Kuur, Jan, Molendi, Silvano, Pajot, François, Pointecouteau, Etienne, Porter, Frederick, Pratt, Gabriel W., van Loon, Dennis, Eiriz, Valvanera, Prêle, Damien, Ravera, Laurent, Sato, Kosuke, Schaye, Joop, Shinozaki, Keisuke, Ledot, Aurélien, Skup, Konrad, Soucek, Jan, Thibert, Tanguy, Yamaguchi, Hiroya, Vink, Jacco, Ercolani, Eric, Webb, Natalie, Beaumont, Sophie, Piconcelli, Enrico, Ceballos, Maria Teresa, Cucchetti, Edoardo, D’Andrea, Matteo, Eckart, Megan, Ferrando, Philippe, Kammoun, Elias, Lotti, Simone, Mesnager, Jean-Michel, Natalucci, Lorenzo, Lyautey, Bertrand, Pinto, Ciro, Peille, Philippe, Doriese, William, de Plaa, Jelle, Ardellier, Florence, Argan, Andrea, Bellouard, Elise, Carron, Jérôme, Cavazzuti, Elisabetta, Fiorini, Mauro, Khosropanah, Pourya, Encinas Plaza, Jose Miguel, Martin, Sylvain, Parot, Yann, Finkbeiner, Fred, Perry, James, Pinsard, Frederic, Pradines, Alice, Rigano, Manuela, Roelfsema, Peter, Schwander, Denis, Torrioli, Guido, Plaza, Borja, Ullom, Joel, Vera, Isabel, Medinaceli Villegas, Eduardo, Fiocchi, Mariateresa, Sakai, Kazuhiro, Zuchniak, Monika, Brachet, Frank, Lo Cicero, Ugo, van Weers, Henk, Wilms, Joern, Fiore, Fabrizio, Abdoelkariem, Shariefa, Adam, Thomas, Adami, Christophe, Aicardi, Corinne, Fossecave, Hervé, Akamatsu, Hiroki, Merino Alonso, Pablo Eleazar, Amato, Roberta, André, Jérôme, Angelinelli, Matteo, Poyatos, David, Anon-Cancela, Manuel, Yamasaki, Noriko, Anvar, Shebli, Atienza, Ricardo, Attard, Anthony, Franssen, Philippe, Auricchio, Natalia, Balado, Ana, Bancel, Florian, Barusso, Lorenzo Ferrari, Prouvé, Thomas, Bascuñan, Arturo, Universidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Universidad de Alicante. Instituto Universitario de Física Aplicada a las Ciencias y las Tecnologías, Barret, Didier, Albouys, Vincent, den Herder, Jan-Willem, Piro, Luigi, Cappi, Massimo, Huovelin, Juhani, Kelley, Richard, Mas-Hesse, J. Miguel, Paltani, Stéphane, Rauw, Gregor, Rozanska, Agata, Bernard, Vivian, Berrocal, Alicia, Audard, Marc, Blin, Sylvie, Bonino, Donata, Frericks, Martin, Bonnet, François, Bonny, Patrick, Boorman, Peter, Ptak, Andy, Chaoul, Laurence, Boreux, Charles, Bounab, Ayoub, Boutelier, Martin, Boyce, Kevin, Brienza, Daniele, Bandler, Simon, Bruijn, Marcel, Gabici, Stefano, Bulgarelli, Andrea, Calarco, Simona, Raulin, Desi, Gloaguen, Emilie, Callanan, Paul, Prada Campello, Alberto, Camus, Thierry, Canourgues, Florent, Capobianco, Vito, Cardiel, Nicolas, Castellani, Florent, Barbera, Marco, Gant, Florent, Simionescu, Aurora, Cheatom, Oscar, Doumayrou, Eric, Chervenak, James, Chiarello, Fabio, Clerc, Laurent, Clerc, Nicolas, Cobo, Beatriz, Coeur-Joly, Odile, Coleiro, Alexis, Colonges, Stéphane, Torrejon, Jose M., Corcione, Leonardo, Gao, Jian-Rong, Puccetti, Simonetta, Barcons, Xavier, Coriat, Mickael, Coynel, Alexandre, Cuttaia, Francesco, D’Ai, Antonino, D’anca, Fabio, Dadina, Mauro, Acero, Fabio, Daniel, Christophe, Dauner, Lea, DeNigris, Natalie, Puccio, Elena, Gastaldello, Fabio, Dercksen, Johannes, Bozzo, Enrico, DiPirro, Michael, Genolet, Ludovic, Durkin, Malcom, van Leeuwen, Bert-Joost, Charles, Ivan, Ghizzardi, Simona, Alcacera Gil, M. Angeles, Giovannini, Elisa, Ramon, Pascale, Godet, Olivier, Gomez-Elvira, Javier, Gonzalez, Raoul, Gonzalez, Manuel, Gottardi, Luciano, Branduardi-Raymont, Graziella, Granat, Dolorès, Fioretti, Valentina, Gros, Michel, Costantini, Elisa, Guignard, Nicolas, Reina, Manuel, Hieltjes, Paul, Hurtado, Adolfo Jesús, Irwin, Kent, Jacquey, Christian, Ettori, Stefano, Janiuk, Agnieszka, Jaubert, Jean, Jiménez, Maria, Geoffray, Hervé, Jolly, Antoine, Jourdan, Thierry, Rioland, Guillaume, Dauser, Thomas, Julien, Sabine, Kedziora, Bartosz, Finoguenov, Alexis, Korb, Andrew, Kreykenbohm, Ingo, König, Ole, Langer, Mathieu, Laudet, Philippe, Jacques, Lionel, Laurent, Philippe, Rodriguez, Louis, Laurenza, Monica, Lesrel, Jean, Etcheverry, Christophe, Decourchelle, Anne, Ligori, Sebastiano, Lorenz, Maximilian, Luminari, Alfredo, Maffei, Bruno, Maisonnave, Océane, Marelli, Lorenzo, Kirsch, Christian, Roig, Anton, Massonet, Didier, Petit, Pascal, Maussang, Irwin, Melchor, Alejandro Gonzalo, Le Mer, Isabelle, Duband, Lionel, San Millan, Francisco Javier, Millerioux, Jean-Pierre, Mineo, Teresa, Minervini, Gabriele, Molin, Alexeï, Gatti, Flavio, Grosso, Nicolas, Smith, Stephen, Monestes, David, Montinaro, Nicola, Mot, Baptiste, Murat, David, Nagayoshi, Kenichiro, Duval, Jean-Marc, Nazé, Yaël, Noguès, Loïc, Pailot, Damien, Kaastra, Jelle, Rollet, Bertrand, Panessa, Francesca, Adams, Joseph, Parodi, Luigi, Roncarelli, Mauro, Dubbeldam, Luc, Hoogeveen, Ruud, Roudil, Gilles, Rudnicki, Tomasz, Sanisidro, Julien, Mazzotta, Pasquale, Sciortino, Luisa, Silva, Vitor, Sordet, Michael, Soto-Aguilar, Javier, Spizzi, Pierre, Goldwurm, Andrea, Dupieux, Michel, Surace, Christian, Svoboda, Jiri, Fernández Sánchez, Miguel, Miller, Jon, Taralli, Emanuele, Terrasa, Guilhem, Terrier, Régis, Todaro, Michela, Ubertini, Pietro, Uslenghi, Michela, Vaate, Jan Geralt Bijd de, Dupourqué, Simon, Vaccaro, Davide, den Hartog, Roland, Miniutti, Giovanni, van der Hulst, Paul, Varisco, Salvatore, Varnière, Peggy, Vibert, Laurent, Vidriales, María, Villa, Fabrizio, Vodopivec, Boris Martin, Volpe, Angela, Durand, Jean Louis, Vries, Cor de, Nicastro, Fabrizio, Wakeham, Nicholas, Walmsley, Gavin, Kiviranta, Mikko, Jackson, Brian, Wise, Michael, Wit, Martin de, Woźniak, Grzegorz, Jonker, Peter, Kilbourne, Caroline, Eckert, Dominique, Sciortino, Salvatore, Korpela, Seppo, Macculi, Claudio, Mendez, Mariano, Mitsuda, Kazuhisa, van der Kuur, Jan, Molendi, Silvano, Pajot, François, Pointecouteau, Etienne, Porter, Frederick, Pratt, Gabriel W., van Loon, Dennis, Eiriz, Valvanera, Prêle, Damien, Ravera, Laurent, Sato, Kosuke, Schaye, Joop, Shinozaki, Keisuke, Ledot, Aurélien, Skup, Konrad, Soucek, Jan, Thibert, Tanguy, Yamaguchi, Hiroya, Vink, Jacco, Ercolani, Eric, Webb, Natalie, Beaumont, Sophie, Piconcelli, Enrico, Ceballos, Maria Teresa, Cucchetti, Edoardo, D’Andrea, Matteo, Eckart, Megan, Ferrando, Philippe, Kammoun, Elias, Lotti, Simone, Mesnager, Jean-Michel, Natalucci, Lorenzo, Lyautey, Bertrand, Pinto, Ciro, Peille, Philippe, Doriese, William, de Plaa, Jelle, Ardellier, Florence, Argan, Andrea, Bellouard, Elise, Carron, Jérôme, Cavazzuti, Elisabetta, Fiorini, Mauro, Khosropanah, Pourya, Encinas Plaza, Jose Miguel, Martin, Sylvain, Parot, Yann, Finkbeiner, Fred, Perry, James, Pinsard, Frederic, Pradines, Alice, Rigano, Manuela, Roelfsema, Peter, Schwander, Denis, Torrioli, Guido, Plaza, Borja, Ullom, Joel, Vera, Isabel, Medinaceli Villegas, Eduardo, Fiocchi, Mariateresa, Sakai, Kazuhiro, Zuchniak, Monika, Brachet, Frank, Lo Cicero, Ugo, van Weers, Henk, Wilms, Joern, Fiore, Fabrizio, Abdoelkariem, Shariefa, Adam, Thomas, Adami, Christophe, Aicardi, Corinne, Fossecave, Hervé, Akamatsu, Hiroki, Merino Alonso, Pablo Eleazar, Amato, Roberta, André, Jérôme, Angelinelli, Matteo, Poyatos, David, Anon-Cancela, Manuel, Yamasaki, Noriko, Anvar, Shebli, Atienza, Ricardo, Attard, Anthony, Franssen, Philippe, Auricchio, Natalia, Balado, Ana, Bancel, Florian, Barusso, Lorenzo Ferrari, Prouvé, Thomas, and Bascuñan, Arturo
Abstract: The Athena X-ray Integral Unit (X-IFU) is the high resolution X-ray spectrometer studied since 2015 for flying in the mid-30s on the Athena space X-ray Observatory. Athena is a versatile observatory designed to address the Hot and Energetic Universe science theme, as selected in November 2013 by the Survey Science Committee. Based on a large format array of Transition Edge Sensors (TES), X-IFU aims to provide spatially resolved X-ray spectroscopy, with a spectral resolution of 2.5 eV (up to 7 keV) over a hexagonal field of view of 5 arc minutes (equivalent diameter). The X-IFU entered its System Requirement Review (SRR) in June 2022, at about the same time when ESA called for an overall X-IFU redesign (including the X-IFU cryostat and the cooling chain), due to an unanticipated cost overrun of Athena. In this paper, after illustrating the breakthrough capabilities of the X-IFU, we describe the instrument as presented at its SRR (i.e. in the course of its preliminary definition phase, so-called B1), browsing through all the subsystems and associated requirements. We then show the instrument budgets, with a particular emphasis on the anticipated budgets of some of its key performance parameters, such as the instrument efficiency, spectral resolution, energy scale knowledge, count rate capability, non X-ray background and target of opportunity efficiency. Finally, we briefly discuss the ongoing key technology demonstration activities, the calibration and the activities foreseen in the X-IFU Instrument Science Center, touch on communication and outreach activities, the consortium organisation and the life cycle assessment of X-IFU aiming at minimising the environmental footprint, associated with the development of the instrument. Thanks to the studies conducted so far on X-IFU, it is expected that along the design-to-cost exercise requested by ESA, the X-IFU will maintain flagship capabilities in spatially resolved high resolution X-ray spectroscopy, enabling most of th
Published: 2023

27. Gravitational waves or electromagnetic counterpart ? No need to choose

Author: Mignon-Risse, Raphaël, Varniere, Peggy, Casse, Fabien, and Coleiro, Alexis
Abstract: Binary black holes emit gravitational waves (GWs) as they inspiral towards coalescence. Searches for electromagnetic counterparts to GWs rely on looking for common sources producing both waves. Here, we take a different approach: we investigate the impact of the binary binary hole onto its outer circumbinary disk in the radiation/wavezone, using general relativistic hydrodynamical simulations and a general relativistic ray-tracing code. We show that in the radiation/wave zone, retardation effects and GWs leave an imprint onto the disk, leading to quasi-periodic patterns in the electromagnetic lightcurve.
Published: 2022
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28. Demonstrator model of the warm front-end electronics for the ATHENA mission's X-IFU instrument

Author: Gonzalez, Manuel, primary, Prêle, Damien, additional, Chen, Si, additional, Ardellier-Desages, Florence, additional, Givaudan, Alain, additional, Courty, Bernard, additional, Blin, Sylvie, additional, Oger, Ronan, additional, Monier, Guy, additional, Colognes, Stephane, additional, Pailot, Damien, additional, Coleiro, Alexis, additional, Varniere, Peggy, additional, and Goldwurm, Andrea, additional
Published: 2022
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29. SNEWPY: A Data Pipeline from Supernova Simulations to Neutrino Signals

Author: Baxter, Amanda L., BenZvi, Segev, Jaimes, Joahan Castaneda, Coleiro, Alexis, Molla, Marta Colomer, Dornic, Damien, Goldhagen, Tomer, Graf, Anne, Griswold, Spencer, Habig, Alec, Hill, Remington, Horiuchi, Shunsaku, Kneller, James P., Lang, Rafael F., Lincetto, Massimiliano, Migenda, Jost, Nakamura, Ko, O'Connor, Evan, Renshaw, Andrew, Scholberg, Kate, Tunnell, Christopher, Uberoi, Navya, Worlikar, Arkin, Baxter, Amanda L., BenZvi, Segev, Jaimes, Joahan Castaneda, Coleiro, Alexis, Molla, Marta Colomer, Dornic, Damien, Goldhagen, Tomer, Graf, Anne, Griswold, Spencer, Habig, Alec, Hill, Remington, Horiuchi, Shunsaku, Kneller, James P., Lang, Rafael F., Lincetto, Massimiliano, Migenda, Jost, Nakamura, Ko, O'Connor, Evan, Renshaw, Andrew, Scholberg, Kate, Tunnell, Christopher, Uberoi, Navya, and Worlikar, Arkin
Abstract: Current neutrino detectors will observe hundreds to thousands of neutrinos from Galactic supernovae, and future detectors will increase this yield by an order of magnitude or more. With such a data set comes the potential for a huge increase in our understanding of the explosions of massive stars, nuclear physics under extreme conditions, and the properties of the neutrino. However, there is currently a large gap between supernova simulations and the corresponding signals in neutrino detectors, which will make any comparison between theory and observation very difficult. SNEWPY is an open-source software package that bridges this gap. The SNEWPY code can interface with supernova simulation data to generate from the model either a time series of neutrino spectral fluences at Earth, or the total time-integrated spectral fluence. Data from several hundred simulations of core-collapse, thermonuclear, and pair-instability supernovae is included in the package. This output may then be used by an event generator such as sntools or an event rate calculator such as the SuperNova Observatories with General Long Baseline Experiment Simulator (SNOwGLoBES). Additional routines in the SNEWPY package automate the processing of the generated data through the SNOwGLoBES software and collate its output into the observable channels of each detector. In this paper we describe the contents of the package, the physics behind SNEWPY, the organization of the code, and provide examples of how to make use of its capabilities.
Published: 2022
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30. Collaborative experience between scientific software projects using Agile Scrum development

Author: Baxter, Amanda L., BenZvi, Segev Y., Bonivento, Walter, Brazier, Adam, Clark, Michael, Coleiro, Alexis, Collom, David, Colomer-Molla, Marta, Cousins, Bryce, Orellana, Aliwen Delgado, Dornic, Damien, Ekimtcov, Vladislav, ElSayed, Shereen, Rosso, Andrea Gallo, Godwin, Patrick, Griswold, Spencer, Habig, Alec, Hill, Remington, Horiuchi, Shunsaku, Howell, D. Andrew, Johnson, Margaret W. G., Kneller, James P., Kopec, Abigail, Kopper, Claudio, Kulikovskiy, Vladimir, Lamoureux, Mathieu, Lang, Rafael F., Li, Shengchao, Lincetto, Massimiliano, Lindstrom, Lindy, Linvill, Mark W., McCully, Curtis, Migenda, Jost, Milisavljevic, Danny, Nelson, Spencer, Novoseltseva, Rita, O'Sullivan, Erin, Petravick, Donald, Pointon, Barry W., Raj, Nirmal, Renshaw, Andrew, Rumleskie, Janet, Sonley, Tom, Tapia, Ron, Tseng, Jeffrey C. L., Tunnell, Christopher D., Vannoye, Godefroy, Vigorito, Carlo F., Virtue, Clarence J., Weaver, Christopher, Weil, Kathryn E., Winslow, Lindley, Wolski, Rich, Xu, Xun-Jie, Xu, Yiyang, Baxter, Amanda L., BenZvi, Segev Y., Bonivento, Walter, Brazier, Adam, Clark, Michael, Coleiro, Alexis, Collom, David, Colomer-Molla, Marta, Cousins, Bryce, Orellana, Aliwen Delgado, Dornic, Damien, Ekimtcov, Vladislav, ElSayed, Shereen, Rosso, Andrea Gallo, Godwin, Patrick, Griswold, Spencer, Habig, Alec, Hill, Remington, Horiuchi, Shunsaku, Howell, D. Andrew, Johnson, Margaret W. G., Kneller, James P., Kopec, Abigail, Kopper, Claudio, Kulikovskiy, Vladimir, Lamoureux, Mathieu, Lang, Rafael F., Li, Shengchao, Lincetto, Massimiliano, Lindstrom, Lindy, Linvill, Mark W., McCully, Curtis, Migenda, Jost, Milisavljevic, Danny, Nelson, Spencer, Novoseltseva, Rita, O'Sullivan, Erin, Petravick, Donald, Pointon, Barry W., Raj, Nirmal, Renshaw, Andrew, Rumleskie, Janet, Sonley, Tom, Tapia, Ron, Tseng, Jeffrey C. L., Tunnell, Christopher D., Vannoye, Godefroy, Vigorito, Carlo F., Virtue, Clarence J., Weaver, Christopher, Weil, Kathryn E., Winslow, Lindley, Wolski, Rich, Xu, Xun-Jie, and Xu, Yiyang
Abstract: Developing sustainable software for the scientific community requires expertise in software engineering and domain science. This can be challenging due to the unique needs of scientific software, the insufficient resources for software engineering practices in the scientific community, and the complexity of developing for evolving scientific contexts. While open-source software can partially address these concerns, it can introduce complicating dependencies and delay development. These issues can be reduced if scientists and software developers collaborate. We present a case study wherein scientists from the SuperNova Early Warning System collaborated with software developers from the Scalable Cyberinfrastructure for Multi-Messenger Astrophysics project. The collaboration addressed the difficulties of open-source software development, but presented additional risks to each team. For the scientists, there was a concern of relying on external systems and lacking control in the development process. For the developers, there was a risk in supporting a user-group while maintaining core development. These issues were mitigated by creating a second Agile Scrum framework in parallel with the developers' ongoing Agile Scrum process. This Agile collaboration promoted communication, ensured that the scientists had an active role in development, and allowed the developers to evaluate and implement the scientists' software requirements. The collaboration provided benefits for each group: the scientists actuated their development by using an existing platform, and the developers utilized the scientists' use-case to improve their systems. This case study suggests that scientists and software developers can avoid scientific computing issues by collaborating and that Agile Scrum methods can address emergent concerns.
Published: 2022
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31. Exploring the Potential of Multi-Detector Analyses for Core-Collapse Supernova Neutrino Detection

Author: Bendahman, Meriem, Bugli, Matteo, Coleiro, Alexis, Colomer Molla, Marta, De Wasseige, Gwenhaël, Foglizzo, Thierry, Kouchner, Antoine, Regnier, Mathias, Tayalati, Yahya, Tonazzo, Alessandra, Van Elewyck, Véronique, Bendahman, Meriem, Bugli, Matteo, Coleiro, Alexis, Colomer Molla, Marta, De Wasseige, Gwenhaël, Foglizzo, Thierry, Kouchner, Antoine, Regnier, Mathias, Tayalati, Yahya, Tonazzo, Alessandra, and Van Elewyck, Véronique
Abstract: The core-collapse supernova (CCSN) SN1987A has been the first extragalactic transient source observed with neutrinos, and the 25 events detected by the neutrino telescopes running at that time marked the beginning of neutrino astronomy. Despite hundreds of CCSNs detected in the electromagnetic spectrum since 1987, neutrino telescopes could not perform another observation due to the far distances of the sources. It is thus of primary importance to optimize the detection channel of sensitive detectors in anticipation of a forthcoming Galactic CCSN. Beyond being used as an early warning of a close-by CCSN, neutrinos can provide unique information on the explosion mechanism, and can be used to probe neutrino oscillation in dense environments. In this contribution, we present the potential of multi-detector analysis to enhance the scientific outputs from the next close-by CCSN. Combining the expected light curves in neutrino detectors sensitive to different flavors, we study the constraints that could be set on the properties of the progenitor itself, such as its mass, as well as on the neutrino oscillation parameters. We also present the results of a triangulation algorithm using a prior source map in the definition of the the region of interest., SCOPUS: cp.p, info:eu-repo/semantics/published
Published: 2022

32. SNEWPY: A Data Pipeline from Supernova Simulations to Neutrino Signals

Author: Baxter, Amanda A.L., Benzvi, Segev, Jaimes, Joahan Castaneda, Coleiro, Alexis, Colomer Molla, Marta, Dornic, Damien, Goldhagen, Tomer, Graf, Anne, Griswold, Spencer, Habig, Alec, Hill, Remington, Horiuchi, Shunsaku, Kneller, James J.P., Lang, Rafael R.F., Lincetto, Massimiliano, Migenda, Jost, Nakamura, Ko, O'Connor, Evan, Renshaw, Andrew, Scholberg, Kate, Tunnell, Christopher, Uberoi, Navya, Worlikar, Arkin, Baxter, Amanda A.L., Benzvi, Segev, Jaimes, Joahan Castaneda, Coleiro, Alexis, Colomer Molla, Marta, Dornic, Damien, Goldhagen, Tomer, Graf, Anne, Griswold, Spencer, Habig, Alec, Hill, Remington, Horiuchi, Shunsaku, Kneller, James J.P., Lang, Rafael R.F., Lincetto, Massimiliano, Migenda, Jost, Nakamura, Ko, O'Connor, Evan, Renshaw, Andrew, Scholberg, Kate, Tunnell, Christopher, Uberoi, Navya, and Worlikar, Arkin
Abstract: Current neutrino detectors will observe hundreds to thousands of neutrinos from Galactic supernovae, and future detectors will increase this yield by an order of magnitude or more. With such a data set comes the potential for a huge increase in our understanding of the explosions of massive stars, nuclear physics under extreme conditions, and the properties of the neutrino. However, there is currently a large gap between supernova simulations and the corresponding signals in neutrino detectors, which will make any comparison between theory and observation very difficult. SNEWPY is an open-source software package that bridges this gap. The SNEWPY code can interface with supernova simulation data to generate from the model either a time series of neutrino spectral fluences at Earth, or the total time-integrated spectral fluence. Data from several hundred simulations of core-collapse, thermonuclear, and pair-instability supernovae is included in the package. This output may then be used by an event generator such as sntools or an event rate calculator such as the SuperNova Observatories with General Long Baseline Experiment Simulator (SNOwGLoBES). Additional routines in the SNEWPY package automate the processing of the generated data through the SNOwGLoBES software and collate its output into the observable channels of each detector. In this paper we describe the contents of the package, the physics behind SNEWPY, the organization of the code, and provide examples of how to make use of its capabilities., SCOPUS: ar.j, info:eu-repo/semantics/published
Published: 2022

33. Athena synergies in the multi-messenger and transient universe

Author: Conferencia de Rectores de las Universidades Españolas, Consejo Superior de Investigaciones Científicas (España), European Commission, Ministerio de Ciencia, Innovación y Universidades (España), Agencia Estatal de Investigación (España), Piro, Luigi, Ahlers, Markus, Coleiro, Alexis, Colpi, Monica, Oña Wilhelmi, Emma de, Guainazzi, Matteo, Jonker, Peter G., Mc Namara, Paul, Nichols, David A., O'Brien, Paul, Troja, Eleonora, Vink, Jacco, Aird, James, Amati, Lorenzo, Anand, Shreya, Bozzo, Enrico, Carrera, Francisco J., Fabian, Andrew C., Fryer, Christopher, Hall, Evan, Korobkin, Oleg, Korol, Valeriya, Mangiagli, Alberto, Martínez-Núñez, Silvia, Nissanke, Samaya, Osborne, Julien, Padovani, Paolo, Rossi, Elena M., Ryan, Geoffrey, Sesana, Alberto, Stratta, Giulia, Tanvir, Niel, Eerten, Hendrik van, Conferencia de Rectores de las Universidades Españolas, Consejo Superior de Investigaciones Científicas (España), European Commission, Ministerio de Ciencia, Innovación y Universidades (España), Agencia Estatal de Investigación (España), Piro, Luigi, Ahlers, Markus, Coleiro, Alexis, Colpi, Monica, Oña Wilhelmi, Emma de, Guainazzi, Matteo, Jonker, Peter G., Mc Namara, Paul, Nichols, David A., O'Brien, Paul, Troja, Eleonora, Vink, Jacco, Aird, James, Amati, Lorenzo, Anand, Shreya, Bozzo, Enrico, Carrera, Francisco J., Fabian, Andrew C., Fryer, Christopher, Hall, Evan, Korobkin, Oleg, Korol, Valeriya, Mangiagli, Alberto, Martínez-Núñez, Silvia, Nissanke, Samaya, Osborne, Julien, Padovani, Paolo, Rossi, Elena M., Ryan, Geoffrey, Sesana, Alberto, Stratta, Giulia, Tanvir, Niel, and Eerten, Hendrik van
Abstract: In this paper we explore the scientific synergies between Athena and some of the key multi-messenger facilities that should be operative concurrently with Athena. These facilities include LIGO A+, Advanced Virgo+ and future detectors for ground-based observation of gravitational waves (GW), LISA for space-based observations of GW, IceCube and KM3NeT for neutrino observations, and CTA for very high energy observations. These science themes encompass pressing issues in astrophysics, cosmology and fundamental physics such as: the central engine and jet physics in compact binary mergers, accretion processes and jet physics in Super-Massive Binary Black Holes (SMBBHs) and in compact stellar binaries, the equation of state of neutron stars, cosmic accelerators and the origin of Cosmic Rays (CRs), the origin of intermediate and high-Z elements in the Universe, the Cosmic distance scale and tests of General Relativity and the Standard Model. Observational strategies for implementing the identified science topics are also discussed. A significant part of the sources targeted by multi-messenger facilities is of transient nature. We have thus also discussed the synergy of Athena with wide-field high-energy facilities, taking THESEUS as a case study for transient discovery. This discussion covers all the Athena science goals that rely on follow-up observations of high-energy transients identified by external observatories, and includes also topics that are not based on multi-messenger observations, such as the search for missing baryons or the observation of early star populations and metal enrichment at the cosmic dawn with Gamma-Ray Bursts (GRBs).
Published: 2022

34. Athena synergies in the multi-messenger and transient universe

Author: MIT Kavli Institute for Astrophysics and Space Research, Piro, Luigi, Ahlers, Markus, Coleiro, Alexis, Colpi, Monica, de Oña Wilhelmi, Emma, Guainazzi, Matteo, Jonker, Peter G., Namara, Paul M., Nichols, David A., O’Brien, Paul, Troja, Eleonora, Vink, Jacco, Aird, James, Amati, Lorenzo, Anand, Shreya, Bozzo, Enrico, MIT Kavli Institute for Astrophysics and Space Research, Piro, Luigi, Ahlers, Markus, Coleiro, Alexis, Colpi, Monica, de Oña Wilhelmi, Emma, Guainazzi, Matteo, Jonker, Peter G., Namara, Paul M., Nichols, David A., O’Brien, Paul, Troja, Eleonora, Vink, Jacco, Aird, James, Amati, Lorenzo, Anand, Shreya, and Bozzo, Enrico
Abstract: In this paper we explore the scientific synergies between Athena and some of the key multi-messenger facilities that should be operative concurrently with Athena. These facilities include LIGO A+, Advanced Virgo+ and future detectors for ground-based observation of gravitational waves (GW), LISA for space-based observations of GW, IceCube and KM3NeT for neutrino observations, and CTA for very high energy observations. These science themes encompass pressing issues in astrophysics, cosmology and fundamental physics such as: the central engine and jet physics in compact binary mergers, accretion processes and jet physics in Super-Massive Binary Black Holes (SMBBHs) and in compact stellar binaries, the equation of state of neutron stars, cosmic accelerators and the origin of Cosmic Rays (CRs), the origin of intermediate and high-Z elements in the Universe, the Cosmic distance scale and tests of General Relativity and the Standard Model. Observational strategies for implementing the identified science topics are also discussed. A significant part of the sources targeted by multi-messenger facilities is of transient nature. We have thus also discussed the synergy of Athena with wide-field high-energy facilities, taking THESEUS as a case study for transient discovery. This discussion covers all the Athena science goals that rely on follow-up observations of high-energy transients identified by external observatories, and includes also topics that are not based on multi-messenger observations, such as the search for missing baryons or the observation of early star populations and metal enrichment at the cosmic dawn with Gamma-Ray Bursts (GRBs).
Published: 2022

35. SNEWPY: A Data Pipeline from Supernova Simulations to Neutrino Signals

Author: Baxter, Amanda L., primary, BenZvi, Segev, additional, Jaimes, Joahan Castaneda, additional, Coleiro, Alexis, additional, Molla, Marta Colomer, additional, Dornic, Damien, additional, Goldhagen, Tomer, additional, Graf, Anne, additional, Griswold, Spencer, additional, Habig, Alec, additional, Hill, Remington, additional, Horiuchi, Shunsaku, additional, Kneller, James P., additional, Lang, Rafael F., additional, Lincetto, Massimiliano, additional, Migenda, Jost, additional, Nakamura, Ko, additional, O’Connor, Evan, additional, Renshaw, Andrew, additional, Scholberg, Kate, additional, Tunnell, Christopher, additional, Uberoi, Navya, additional, and Worlikar, Arkin, additional
Published: 2022
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36. INTEGRAL reloaded: Spacecraft, instruments and ground system

Author: Kuulkers, Erik, primary, Ferrigno, Carlo, additional, Kretschmar, Peter, additional, Alfonso-Garzón, Julia, additional, Baab, Marius, additional, Bazzano, Angela, additional, Bélanger, Guillaume, additional, Benson, Ian, additional, Bird, Antony J., additional, Bozzo, Enrico, additional, Brandt, Søren, additional, Coe, Elliott, additional, Caballero, Isabel, additional, Cangemi, Floriane, additional, Chenevez, Jérôme, additional, Cenko, Bradley, additional, Cinar, Nebil, additional, Coleiro, Alexis, additional, De Padova, Stefano, additional, Diehl, Roland, additional, Dietze, Claudia, additional, Domingo, Albert, additional, Drapes, Mark, additional, D’uva, Eleonora, additional, Ehle, Matthias, additional, Ebrero, Jacobo, additional, Edirimanne, Mithrajith, additional, Eismont, Natan A., additional, Finn, Timothy, additional, Fiocchi, Mariateresa, additional, Tomas, Elena Garcia, additional, Gaudenzi, Gianluca, additional, Godard, Thomas, additional, Goldwurm, Andrea, additional, Götz, Diego, additional, Gouiffès, Christian, additional, Grebenev, Sergei A., additional, Greiner, Jochen, additional, Gros, Aleksandra, additional, Hajdas, Wojciech, additional, Hanlon, Lorraine, additional, Hermsen, Wim, additional, Hernández, Cristina, additional, Hernanz, Margarita, additional, Hübner, Jutta, additional, Jourdain, Elisabeth, additional, La Rosa, Giovanni, additional, Labanti, Claudio, additional, Laurent, Philippe, additional, Lehanka, Alexander, additional, Lund, Niels, additional, Madison, James, additional, Malzac, Julien, additional, Martin, Jim, additional, Mas-Hesse, J. Miguel, additional, McBreen, Brian, additional, McDonald, Alastair, additional, McEnery, Julie, additional, Mereghetti, Sandro, additional, Natalucci, Lorenzo, additional, Ness, Jan-Uwe, additional, Oxborrow, Carol Anne, additional, Palmer, John, additional, Peschke, Sibylle, additional, Petrucciani, Francesco, additional, Pfeil, Norbert, additional, Reichenbaecher, Michael, additional, Rodi, James, additional, Rodriguez, Jérôme, additional, Roques, Jean-Pierre, additional, Doñate, Emilio Salazar, additional, Salt, Dave, additional, Sánchez-Fernández, Celia, additional, Sauvageon, Aymeric, additional, Savchenko, Volodymyr, additional, Sazonov, Sergey Yu., additional, Scaglioni, Stefano, additional, Schartel, Norbert, additional, Siegert, Thomas, additional, Southworth, Richard, additional, Sunyaev, Rashid A., additional, Toma, Liviu, additional, Ubertini, Pietro, additional, van den Heuvel, Edward P.J., additional, von Kienlin, Andreas, additional, von Krusenstiern, Nikolai, additional, Winkler, Christoph, additional, and Zannoni, Ugo, additional
Published: 2021
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37. SNEWPY: A Data Pipeline from Supernova Simulations to Neutrino Signals

Author: Baxter, Amanda, primary, BenZvi, Segev, additional, Jaimes, Joahan, additional, Coleiro, Alexis, additional, Molla, Marta, additional, Dornic, Damien, additional, Griswold, Spencer, additional, Goldhagen, Tomer, additional, Graf, Anne, additional, Habig, Alec, additional, Hill, Remington, additional, Horiuchi, Shunsaku, additional, Kneller, James, additional, Lamoureux, Mathieu, additional, Lang, Rafael, additional, Lincetto, Massimiliano, additional, Migenda, Jost, additional, Myers, McKenzie, additional, O’Connor, Evan, additional, Renshaw, Andrew, additional, Scholberg, Kate, additional, Sheshukov, Andrey, additional, Tseng, Jeff, additional, Tunnell, Christopher, additional, Uberoi, Navya, additional, and Worlikar, Arkin, additional
Published: 2021
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38. Sensitivity estimates for diffuse, point-like and extended neutrino sources with KM3NeT/ARCA

Author: Muller, Rasa, primary, heijboer, aart, additional, Garcia Soto, Alfonso, additional, Caiffi, Barbara, additional, Sanguineti, Matteo, additional, Kulikovskiy, Vladimir, additional, Ageron, Michel, additional, Aiello, Sebastiano, additional, Albert, Arnauld, additional, Alshamsi, Maitha, additional, Alves Garre, Sergio, additional, Aly, Zineb, additional, Ambrosone, Antonio, additional, Ameli, Fabrizio, additional, Andre, Michel, additional, Androulakis, Giorgos, additional, Anghinolfi, Marco, additional, Anguita, Mancia, additional, Anton, Gisela, additional, Ardid, Miquel, additional, Ardid, Salva, additional, Assal, William, additional, Aublin, Julien, additional, Bagatelas, Christos, additional, Baret, Bruny, additional, Basegmez du Pree, Suzan, additional, Bendahman, Meriem, additional, Benfenati, Francesco, additional, Berbee, Edward, additional, van den Berg, Ad, additional, Bertin, Vincent, additional, Beurthey, Stephan, additional, van Beveren, Vincent, additional, Biagi, Simone, additional, Billault, Michel, additional, Bissinger, Matthias, additional, Böttcher, Markus, additional, Bou Cabo, Manuel, additional, Boumaaza, Jihad, additional, Bouta, Mohammed, additional, Boutonnet, Claude, additional, Bouvet, Gilles, additional, Bouwhuis, Mieke, additional, Bozza, Cristiano, additional, Branzas, Horea, additional, Bruijn, Ronald, additional, Brunner, Juergen, additional, BRUNO, Riccardo, additional, Buis, Ernst-Jan, additional, Buompane, Raffaele, additional, Busto, Jose, additional, Caillat, Laurence, additional, CALVO, David, additional, Campion, Stefano, additional, Capone, Antonio, additional, Carduner, Hervé, additional, Carretero, Victor, additional, Castaldi, Paolo, additional, Celli, Silvia, additional, Cereseto, Roberto, additional, Chabab, Mohamed, additional, Champion, Cédric, additional, Chau, Nhan, additional, Chen, Andrew, additional, Cherubini, Silvio, additional, Chiarella, Vitaliano, additional, Chiarusi, Tommaso, additional, Circella, Marco, additional, Cocimano, Rosanna, additional, Coelho, Joao, additional, Coleiro, Alexis, additional, Colomer Molla, Marta, additional, Colonges, Stèphane, additional, Coniglione, Rosa, additional, Cosquer, Alain, additional, Coyle, Paschal, additional, Cresta, Massimiliano, additional, Creusot, Alexandre, additional, Cruz, Anvil, additional, CUTTONE, Giacomo, additional, D'Amico, Antonio, additional, Dallier, Richard, additional, De Martino, Bianca, additional, De Palma, Mauro, additional, Di Palma, Irene, additional, Diaz, Antonio, additional, Diego-Tortosa, Dídac, additional, Distefano, Carla, additional, Domi, Alba, additional, Donzaud, Corinne, additional, Dornic, Damien, additional, Doerr, Manuel, additional, Drouhin, Doriane, additional, Eberl, Thomas, additional, Eddyamoui, Ahmed, additional, van Eeden, Thijs, additional, van Eijk, Daan, additional, El Bojaddaini, Imad, additional, Eljarrari, Hassnae, additional, Elsaesser, Dominik, additional, Enzenhoefer, Alexander, additional, Espinosa Rosello, Victor, additional, Fermani, Paolo, additional, Ferrara, Giovanna, additional, Filipovic, Miroslav D., additional, Filippini, Francesco, additional, Fransen, Jean-Paul, additional, Fusco, Luigi Antonio, additional, Gajanana, Deepak, additional, Gal, Tamas, additional, Garcia Mendez, Juan, additional, Garcia Soto, Alfonso Andres, additional, Garcon, Evelyne, additional, Garufi, Fabio, additional, Gatius Oliver, Clara, additional, Geisselbrecht, Nicole, additional, Gialanella, Lucio, additional, Giorgio, Emidio, additional, Gozzini, Sara Rebecca, additional, Gracia, Rodrigo, additional, Graf, Kay, additional, Grella, Giuseppe, additional, Guderian, Daniel, additional, Guidi, Carlo, additional, Guillon, Benoit, additional, Gutiérrez, Miguel, additional, Haefner, Julia, additional, Hallmann, Steffen, additional, Hamdaoui, Hassane, additional, van Haren, Hans, additional, Hekalo, Amar, additional, Hennig, Lukas, additional, Henry, Sylvain, additional, Hernandez-Rey, Juan-Jose, additional, Hofestaedt, Jannik, additional, Huang, Feifei, additional, Idrissi Ibnsalih, Walid, additional, Ilioni, Alin, additional, Illuminati, Giulia, additional, James, Clancy, additional, Janezashvili, Davit, additional, Jansweijer, Peter, additional, De Jong, Maarten, additional, de Jong, Paul, additional, Jung, Bouke Jisse, additional, Kadler, Matthias, additional, Kalaczyński, Piotr, additional, KALEKIN, Oleg, additional, Katz, Ulì, additional, Kayzel, Frank, additional, Keller, Pascale, additional, Khan Chowdhury, Nafis Rezwan, additional, Kistauri, Giorgi, additional, van der Knaap, Frits, additional, Kooijman, Paul, additional, Kouchner, Antoine, additional, Kreter, Michael, additional, Labalme, Marc, additional, Lagier, Philippe, additional, Lahmann, Robert, additional, Lamare, Patrick, additional, Lamoureux, Mathieu, additional, Larosa, Giuseppina, additional, Lastoria, Chiara Filomena, additional, Laurence, Jerome, additional, Lazo, Alfonso, additional, Le Breton, Rémy, additional, Le Guirriec, Emmanuel, additional, Le Stum, Sébastien, additional, Lehaut, Gregory, additional, Leonardi, Ornella, additional, Leone, Francesco, additional, Leonora, Emanuele, additional, Lerouvillois, Christophe, additional, Lesrel, Jean, additional, Lessing, Nadja, additional, Levi, Giuseppe, additional, Lincetto, Massimiliano, additional, Lindsey Clark, Miles, additional, Lipreau, Thomas, additional, LLorens Alvarez, Carlos, additional, Lonardo, Alessandro, additional, Longhitano, Fabio, additional, Lopez Coto, Daniel, additional, Lumb, Nick, additional, Maderer, Lukas, additional, Majumdar, Jhilik, additional, Manczak, Jerzy, additional, Margiotta, Annarita, additional, Marinelli, Antonio, additional, Marini, Aurelien, additional, Markou, Christos, additional, Martin, Lilian, additional, Martinez-Mora, Juan Antonio, additional, Martini, Agnese, additional, Marzaioli, Fabio, additional, Mastroianni, Stefano, additional, Melis, Karel, additional, Miele, Gennaro, additional, Migliozzi, Pasquale, additional, Migneco, Emilio, additional, Mijakowski, Piotr, additional, Miranda Palacios, Luis Salvador, additional, Mollo, Carlos Maximiliano, additional, Mongelli, Maurizio, additional, Moussa, Abdelilah, additional, MUSICO, Paolo, additional, Musumeci, Mario, additional, Nauta, Lodewijk, additional, Navas, Sergio, additional, Nicolau, Carlo Alessandro, additional, Nkosi, Bhuti, additional, O'Fearraigh, Brian, additional, O'Sullivan, Mitchell, additional, Orlando, Angelo, additional, Ottonello, Giacomo, additional, Ottonello, Stefano, additional, Palacios González, Juan, additional, Papalashvili, Gogita, additional, Papaleo, Riccardo, additional, Pastore, Cosimo, additional, Păun, Alice, additional, Păvălaş, Gabriela Emilia, additional, Pellegrini, Giuliano, additional, Pellegrino, Carmelo, additional, Perrin-Terrin, Mathieu, additional, Pestel, Valentin, additional, Piattelli, Paolo, additional, Pieterse, Camiel, additional, Pisanti, Ofelia, additional, Poirè, Chiara, additional, Popa, Vlad, additional, Pradier, Thierry, additional, Pratolongo, Fabio, additional, Probst, Isabella, additional, PUEHLHOFER, Gerd, additional, Pulvirenti, Sara, additional, Quemener, Gilles, additional, Randazzo, Nunzio, additional, Rapicavoli, Antonio, additional, Razzaque, Soebur, additional, REAL, Diego, additional, Reck, Stefan, additional, Riccobene, Giorgio, additional, Rigalleau, Louis-Marie, additional, Romanov, Andrey, additional, Rovelli, Alberto, additional, Royon, Jerome, additional, Salesa Greus, Francisco, additional, Samtleben, Dorothea Franziska Elisabeth, additional, Sánchez-Losa, Agustín, additional, Santangelo, Andrea, additional, Santonocito, Domenico, additional, Sapienza, Piera, additional, Schmelling, Jan-Willem, additional, Schnabel, Jutta, additional, Schneider, Martin Friedrich, additional, Schumann, Johannes, additional, Schutte, Hester, additional, Seneca, Jordan, additional, Sgura, Irene, additional, Shanidze, Rezo, additional, Sharma, Ankur, additional, Sinopoulou, Anna, additional, Spisso, Bernardino, additional, Spurio, Maurizio, additional, Stavropoulos, Dimitris, additional, Steijger, Jos, additional, Stellacci, Simona Maria, additional, Taiuti, Mauro, additional, Tatone, Francesca, additional, Tayalati, Yahya, additional, Tenllado, Enrique, additional, Tezier, Damien, additional, Thakore, Tarak, additional, Theraube, Stephane, additional, Thiersen, Hannes, additional, Timmer, Paul, additional, Tingay, Steven, additional, Tsagkli, Stavroula, additional, Tsourapis, Vasileios, additional, Tzamariudaki, Ekaterini, additional, Tzanetatos, Dimitrios, additional, Valieri, Claudia, additional, Van Elewyck, Veronique, additional, Vasileiadis, George, additional, Versari, Federico, additional, Viola, Salvatore, additional, Vivolo, Daniele, additional, de Wasseige, Gwenhaël, additional, Wilms, Joern, additional, Wojaczynski, Rafal, additional, de WOLF, Els, additional, Yousfi, Tarik, additional, Zavatarelli, Sandra, additional, Zegarelli, Angela, additional, Zito, Daniele, additional, Zornoza, Juan-de-Dios, additional, Zúñiga, Juan, additional, and Żywucka, Natalia, additional
Published: 2021
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39. Follow-up of GW150914 and multi-messenger studies of transient astrophysical sources with the ANTARES neutrino telescope

Author: Coleiro Alexis
Subjects: Physics, QC1-999
Abstract: By constantly monitoring at least one complete hemisphere of the sky, neutrino telescopes are well designed to detect neutrinos emitted by transient astrophysical sources. In particular, the ANTARES telescope is currently the largest high-energy neutrino detector in the Northern Hemisphere. Searches for ANTARES neutrino candidates coincident with multi-wavelength and multi-messenger transient phenomena are performed by triggering optical, X-ray and radio observations immediately after the detection of an interesting ANTARES event and also by looking for neutrino emission spatially and temporally coincident with transient astrophysical events detected across the electromagnetic spectrum or with new messengers as gravitational-wave signals. The latest results of the multi-messenger analyses performed with ANTARES will be presented in this contribution. In particular, we will focus on the neutrino follow-up performed after the detection of the first gravitation-wave event, GW150914.
Published: 2017
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40. Comparison of the measured atmospheric muon rate with Monte Carlo simulations and sensitivity study for detection of prompt atmospheric muons with KM3NeT

Author: Kalaczyński, Piotr, primary, Ageron, Michel, additional, Aiello, Sebastiano, additional, Albert, Arnauld, additional, Alshamsi, Maitha, additional, Alves Garre, Sergio, additional, Aly, Zineb, additional, Ambrosone, Antonio, additional, Ameli, Fabrizio, additional, Andre, Michel, additional, Androulakis, Giorgos, additional, Anghinolfi, Marco, additional, Anguita, Mancia, additional, Anton, Gisela, additional, Ardid, Miquel, additional, Ardid, Salva, additional, Assal, William, additional, Aublin, Julien, additional, Bagatelas, Christos, additional, Baret, Bruny, additional, Basegmez du Pree, Suzan, additional, Bendahman, Meriem, additional, Benfenati, Francesco, additional, Berbee, Edward, additional, van den Berg, Ad, additional, Bertin, Vincent, additional, Beurthey, Stephan, additional, van Beveren, Vincent, additional, Biagi, Simone, additional, Billault, Michel, additional, Bissinger, Matthias, additional, Böttcher, Markus, additional, Bou Cabo, Manuel, additional, Boumaaza, Jihad, additional, Bouta, Mohammed, additional, Boutonnet, Claude, additional, Bouvet, Gilles, additional, Bouwhuis, Mieke, additional, Bozza, Cristiano, additional, Branzas, Horea, additional, Bruijn, Ronald, additional, Brunner, Juergen, additional, BRUNO, Riccardo, additional, Buis, Ernst-Jan, additional, Buompane, Raffaele, additional, Busto, Jose, additional, Caiffi, Barbara, additional, Caillat, Laurence, additional, CALVO, David, additional, Campion, Stefano, additional, Capone, Antonio, additional, Carduner, Hervé, additional, Carretero, Victor, additional, Castaldi, Paolo, additional, Celli, Silvia, additional, Cereseto, Roberto, additional, Chabab, Mohamed, additional, Champion, Cédric, additional, Chau, Nhan, additional, Chen, Andrew, additional, Cherubini, Silvio, additional, Chiarella, Vitaliano, additional, Chiarusi, Tommaso, additional, Circella, Marco, additional, Cocimano, Rosanna, additional, Coelho, Joao, additional, Coleiro, Alexis, additional, Colomer Molla, Marta, additional, Colonges, Stèphane, additional, Coniglione, Rosa, additional, Cosquer, Alain, additional, Coyle, Paschal, additional, Cresta, Massimiliano, additional, Creusot, Alexandre, additional, Cruz, Anvil, additional, CUTTONE, Giacomo, additional, D'Amico, Antonio, additional, Dallier, Richard, additional, De Martino, Bianca, additional, De Palma, Mauro, additional, Di Palma, Irene, additional, Diaz, Antonio, additional, Diego-Tortosa, Dídac, additional, Distefano, Carla, additional, Domi, Alba, additional, Donzaud, Corinne, additional, Dornic, Damien, additional, Doerr, Manuel, additional, Drouhin, Doriane, additional, Eberl, Thomas, additional, Eddyamoui, Ahmed, additional, van Eeden, Thijs, additional, van Eijk, Daan, additional, El Bojaddaini, Imad, additional, Eljarrari, Hassnae, additional, Elsaesser, Dominik, additional, Enzenhoefer, Alexander, additional, Espinosa Rosello, Victor, additional, Fermani, Paolo, additional, Ferrara, Giovanna, additional, Filipovic, Miroslav D., additional, Filippini, Francesco, additional, Fransen, Jean-Paul, additional, Fusco, Luigi Antonio, additional, Gajanana, Deepak, additional, Gal, Tamas, additional, Garcia-Mendez, Juan, additional, Garcia Soto, Alfonso Andres, additional, Garcon, Evelyne, additional, Garufi, Fabio, additional, Gatius Oliver, Clara, additional, Geisselbrecht, Nicole, additional, Gialanella, Lucio, additional, Giorgio, Emidio, additional, Gozzini, Sara Rebecca, additional, Gracia, Rodrigo, additional, Graf, Kay, additional, Grella, Giuseppe, additional, Guderian, Daniel, additional, Guidi, Carlo, additional, Guillon, Benoit, additional, Gutierrez, Miguel, additional, Haefner, Julia, additional, Hallmann, Steffen, additional, Hamdaoui, Hassane, additional, van Haren, Hans, additional, heijboer, aart, additional, Hekalo, Amar, additional, Hennig, Lukas, additional, Henry, Sylvain, additional, Hernandez-Rey, Juan-Jose, additional, Hofestaedt, Jannik, additional, Huang, Feifei, additional, Idrissi Ibnsalih, Walid, additional, Ilioni, Alin, additional, Illuminati, Giulia, additional, James, Clancy, additional, Janezashvili, Davit, additional, Jansweijer, Peter, additional, De Jong, Maarten, additional, de Jong, Paul, additional, Jung, Bouke Jisse, additional, Kadler, Matthias, additional, KALEKIN, Oleg, additional, Katz, Ulì, additional, Kayzel, Frank, additional, Keller, Pascale, additional, Khan Chowdhury, Nafis Rezwan, additional, Kistauri, Giorgi, additional, van der Knaap, Frits, additional, Kooijman, Paul, additional, Kouchner, Antoine, additional, Kreter, Michael, additional, Kulikovskiy, Vladimir, additional, Labalme, Marc, additional, Lagier, Philippe, additional, Lahmann, Robert, additional, Lamare, Patrick, additional, Lamoureux, Mathieu, additional, Larosa, Giuseppina, additional, Lastoria, Chiara Filomena, additional, Laurence, Jerome, additional, Lazo, Alfonso, additional, Le Breton, Remy, additional, Le Guirriec, Emmanuel, additional, Le Stum, Sebastien, additional, Lehaut, Gregory, additional, Leonardi, Ornella, additional, Leone, Francesco, additional, Leonora, Emanuele, additional, Lerouvillois, Christophe, additional, Lesrel, Jean, additional, Lessing, Nadja, additional, Levi, Giuseppe, additional, Lincetto, Massimiliano, additional, Lindsey Clark, Miles, additional, Lipreau, Thomas, additional, LLorens Alvarez, Carlos, additional, Lonardo, Alessandro, additional, Longhitano, Fabio, additional, Lopez Coto, Daniel, additional, Lumb, Nick, additional, Maderer, Lukas, additional, Majumdar, Jhilik, additional, Manczak, Jerzy, additional, Margiotta, Annarita, additional, Marinelli, Antonio, additional, Marini, Aurelien, additional, Markou, Christos, additional, Martin, Lilian, additional, Martinez-Mora, Juan Antonio, additional, Martini, Agnese, additional, Marzaioli, Fabio, additional, Mastroianni, Stefano, additional, Melis, Karel, additional, Miele, Gennaro, additional, Migliozzi, Pasquale, additional, Migneco, Emilio, additional, Mijakowski, Piotr, additional, Miranda Palacios, Luis Salvador, additional, Mollo, Carlos Maximiliano, additional, Mongelli, Maurizio, additional, Moussa, Abdelilah, additional, Muller, Rasa, additional, MUSICO, Paolo, additional, Musumeci, Mario, additional, Nauta, Lodewijk, additional, Navas, Sergio, additional, Nicolau, Carlo Alessandro, additional, Nkosi, Bhuti, additional, O'Fearraigh, Brian, additional, O'Sullivan, Mitchell, additional, Orlando, Angelo, additional, Ottonello, Giacomo, additional, Ottonello, Stefano, additional, Palacios Gonzalez, Juan, additional, Papalashvili, Gogita, additional, Papaleo, Riccardo, additional, Pastore, Cosimo, additional, Păun, Alice, additional, Păvălaş, Gabriela Emilia, additional, Pellegrini, Giuliano, additional, Pellegrino, Carmelo, additional, Perrin-Terrin, Mathieu, additional, Pestel, Valentin, additional, Piattelli, Paolo, additional, Pieterse, Camiel, additional, Pisanti, Ofelia, additional, Poirè, Chiara, additional, Popa, Vlad, additional, Pradier, Thierry, additional, Pratolongo, Fabio, additional, Probst, Isabella, additional, PUEHLHOFER, Gerd, additional, Pulvirenti, Sara, additional, Quemener, Gilles, additional, Randazzo, Nunzio, additional, Rapicavoli, Antonio, additional, Razzaque, Soebur, additional, REAL, Diego, additional, Reck, Stefan, additional, Riccobene, Giorgio, additional, Rigalleau, Louis-Marie, additional, Romanov, Andrey, additional, Rovelli, Alberto, additional, Royon, Jerome, additional, Salesa Greus, Francisco, additional, Samtleben, Dorothea Franziska Elisabeth, additional, Sánchez Losa, Agustín, additional, Sanguineti, Matteo, additional, Santangelo, Andrea, additional, Santonocito, Domenico, additional, Sapienza, Piera, additional, Schmelling, Jan-Willem, additional, Schnabel, Jutta, additional, Schneider, Martin Friedrich, additional, Schumann, Johannes, additional, Schutte, Hester, additional, Seneca, Jordan, additional, Sgura, Irene, additional, Shanidze, Rezo, additional, Sharma, Ankur, additional, Sinopoulou, Anna, additional, Spisso, Bernardino, additional, Spurio, Maurizio, additional, Stavropoulos, Dimitris, additional, Steijger, Jos, additional, Stellacci, Simona Maria, additional, Taiuti, Mauro, additional, Tatone, Francesca, additional, Tayalati, Yahya, additional, Tenllado, Enrique, additional, Tezier, Damien, additional, Thakore, Tarak, additional, Theraube, Stephane, additional, Thiersen, Hannes, additional, Timmer, Paul, additional, Tingay, Steven, additional, Tsagkli, Stavroula, additional, Tsourapis, Vasileios, additional, Tzamariudaki, Ekaterini, additional, Tzanetatos, Dimitrios, additional, Valieri, Claudia, additional, Van Elewyck, Veronique, additional, Vasileiadis, George, additional, Versari, Federico, additional, Viola, Salvatore, additional, Vivolo, Daniele, additional, de Wasseige, Gwenhaël, additional, Wilms, Joern, additional, Wojaczynski, Rafal, additional, de WOLF, Els, additional, Yousfi, Tarik, additional, Zavatarelli, Sandra, additional, Zegarelli, Angela, additional, Zito, Daniele, additional, Zornoza, Juan-de-Dios, additional, Zúñiga, Juan, additional, and Żywucka, Natalia, additional
Published: 2021
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41. PMT gain calibration and monitoring based on highly compressed hit information in KM3NeT

Author: Jung, Bouke Jisse, primary, Ageron, Michel, additional, Aiello, Sebastiano, additional, Albert, Arnauld, additional, Alshamsi, Maitha, additional, Alves Garre, Sergio, additional, Aly, Zineb, additional, Ambrosone, Antonio, additional, Ameli, Fabrizio, additional, Andre, Michel, additional, Androulakis, Giorgos, additional, Anghinolfi, Marco, additional, Anguita, Mancia, additional, Anton, Gisela, additional, Ardid, Miquel, additional, Ardid, Salva, additional, Assal, William, additional, Aublin, Julien, additional, Bagatelas, Christos, additional, Baret, Bruny, additional, Basegmez du Pree, Suzan, additional, Bendahman, Meriem, additional, Benfenati, Francesco, additional, Berbee, Edward, additional, van den Berg, Ad, additional, Bertin, Vincent, additional, Beurthey, Stephan, additional, van Beveren, Vincent, additional, Biagi, Simone, additional, Billault, Michel, additional, Bissinger, Matthias, additional, Böttcher, Markus, additional, Bou Cabo, Manuel, additional, Boumaaza, Jihad, additional, Bouta, Mohammed, additional, Boutonnet, Claude, additional, Bouvet, Gilles, additional, Bouwhuis, Mieke, additional, Bozza, Cristiano, additional, Branzas, Horea, additional, Bruijn, Ronald, additional, Brunner, Juergen, additional, BRUNO, Riccardo, additional, Buis, Ernst-Jan, additional, Buompane, Raffaele, additional, Busto, Jose, additional, Caiffi, Barbara, additional, Caillat, Laurence, additional, CALVO, David, additional, Campion, Stefano, additional, Capone, Antonio, additional, Carduner, Hervé, additional, Carretero, Victor, additional, Castaldi, Paolo, additional, Celli, Silvia, additional, Cereseto, Roberto, additional, Chabab, Mohamed, additional, Champion, Cédric, additional, Chau, Nhan, additional, Chen, Andrew, additional, Cherubini, Silvio, additional, Chiarella, Vitaliano, additional, Chiarusi, Tommaso, additional, Circella, Marco, additional, Cocimano, Rosanna, additional, Coelho, Joao, additional, Coleiro, Alexis, additional, Colomer Molla, Marta, additional, Colonges, Stèphane, additional, Coniglione, Rosa, additional, Cosquer, Alain, additional, Coyle, Paschal, additional, Cresta, Massimiliano, additional, Creusot, Alexandre, additional, Cruz, Anvil, additional, CUTTONE, Giacomo, additional, D'Amico, Antonio, additional, Dallier, Richard, additional, De Martino, Bianca, additional, De Palma, Mauro, additional, Di Palma, Irene, additional, Diaz, Antonio, additional, Diego-Tortosa, Dídac, additional, Distefano, Carla, additional, Domi, Alba, additional, Donzaud, Corinne, additional, Dornic, Damien, additional, Doerr, Manuel, additional, Drouhin, Doriane, additional, Eberl, Thomas, additional, Eddyamoui, Ahmed, additional, van Eeden, Thijs, additional, van Eijk, Daan, additional, El Bojaddaini, Imad, additional, Eljarrari, Hassnae, additional, Elsaesser, Dominik, additional, Enzenhoefer, Alexander, additional, Espinosa Rosello, Victor, additional, Fermani, Paolo, additional, Ferrara, Giovanna, additional, Filipovic, Miroslav D., additional, Filippini, Francesco, additional, Fransen, Jean-Paul, additional, Fusco, Luigi Antonio, additional, Gajanana, Deepak, additional, Gal, Tamas, additional, Garcia-Mendez, Juan, additional, Garcia Soto, Alfonso Andres, additional, Garcon, Evelyne, additional, Garufi, Fabio, additional, Gatius Oliver, Clara, additional, Geiselbrecht, Nicole, additional, Gialanella, Lucio, additional, Giorgio, Emidio, additional, Gozzini, Sara Rebecca, additional, Gracia, Rodrigo, additional, Graf, Kay, additional, Grella, Giuseppe, additional, Guderian, Daniel, additional, Guidi, Carlo, additional, Guillon, Benoit, additional, Gutierrez, Miguel, additional, Haefner, Julia, additional, Hallmann, Steffen, additional, Hamdaoui, Hassane, additional, van Haren, Hans, additional, heijboer, aart, additional, Hekalo, Amar, additional, Hennig, Lukas, additional, Henry, Sylvain, additional, Hernandez-Rey, Juan-Jose, additional, Hofestaedt, Jannik, additional, Huang, Feifei, additional, Idrissi Ibnsalih, Walid, additional, Ilioni, Alin, additional, Illuminati, Giulia, additional, James, Clancy, additional, Janezashvili, Davit, additional, Jansweijer, Peter, additional, De Jong, Maarten, additional, de Jong, Paul, additional, Jung, Bouke Jisse, additional, Kadler, Matthias, additional, Kalaczyński, Piotr, additional, KALEKIN, Oleg, additional, Katz, Ulì, additional, Kayzel, Frank, additional, Keller, Pascale, additional, Khan Chowdhury, Nafis Rezwan, additional, Kistauri, Giorgi, additional, van der Knaap, Frits, additional, Kooijman, Paul, additional, Kouchner, Antoine, additional, Kreter, Michael, additional, Kulikovskiy, Vladimir, additional, Labalme, Marc, additional, Lagier, Philippe, additional, Lahmann, Robert, additional, Lamare, Patrick, additional, Lamoureux, Mathieu, additional, Larosa, Giuseppina, additional, Lastoria, Chiara Filomena, additional, Laurence, Jerome, additional, Lazo, Alfonso, additional, Le Breton, Remy, additional, Le Guirriec, Emmanuel, additional, Le Stum, Sebastien, additional, Lehaut, Gregory, additional, Leonardi, Ornella, additional, Leone, Francesco, additional, Leonora, Emanuele, additional, Lerouvillois, Christophe, additional, Lesrel, Jean, additional, Lessing, Nadja, additional, Levi, Giuseppe, additional, Lincetto, Massimiliano, additional, Lindsey Clark, Miles, additional, Lipreau, Thomas, additional, LLorens Alvarez, Carlos, additional, Lonardo, Alessandro, additional, Longhitano, Fabio, additional, Lopez Coto, Daniel, additional, Lumb, Nick, additional, Maderer, Lukas, additional, Majumdar, Jhilik, additional, Manczak, Jerzy, additional, Margiotta, Annarita, additional, Marinelli, Antonio, additional, Marini, Aurelien, additional, Markou, Christos, additional, Martin, Lilian, additional, Martinez-Mora, Juan Antonio, additional, Martini, Agnese, additional, Marzaioli, Fabio, additional, Mastroianni, Stefano, additional, Melis, Karel, additional, Miele, Gennaro, additional, Migliozzi, Pasquale, additional, Migneco, Emilio, additional, Mijakowski, Piotr, additional, Miranda Palacios, Luis Salvador, additional, Mollo, Carlos Maximiliano, additional, Mongelli, Maurizio, additional, Moussa, Abdelilah, additional, Muller, Rasa, additional, MUSICO, Paolo, additional, Musumeci, Mario, additional, Nauta, Lodewijk, additional, Navas, Sergio, additional, Nicolau, Carlo Alessandro, additional, Nkosi, Bhuti, additional, O'Fearraigh, Brian, additional, O'Sullivan, Mitchell, additional, Orlando, Angelo, additional, Ottonello, Giacomo, additional, Ottonello, Stefano, additional, Palacios Gonzalez, Juan, additional, Papalashvili, Gogita, additional, Papaleo, Riccardo, additional, Pastore, Cosimo, additional, Păun, Alice, additional, Păvălaş, Gabriela Emilia, additional, Pellegrini, Giuliano, additional, Pellegrino, Carmelo, additional, Perrin-Terrin, Mathieu, additional, Pestel, Valentin, additional, Piattelli, Paolo, additional, Pieterse, Camiel, additional, Pisanti, Ofelia, additional, Poirè, Chiara, additional, Popa, Vlad, additional, Pradier, Thierry, additional, Pratolongo, Fabio, additional, Probst, Isabella, additional, PUEHLHOFER, Gerd, additional, Pulvirenti, Sara, additional, Quemener, Gilles, additional, Randazzo, Nunzio, additional, Rapicavoli, Antonio, additional, Razzaque, Soebur, additional, REAL, Diego, additional, Reck, Stefan, additional, Riccobene, Giorgio, additional, Rigalleau, Louis-Marie, additional, Romanov, Andrey, additional, Rovelli, Alberto, additional, Royon, Jerome, additional, Salesa Greus, Francisco, additional, Samtleben, Dorothea Franziska Elisabeth, additional, Sánchez Losa, Agustín, additional, Sanguineti, Matteo, additional, Santangelo, Andrea, additional, Santonocito, Domenico, additional, Sapienza, Piera, additional, Schmelling, Jan-Willem, additional, Schnabel, Jutta, additional, Schneider, Martin Friedrich, additional, Schumann, Johannes, additional, Schutte, Hester, additional, Seneca, Jordan, additional, Sgura, Irene, additional, Shanidze, Rezo, additional, Sharma, Ankur, additional, Sinopoulou, Anna, additional, Spisso, Bernardino, additional, Spurio, Maurizio, additional, Stavropoulos, Dimitris, additional, Steijger, Jos, additional, Stellacci, Simona Maria, additional, Taiuti, Mauro, additional, Tatone, Francesca, additional, Tayalati, Yahya, additional, Tenllado, Enrique, additional, Tezier, Damien, additional, Thakore, Tarak, additional, Theraube, Stephane, additional, Thiersen, Hannes, additional, Timmer, Paul, additional, Tingay, Steven, additional, Tsagkli, Stavroula, additional, Tsourapis, Vasileios, additional, Tzamariudaki, Ekaterini, additional, Tzanetatos, Dimitrios, additional, Valieri, Claudia, additional, Van Elewyck, Veronique, additional, Vasileiadis, George, additional, Versari, Federico, additional, Viola, Salvatore, additional, Vivolo, Daniele, additional, de Wasseige, Gwenhaël, additional, Wilms, Joern, additional, Wojaczynski, Rafal, additional, de WOLF, Els, additional, Yousfi, Tarik, additional, Zavatarelli, Sandra, additional, Zegarelli, Angela, additional, Zito, Daniele, additional, Zornoza, Juan-de-Dios, additional, Zúñiga, Juan, additional, and Żywucka, Natalia, additional
Published: 2021
Full Text: View/download PDF

42. KM3NeT Detection Unit Line Fit reconstruction using positioning sensors data

Author: Poirè, Chiara, primary, Diego-Tortosa, Dídac, additional, Ageron, Michel, additional, Aiello, Sebastiano, additional, Albert, Arnauld, additional, Alshamsi, Maitha, additional, Alves Garre, Sergio, additional, Aly, Zineb, additional, Ambrosone, Antonio, additional, Ameli, Fabrizio, additional, Andre, Michel, additional, Androulakis, Giorgos, additional, Anghinolfi, Marco, additional, Anguita, Mancia, additional, Anton, Gisela, additional, Ardid, Miquel, additional, Ardid, Salva, additional, Assal, William, additional, Aublin, Julien, additional, Bagatelas, Christos, additional, Baret, Bruny, additional, Basegmez du Pree, Suzan, additional, Bendahman, Meriem, additional, Benfenati, Francesco, additional, Berbee, Edward, additional, van den Berg, Ad, additional, Bertin, Vincent, additional, Beurthey, Stephan, additional, van Beveren, Vincent, additional, Biagi, Simone, additional, Billault, Michel, additional, Bissinger, Matthias, additional, Böttcher, Markus, additional, Bou Cabo, Manuel, additional, Boumaaza, Jihad, additional, Bouta, Mohammed, additional, Boutonnet, Claude, additional, Bouvet, Gilles, additional, Bouwhuis, Mieke, additional, Bozza, Cristiano, additional, Branzas, Horea, additional, Bruijn, Ronald, additional, Brunner, Juergen, additional, BRUNO, Riccardo, additional, Buis, Ernst-Jan, additional, Buompane, Raffaele, additional, Busto, Jose, additional, Caiffi, Barbara, additional, Caillat, Laurence, additional, CALVO, David, additional, Campion, Stefano, additional, Capone, Antonio, additional, Carduner, Hervé, additional, Carretero, Victor, additional, Castaldi, Paolo, additional, Celli, Silvia, additional, Cereseto, Roberto, additional, Chabab, Mohamed, additional, Champion, Cédric, additional, Chau, Nhan, additional, Chen, Andrew, additional, Cherubini, Silvio, additional, Chiarella, Vitaliano, additional, Chiarusi, Tommaso, additional, Circella, Marco, additional, Cocimano, Rosanna, additional, Coelho, Joao, additional, Coleiro, Alexis, additional, Colomer Molla, Marta, additional, Colonges, Stèphane, additional, Coniglione, Rosa, additional, Cosquer, Alain, additional, Coyle, Paschal, additional, Cresta, Massimiliano, additional, Creusot, Alexandre, additional, Cruz, Anvil, additional, CUTTONE, Giacomo, additional, D'Amico, Antonio, additional, Dallier, Richard, additional, De Martino, Bianca, additional, De Palma, Mauro, additional, Di Palma, Irene, additional, Diaz, Antonio, additional, Distefano, Carla, additional, Domi, Alba, additional, Donzaud, Corinne, additional, Dornic, Damien, additional, Doerr, Manuel, additional, Drouhin, Doriane, additional, Eberl, Thomas, additional, Eddyamoui, Ahmed, additional, van Eeden, Thijs, additional, van Eijk, Daan, additional, El Bojaddaini, Imad, additional, Eljarrari, Hassnae, additional, Elsaesser, Dominik, additional, Enzenhoefer, Alexander, additional, Espinosa Rosello, Victor, additional, Fermani, Paolo, additional, Ferrara, Giovanna, additional, Filipovic, Miroslav D., additional, Filippini, Francesco, additional, Fransen, Jean-Paul, additional, Fusco, Luigi Antonio, additional, Gajanana, Deepak, additional, Gal, Tamas, additional, Garcia-Mendez, Juan, additional, Garcia Soto, Alfonso Andres, additional, Garcon, Evelyne, additional, Garufi, Fabio, additional, Gatius Oliver, Clara, additional, Geisselbrecht, Nicole, additional, Gialanella, Lucio, additional, Giorgio, Emidio, additional, Gozzini, Sara Rebecca, additional, Gracia, Rodrigo, additional, Graf, Kay, additional, Grella, Giuseppe, additional, Guderian, Daniel, additional, Guidi, Carlo, additional, Guillon, Benoit, additional, Gutierrez, Miguel, additional, Haefner, Julia, additional, Hallmann, Steffen, additional, Hamdaoui, Hassane, additional, van Haren, Hans, additional, heijboer, aart, additional, Hekalo, Amar, additional, Hennig, Lukas, additional, Henry, Sylvain, additional, Hernandez-Rey, Juan-Jose, additional, Hofestaedt, Jannik, additional, Huang, Feifei, additional, Idrissi Ibnsalih, Walid, additional, Ilioni, Alin, additional, Illuminati, Giulia, additional, James, Clancy, additional, Janezashvili, Davit, additional, Jansweijer, Peter, additional, De Jong, Maarten, additional, de Jong, Paul, additional, Jung, Bouke Jisse, additional, Kadler, Matthias, additional, Kalaczyński, Piotr, additional, KALEKIN, Oleg, additional, Katz, Ulì, additional, Kayzel, Frank, additional, Keller, Pascale, additional, Khan Chowdhury, Nafis Rezwan, additional, Kistauri, Giorgi, additional, van der Knaap, Frits, additional, Kooijman, Paul, additional, Kouchner, Antoine, additional, Kreter, Michael, additional, Kulikovskiy, Vladimir, additional, Labalme, Marc, additional, Lagier, Philippe, additional, Lahmann, Robert, additional, Lamare, Patrick, additional, Lamoureux, Mathieu, additional, Larosa, Giuseppina, additional, Lastoria, Chiara Filomena, additional, Laurence, Jerome, additional, Lazo, Alfonso, additional, Le Breton, Remy, additional, Le Guirriec, Emmanuel, additional, Le Stum, Sebastien, additional, Lehaut, Gregory, additional, Leonardi, Ornella, additional, Leone, Francesco, additional, Leonora, Emanuele, additional, Lerouvillois, Christophe, additional, Lesrel, Jean, additional, Lessing, Nadja, additional, Levi, Giuseppe, additional, Lincetto, Massimiliano, additional, Lindsey Clark, Miles, additional, Lipreau, Thomas, additional, LLorens Alvarez, Carlos, additional, Lonardo, Alessandro, additional, Longhitano, Fabio, additional, Lopez Coto, Daniel, additional, Lumb, Nick, additional, Maderer, Lukas, additional, Majumdar, Jhilik, additional, Manczak, Jerzy, additional, Margiotta, Annarita, additional, Marinelli, Antonio, additional, Marini, Aurelien, additional, Markou, Christos, additional, Martin, Lilian, additional, Martinez-Mora, Juan Antonio, additional, Martini, Agnese, additional, Marzaioli, Fabio, additional, Mastroianni, Stefano, additional, Melis, Karel, additional, Miele, Gennaro, additional, Migliozzi, Pasquale, additional, Migneco, Emilio, additional, Mijakowski, Piotr, additional, Miranda Palacios, Luis Salvador, additional, Mollo, Carlos Maximiliano, additional, Mongelli, Maurizio, additional, Moussa, Abdelilah, additional, Muller, Rasa, additional, MUSICO, Paolo, additional, Musumeci, Mario, additional, Nauta, Lodewijk, additional, Navas, Sergio, additional, Nicolau, Carlo Alessandro, additional, Nkosi, Bhuti, additional, O'Fearraigh, Brian, additional, O'Sullivan, Mitchell, additional, Orlando, Angelo, additional, Ottonello, Giacomo, additional, Ottonello, Stefano, additional, Palacios Gonzalez, Juan, additional, Papalashvili, Gogita, additional, Papaleo, Riccardo, additional, Pastore, Cosimo, additional, Păun, Alice, additional, Păvălaş, Gabriela Emilia, additional, Pellegrini, Giuliano, additional, Pellegrino, Carmelo, additional, Perrin-Terrin, Mathieu, additional, Pestel, Valentin, additional, Piattelli, Paolo, additional, Pieterse, Camiel, additional, Pisanti, Ofelia, additional, Popa, Vlad, additional, Pradier, Thierry, additional, Pratolongo, Fabio, additional, Probst, Isabella, additional, PUEHLHOFER, Gerd, additional, Pulvirenti, Sara, additional, Quemener, Gilles, additional, Randazzo, Nunzio, additional, Rapicavoli, Antonio, additional, Razzaque, Soebur, additional, REAL, Diego, additional, Reck, Stefan, additional, Riccobene, Giorgio, additional, Rigalleau, Louis-Marie, additional, Romanov, Andrey, additional, Rovelli, Alberto, additional, Royon, Jerome, additional, Salesa Greus, Francisco, additional, Samtleben, Dorothea Franziska Elisabeth, additional, Sánchez Losa, Agustín, additional, Sanguineti, Matteo, additional, Santangelo, Andrea, additional, Santonocito, Domenico, additional, Sapienza, Piera, additional, Schmelling, Jan-Willem, additional, Schnabel, Jutta, additional, Schneider, Martin Friedrich, additional, Schumann, Johannes, additional, Schutte, Hester, additional, Seneca, Jordan, additional, Sgura, Irene, additional, Shanidze, Rezo, additional, Sharma, Ankur, additional, Sinopoulou, Anna, additional, Spisso, Bernardino, additional, Spurio, Maurizio, additional, Stavropoulos, Dimitris, additional, Steijger, Jos, additional, Stellacci, Simona Maria, additional, Taiuti, Mauro, additional, Tatone, Francesca, additional, Tayalati, Yahya, additional, Tenllado, Enrique, additional, Tezier, Damien, additional, Thakore, Tarak, additional, Theraube, Stephane, additional, Thiersen, Hannes, additional, Timmer, Paul, additional, Tingay, Steven, additional, Tsagkli, Stavroula, additional, Tsourapis, Vasileios, additional, Tzamariudaki, Ekaterini, additional, Tzanetatos, Dimitrios, additional, Valieri, Claudia, additional, Van Elewyck, Veronique, additional, Vasileiadis, George, additional, Versari, Federico, additional, Viola, Salvatore, additional, Vivolo, Daniele, additional, de Wasseige, Gwenhaël, additional, Wilms, Joern, additional, Wojaczynski, Rafal, additional, de WOLF, Els, additional, Yousfi, Tarik, additional, Zavatarelli, Sandra, additional, Zegarelli, Angela, additional, Zito, Daniele, additional, Zornoza, Juan-de-Dios, additional, Zúñiga, Juan, additional, and Żywucka, Natalia, additional
Published: 2021
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43. Multi-Messenger observations of the Fermi-LAT blazar 4FGL J0658.6+0636 consistent with an IceCube high-energy neutrino

Author: de Menezes, Raniere, primary, Buson, Sara, additional, Garrappa, Simone, additional, Gokus, Andrea, additional, Kadler, Matthias, additional, Cheung, Teddy, additional, Giroletti, Marcello, additional, Ajello, Marco, additional, Massaro, Francesco, additional, Peña-Herazo, Harold, additional, Schüssler, Fabian, additional, Bernardini, Elisa, additional, Satalecka, Konstancja, additional, Berti, Alessio, additional, Otero-Santos, Jorge, additional, Paggi, Alessandro, additional, Tramacere, Andrea, additional, Ward, Charlotte, additional, Gezari, Suvi, additional, Hämmerich, Steven, additional, Wilms, Joern, additional, Colmar, Werner, additional, Bach, Uwe, additional, Eppel, Florian, additional, Heßdörfer, Jonas, additional, Kraus, Alex, additional, Paraschos, Georgios Filippos, additional, Moldon, Javier, additional, Perez-Torres, Miguel, additional, Agudo, Ivan, additional, Bonnoli, Giacomo, additional, Castro-Tirado, Alberto, additional, Hu, Youdong, additional, CABALLERO-GARCIA, Maria, additional, Fernandez-Garcia, Emilio, additional, Sanchez-Ramirez, Ruben, additional, Coleiro, Alexis, additional, Kouchner, Antoine, additional, Nanci, Cristina, additional, Sheng, Yong, additional, Rajagopal, Meenakshi, additional, Adams, C., additional, Archer, A., additional, Benbow, W., additional, Brill, A., additional, Buckley, J. H., additional, Capasso, M., additional, Christiansen, J., additional, Chromey, A. J., additional, Errando, M., additional, Falcone, A., additional, Farrell, K. A., additional, Feng, Q., additional, Foote, G. M., additional, Fortson, L., additional, Furniss, A., additional, Gent, A., additional, Gillanders, G. H., additional, Giuri, C., additional, Gueta, O., additional, Hanna, D., additional, Hervet, O., additional, Holder, J., additional, Hona, B., additional, Humensky, T. B., additional, Jin, W., additional, Kaaret, P., additional, Kertzman, M., additional, K.~Kleiner, T., additional, Kumar, S., additional, Lang, M., additional, Lundy, M., additional, Maier, G., additional, McGrath, C. E., additional, Moriarty, P., additional, Mukherjee, R., additional, Nieto, D., additional, Nievas-Rosillo, M., additional, O'Brien, S., additional, Ong, R. A., additional, Otte, A., additional, Patel, S. R., additional, Pfrang, K., additional, Pohl, M., additional, Prado, R., additional, Pueschel, E., additional, Quinn, J., additional, Ragan, K., additional, Reynolds, P. T., additional, Ribeiro, D., additional, Roache, E., additional, Ryan, J. A., additional, Sadeh, I., additional, Santander, M., additional, Sembroski, G. H., additional, Shang, R., additional, Tak, D., additional, Vassiliev, V., additional, Weinstein, A., additional, Williams, D. A., additional, Williamson, T. J., additional, Walters, Richard, additional, and J. Masci, Frank, additional
Published: 2021
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44. Real-time Multi-Messenger Analysis Framework of KM3NeT

Author: Huang, Feifei, primary, Assal, William, additional, Dornic, Damien, additional, Le Guirriec, Emmanuel, additional, Lincetto, Massimiliano, additional, Vannoye, Godefroy, additional, Ageron, Michel, additional, Aiello, Sebastiano, additional, Albert, Arnauld, additional, Alshamsi, Maitha, additional, Alves Garre, Sergio, additional, Aly, Zineb, additional, Ambrosone, Antonio, additional, Ameli, Fabrizio, additional, Andre, Michel, additional, Androulakis, Giorgos, additional, Anghinolfi, Marco, additional, Anguita, Mancia, additional, Anton, Gisela, additional, Ardid, Miquel, additional, Ardid, Salva, additional, Aublin, Julien, additional, Bagatelas, Christos, additional, Baret, Bruny, additional, Basegmez du Pree, Suzan, additional, Bendahman, Meriem, additional, Benfenati, Francesco, additional, Berbee, Edward, additional, van den Berg, Ad, additional, Bertin, Vincent, additional, Beurthey, Stephan, additional, van Beveren, Vincent, additional, Biagi, Simone, additional, Billault, Michel, additional, Bissinger, Matthias, additional, Böttcher, Markus, additional, Bou Cabo, Manuel, additional, Boumaaza, Jihad, additional, Bouta, Mohammed, additional, Boutonnet, Claude, additional, Bouvet, Gilles, additional, Bouwhuis, Mieke, additional, Bozza, Cristiano, additional, Branzas, Horea, additional, Bruijn, Ronald, additional, Brunner, Juergen, additional, BRUNO, Riccardo, additional, Buis, Ernst-Jan, additional, Buompane, Raffaele, additional, Busto, Jose, additional, Caiffi, Barbara, additional, Caillat, Laurence, additional, CALVO, David, additional, Campion, Stefano, additional, Capone, Antonio, additional, Carduner, Hervé, additional, Carretero, Victor, additional, Castaldi, Paolo, additional, Celli, Silvia, additional, Cereseto, Roberto, additional, Chabab, Mohamed, additional, Champion, Cédric, additional, Chau, Nhan, additional, Chen, Andrew, additional, Cherubini, Silvio, additional, Chiarella, Vitaliano, additional, Chiarusi, Tommaso, additional, Circella, Marco, additional, Cocimano, Rosanna, additional, Coelho, Joao, additional, Coleiro, Alexis, additional, Colomer Molla, Marta, additional, Colonges, Stèphane, additional, Coniglione, Rosa, additional, Cosquer, Alain, additional, Coyle, Paschal, additional, Cresta, Massimiliano, additional, Creusot, Alexandre, additional, Cruz, Anvil, additional, CUTTONE, Giacomo, additional, D'Amico, Antonio, additional, Dallier, Richard, additional, De Martino, Bianca, additional, De Palma, Mauro, additional, Di Palma, Irene, additional, Diaz, Antonio, additional, Diego-Tortosa, Dídac, additional, Distefano, Carla, additional, Domi, Alba, additional, Donzaud, Corinne, additional, Doerr, Manuel, additional, Drouhin, Doriane, additional, Eberl, Thomas, additional, Eddyamoui, Ahmed, additional, van Eeden, Thijs, additional, van Eijk, Daan, additional, El Bojaddaini, Imad, additional, Eljarrari, Hassnae, additional, Elsaesser, Dominik, additional, Enzenhoefer, Alexander, additional, Espinosa Rosello, Victor, additional, Fermani, Paolo, additional, Ferrara, Giovanna, additional, Filipovic, Miroslav D., additional, Filippini, Francesco, additional, Fransen, Jean-Paul, additional, Fusco, Luigi Antonio, additional, Gajanana, Deepak, additional, Gal, Tamas, additional, Garcia-Mendez, Juan, additional, Garcia Soto, Alfonso Andres, additional, Garcon, Evelyne, additional, Garufi, Fabio, additional, Gatius Oliver, Clara, additional, Geisselbrecht, Nicole, additional, Gialanella, Lucio, additional, Giorgio, Emidio, additional, Gozzini, Sara Rebecca, additional, Gracia, Rodrigo, additional, Graf, Kay, additional, Grella, Giuseppe, additional, Guderian, Daniel, additional, Guidi, Carlo, additional, Guillon, Benoit, additional, Gutierrez, Miguel, additional, Haefner, Julia, additional, Hallmann, Steffen, additional, Hamdaoui, Hassane, additional, van Haren, Hans, additional, heijboer, aart, additional, Hekalo, Amar, additional, Hennig, Lukas, additional, Henry, Sylvain, additional, Hernandez-Rey, Juan-Jose, additional, Hofestaedt, Jannik, additional, Idrissi Ibnsalih, Walid, additional, Ilioni, Alin, additional, Illuminati, Giulia, additional, James, Clancy, additional, Janezashvili, Davit, additional, Jansweijer, Peter, additional, De Jong, Maarten, additional, de Jong, Paul, additional, Jung, Bouke Jisse, additional, Kadler, Matthias, additional, Kalaczyński, Piotr, additional, KALEKIN, Oleg, additional, Katz, Ulì, additional, Kayzel, Frank, additional, Keller, Pascale, additional, Khan Chowdhury, Nafis Rezwan, additional, Kistauri, Giorgi, additional, van der Knaap, Frits, additional, Kooijman, Paul, additional, Kouchner, Antoine, additional, Kreter, Michael, additional, Kulikovskiy, Vladimir, additional, Labalme, Marc, additional, Lagier, Philippe, additional, Lahmann, Robert, additional, Lamare, Patrick, additional, Lamoureux, Mathieu, additional, Larosa, Giuseppina, additional, Lastoria, Chiara Filomena, additional, Laurence, Jerome, additional, Lazo, Alfonso, additional, Le Breton, Remy, additional, Le Stum, Sebastien, additional, Lehaut, Gregory, additional, Leonardi, Ornella, additional, Leone, Francesco, additional, Leonora, Emanuele, additional, Lerouvillois, Christophe, additional, Lesrel, Jean, additional, Lessing, Nadja, additional, Levi, Giuseppe, additional, Lindsey Clark, Miles, additional, Lipreau, Thomas, additional, LLorens Alvarez, Carlos, additional, Lonardo, Alessandro, additional, Longhitano, Fabio, additional, Lopez Coto, Daniel, additional, Lumb, Nick, additional, Maderer, Lukas, additional, Majumdar, Jhilik, additional, Manczak, Jerzy, additional, Margiotta, Annarita, additional, Marinelli, Antonio, additional, Marini, Aurelien, additional, Markou, Christos, additional, Martin, Lilian, additional, Martinez-Mora, Juan Antonio, additional, Martini, Agnese, additional, Marzaioli, Fabio, additional, Mastroianni, Stefano, additional, Melis, Karel, additional, Miele, Gennaro, additional, Migliozzi, Pasquale, additional, Migneco, Emilio, additional, Mijakowski, Piotr, additional, Miranda Palacios, Luis Salvador, additional, Mollo, Carlos Maximiliano, additional, Mongelli, Maurizio, additional, Moussa, Abdelilah, additional, Muller, Rasa, additional, MUSICO, Paolo, additional, Musumeci, Mario, additional, Nauta, Lodewijk, additional, Navas, Sergio, additional, Nicolau, Carlo Alessandro, additional, Nkosi, Bhuti, additional, O'Fearraigh, Brian, additional, O'Sullivan, Mitchell, additional, Orlando, Angelo, additional, Ottonello, Giacomo, additional, Ottonello, Stefano, additional, Palacios Gonzalez, Juan, additional, Papalashvili, Gogita, additional, Papaleo, Riccardo, additional, Pastore, Cosimo, additional, Păun, Alice, additional, Păvălaş, Gabriela Emilia, additional, Pellegrini, Giuliano, additional, Pellegrino, Carmelo, additional, Perrin-Terrin, Mathieu, additional, Pestel, Valentin, additional, Piattelli, Paolo, additional, Pieterse, Camiel, additional, Pisanti, Ofelia, additional, Poirè, Chiara, additional, Popa, Vlad, additional, Pradier, Thierry, additional, Pratolongo, Fabio, additional, Probst, Isabella, additional, PUEHLHOFER, Gerd, additional, Pulvirenti, Sara, additional, Quemener, Gilles, additional, Randazzo, Nunzio, additional, Rapicavoli, Antonio, additional, Razzaque, Soebur, additional, REAL, Diego, additional, Reck, Stefan, additional, Riccobene, Giorgio, additional, Rigalleau, Louis-Marie, additional, Romanov, Andrey, additional, Rovelli, Alberto, additional, Royon, Jerome, additional, Salesa Greus, Francisco, additional, Samtleben, Dorothea Franziska Elisabeth, additional, Sánchez Losa, Agustín, additional, Sanguineti, Matteo, additional, Santangelo, Andrea, additional, Santonocito, Domenico, additional, Sapienza, Piera, additional, Schmelling, Jan-Willem, additional, Schnabel, Jutta, additional, Schneider, Martin Friedrich, additional, Schumann, Johannes, additional, Schutte, Hester, additional, Seneca, Jordan, additional, Sgura, Irene, additional, Shanidze, Rezo, additional, Sharma, Ankur, additional, Sinopoulou, Anna, additional, Spisso, Bernardino, additional, Spurio, Maurizio, additional, Stavropoulos, Dimitris, additional, Steijger, Jos, additional, Stellacci, Simona Maria, additional, Taiuti, Mauro, additional, Tatone, Francesca, additional, Tayalati, Yahya, additional, Tenllado, Enrique, additional, Tezier, Damien, additional, Thakore, Tarak, additional, Theraube, Stephane, additional, Thiersen, Hannes, additional, Timmer, Paul, additional, Tingay, Steven, additional, Tsagkli, Stavroula, additional, Tsourapis, Vasileios, additional, Tzamariudaki, Ekaterini, additional, Tzanetatos, Dimitrios, additional, Valieri, Claudia, additional, Van Elewyck, Veronique, additional, Vasileiadis, George, additional, Versari, Federico, additional, Viola, Salvatore, additional, Vivolo, Daniele, additional, de Wasseige, Gwenhaël, additional, Wilms, Joern, additional, Wojaczynski, Rafal, additional, de WOLF, Els, additional, Yousfi, Tarik, additional, Zavatarelli, Sandra, additional, Zegarelli, Angela, additional, Zito, Daniele, additional, Zornoza, Juan-de-Dios, additional, Zúñiga, Juan, additional, and Żywucka, Natalia, additional
Published: 2021
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45. Exploring the Potential of Multi-Detector Analyses for Core-Collapse Supernova Neutrino Detection

Author: Bendahman, Meriem, primary, Bugli, Matteo, additional, Coleiro, Alexis, additional, Colomer Molla, Marta, additional, de Wasseige, Gwenhaël, additional, Foglizzo, Thierry, additional, Kouchner, Antoine, additional, Regnier, Mathias, additional, Tayalati, Yahya, additional, Tonazzo, Alessandra, additional, and Van Elewyck, Veronique, additional
Published: 2021
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46. SNEWPY: A Data Pipeline from Supernova Simulations to Neutrino Signals

Author: Baxter, Amanda A.L., Benzvi, Segev, Jaimes, Joahan Castaneda, Coleiro, Alexis, Colomer Molla, Marta, Dornic, Damien, Griswold, Spencer, Goldhagen, Tomer, Graf, Anne, Habig, Alec, Hill, Remington, Horiuchi, Shunsaku, Kneller, James J.P., Lamoureux, Mathieu, Lang, Rafael R.F., Lincetto, Massimiliano, Migenda, Jost, Myers, McKenzie, O'Connor, Evan, Renshaw, Andrew, Scholberg, Kate, Sheshukov, Andrey, Tseng, Jeff, Tunnell, Christopher, Uberoi, Navya, Worlikar, Arkin, Baxter, Amanda A.L., Benzvi, Segev, Jaimes, Joahan Castaneda, Coleiro, Alexis, Colomer Molla, Marta, Dornic, Damien, Griswold, Spencer, Goldhagen, Tomer, Graf, Anne, Habig, Alec, Hill, Remington, Horiuchi, Shunsaku, Kneller, James J.P., Lamoureux, Mathieu, Lang, Rafael R.F., Lincetto, Massimiliano, Migenda, Jost, Myers, McKenzie, O'Connor, Evan, Renshaw, Andrew, Scholberg, Kate, Sheshukov, Andrey, Tseng, Jeff, Tunnell, Christopher, Uberoi, Navya, and Worlikar, Arkin
Abstract: Current neutrino detectors will observe hundreds to thousands of neutrinos from a Galactic supernova, and future detectors will increase this yield by an order of magnitude or more. With such neutrino data sets, the next Galactic supernova will significantly increase our un- derstanding of the explosions of massive stars, nuclear physics under extreme conditions, and the fundamental properties of neutrinos. However, there is a gulf between supernova simu- lations and the corresponding signals in detectors, making comparisons between theory and observation, as well as between different detectors, very diﬀicult. SNEWPY offers a unified interface for hundreds of supernova simulations, a large library of flux transformations on the way towards the detector, and an interface to SNOwGLoBES (Scholberg & SNOwGLoBES Contributors, 2021), allowing users to easily calculate and compare expected event rates from many supernova models in many different neutrino detectors., info:eu-repo/semantics/published
Published: 2021

47. PHEMTO: the polarimetric high energy modular telescope observatory

Author: Istituto Nazionale di Astrofisica, Laurent, P., Acero, F., Beckmann, V., Brandt, S., Cangemi, F., Civitani, M., Clavel-Henry, Morane, Coleiro, Alexis, Curado, R., Ferrando, P., Ferrigno, Carlo, Frontera, F., Gasteldello, F., Götz, Diego, Gouiffès, C., Grinberg, Victoria, Hanlon, L., Hartmann, D., Maggi, P., Marin, F. R., Meuris, A., Okajima, S., Pareschi, G., Pratt, G.W., Rea, Nanda, Rodríguez, J., Rossetti, M., Spiga, Daniele, Virgilli, E., Zane, Silvia, Istituto Nazionale di Astrofisica, Laurent, P., Acero, F., Beckmann, V., Brandt, S., Cangemi, F., Civitani, M., Clavel-Henry, Morane, Coleiro, Alexis, Curado, R., Ferrando, P., Ferrigno, Carlo, Frontera, F., Gasteldello, F., Götz, Diego, Gouiffès, C., Grinberg, Victoria, Hanlon, L., Hartmann, D., Maggi, P., Marin, F. R., Meuris, A., Okajima, S., Pareschi, G., Pratt, G.W., Rea, Nanda, Rodríguez, J., Rossetti, M., Spiga, Daniele, Virgilli, E., and Zane, Silvia
Abstract: Based upon dual focusing techniques, the Polarimetric High-Energy Modular Telescope Observatory (PHEMTO) is designed to have performance several orders of magnitude better than the present hard X-ray instruments, in the 1–600 keV energy range. This, together with its angular resolution of around one arcsecond, and its sensitive polarimetry measurement capability, will give PHEMTO the improvements in scientific performance needed for a mission in the 2050 era in order to study AGN, galactic black holes, neutrons stars, and supernovae. In addition, its high performance will enable the study of the non-thermal processes in galaxy clusters with an unprecedented accuracy.
Published: 2021

48. Search for spatial and temporal collective effects in the ANTARES neutrino telescope data

Author: Coleiro Alexis, Ruiz Rodrigo Gracia, and Kouchner Antoine
Subjects: Physics, QC1-999
Abstract: We investigate potential collective effects in the spatial and temporal domains in ANTARES data sets. On the one hand, we apply a two-point correlation analysis to look for inhomogeneities in the arrival directions of the high energy muon neutrino candidates detected between 2007 and 2012. This enables us to provide constraints on models of a population of point sources too faint to be detected by a likelihood-based method. On the other hand, we perform a search for ANTARES neutrino events in temporal coincidence with IceCube High-Energy Starting Events located within 45∘ from the Galactic Center. This study, also based on a two-point correlation function, is sensitive to transient emission and does not a prior on either the burst timing structure or on the electromagnetic emission. Therefore, it provides an effective way to acquire information on the possible origin of the IceCube astrophysical signal from transient sources.
Published: 2016
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49. Offline perfomance studies and first real-time results on CCSN neutrinos searches with the KM3NeT neutrino detectors

Author: Kulikovskiy, Vladimir, Molla, Marta Colomer, Lincetto, Massimiliano, Dornic, Damien, and Coleiro, Alexis
Subjects: Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, High Energy Physics::Experiment
Abstract: The KM3NeT collaboration has started the building of the ARCA and ORCA neutrino telescopes in the Mediterranean Sea. Both detectors can be used to detect core-collapse supernova neutrino bursts, exploiting correlations in the signals recorded by the 31 directional PMTs of the KM3NeT Digital Optical Modules. With the most recent data from the deployed lines, the supernovae detection algorithm and its implementation as a real time trigger have been refined and tested to be robust and effective. The first results are presented here. The expected sensitivities to the neutrino energy spectrum and time profile have also been evaluated. In addition, new approaches for the determination of the arrival time of the neutrinos at different neutrino detectors using the experimental light-curves is described. The combination of the estimations for currently running and near future neutrino detectors allows to triangulate the supernova direction in the sky.
Published: 2020
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50. Dependence of atmospheric muon flux on seawater depth measured with the first KM3NeT detection units: The KM3NeT Collaboration

Author: Ministerio de Economía y Competitividad (España), Ministerio de Ciencia, Innovación y Universidades (España), KM3NeT Collaboration, Calvo Díaz-Aldagalán, D., Coleiro, Alexis, Colomer, M., Gozzini, S.R., Hernández Rey, Juan José, Illuminati, Giulia, Khan Chowdhury, N.R., Manczak, J., Real, Diego, Thakore, T., Zornoza, J. D., Zúñiga Román, Juan, Ministerio de Economía y Competitividad (España), Ministerio de Ciencia, Innovación y Universidades (España), KM3NeT Collaboration, Calvo Díaz-Aldagalán, D., Coleiro, Alexis, Colomer, M., Gozzini, S.R., Hernández Rey, Juan José, Illuminati, Giulia, Khan Chowdhury, N.R., Manczak, J., Real, Diego, Thakore, T., Zornoza, J. D., and Zúñiga Román, Juan
Abstract: KM3NeT is a research infrastructure located in the Mediterranean Sea, that will consist of two deep-sea Cherenkov neutrino detectors. With one detector (ARCA), the KM3NeT Collaboration aims at identifying and studying TeV–PeV astrophysical neutrino sources. With the other detector (ORCA), the neutrino mass ordering will be determined by studying GeV-scale atmospheric neutrino oscillations. The first KM3NeT detection units were deployed at the Italian and French sites between 2015 and 2017. In this paper, a description of the detector is presented, together with a summary of the procedures used to calibrate the detector in-situ. Finally, the measurement of the atmospheric muon flux between 2232–3386 m seawater depth is obtained.
Published: 2020

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