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1. Purine Nucleosides with a Reactive ( β ‐Iodovinyl)sulfone or a ( β ‐Keto)sulfone Group at the C8 Position and Their Polymerase‐Catalyzed Incorporation into DNA

Author: Hasan Howlader, Sazzad H. Suzol, Kevin Blanco, Lilian Martin‐Rafa, Eduardo E. Laverde, Yuan Liu, and Stanislaw F. Wnuk
Subjects: Organic Chemistry
Published: 2022
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2. Radio detection of cosmic rays in [1.7–3.7] MHz: The EXTASIS experiment

Author: Richard Dallier, Lilian Martin, Alain Lecacheux, Benoît Revenu, D. García-Fernández, Antony Escudie, Didier Charrier, Laboratoire de physique subatomique et des technologies associées (SUBATECH), Université de Nantes - Faculté des Sciences et des Techniques, Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Unité Scientifique de la Station de Nançay (USN), Université d'Orléans (UO)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Observatoire de Paris - Site de Meudon (OBSPM), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)
Subjects: air, FOS: Physical sciences, Cosmic ray, Scintillator, 01 natural sciences, Sudden death, Signal, Observatory, Electric field, 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Instrumentation and Methods for Astrophysics (astro-ph.IM), electric field: high, 010303 astronomy & astrophysics, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, radio wave, showers: atmosphere, 010308 nuclear & particles physics, Astronomy, Astronomy and Astrophysics, observatory, cosmic radiation, Pulse-amplitude modulation, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Radio wave
Abstract: Since 2003, significant efforts have been devoted to the understanding of the radio emission of extensive air showers above 20 MHz. Despite some studies led until the early nineties, the band available below 20 MHz has remained unused for 20 years. However, it has been claimed by some pioneering experiments that extensive air showers emit a strong electric field in this band and that there is evidence of a large increase of the radio pulse amplitude with decreasing frequencies. The EXTASIS experiment, located within the Nan\c{c}ay Radioastronomy Observatory and supported by the scintillator array and the autonomous radio stations of the CODALEMA experiment, aims to re-investigate the low-frequency band, and especially to study the so-called "sudden death" contribution, the expected electric field radiated by the shower front when hitting ground level. In this work, we present the instrumental setup of the EXTASIS experiment composed of~$7$ low-frequency antennas operating in [1.7-3.7] MHz and covering approximately \SI{1}{\kilo\metre\squared}. We report the observation of~$18$ air showers detected in coincidence in the three instruments, and estimate a detection threshold of \SI{23\pm4}{\micro\volt\per\metre} from comparisons with detailed SELFAS3 simulations. We also report a strong correlation of the low-frequency signal observation with the atmospheric electric field., Comment: Submitted to Astroparticle Physics, corresponding author: Antony Escudie
Published: 2019
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3. Neutrino non-standard interactions with theKM3NeT/ORCA detector

Author: Maarten De Jong, Ad van den Berg, Nick Lumb, A. Creusot, Gennaro Miele, Giorgio Riccobene, Lucio Gialanella, Nunzio Randazzo, Giuseppe Levi, F. Filippini, Frits van der Knaap, Steven Tingay, Domenico Santonocito, Alba Domi, D. Calvo, Clara Gatius Oliver, Piera Sapienza, Evelyne Garcon, V. Popa, Steffen Hallmann, Tommaso Chiarusi, Paolo Piattelli, J. Brunner, R. Coniglione, Silvia Celli, A. Sinopoulou, Gerd Puehlhofer, Richard Dallier, S. Biagi, Daan van Eijk, Emanuele Leonora, J.D. Zornoza, Manuel Bou Cabo, Fabio Longhitano, Sandra Zavatarelli, Alessandro Lonardo, D. Gajanana, Jihad Boumaaza, Bianca De Martino, Nadja Lessing, Luis Salvador Miranda Palacios, Soebur Razzaque, Jutta Schnabel, Daniele Vivolo, Davit Janezashvili, M. Taiuti, Emmanuel Le Guirriec, Carlos Maximiliano Mollo, Ankur Sharma, S. Reck, Matthias Bissinger, Horea Branzas, Thomas Eberl, Chiara Filomena Lastoria, Mohamed Chabab, Francesco Benfenati, S. Colonges, J.A. Martínez-Mora, Alexis Coleiro, Gilles Quemener, Hannes Thiersen, Bhuti Nkosi, Stefano Ottonello, R. Muller, Fabrizio Ameli, Sergio Alves Garre, Nhan Chau, Emilio Migneco, Gwenhaël de Wasseige, Mario Musumeci, S. R. Gozzini, Bouke Jisse Jung, Alfonso Lazo, Thierry Pradier, Emidio Giorgio, D. Guderian, Piotr Mijakowski, Tarik Yousfi, Massimiliano Cresta, V. Carretero, S. Henry, Kay Graf, Karel Melis, P. Keller, Piotr Kalaczyński, A. D'Amico, Gregory Lehaut, A. Cosquer, Giovanna Ferrara, Angelo Orlando, Carmelo Pellegrino, F. Garufi, Jhilik Majumdar, Salva Ardid, Christos Markou, C. Champion, Sergio Navas Concha, C. Pieterse, Mathieu Lamoureux, C. W. James, Ornella Leonardi, Marta Colomer Molla, E. Berbee, R. Bruijn, R. Wojaczyński, Andrey Romanov, Giuseppina Larosa, Riccardo Papaleo, Anvil Cruz, L. Maderer, G. Androulakis, R. Gracia, Mauro De Palma, V. Chiarella, H. M. Schutte, Jean-Paul Fransen, Uli Katz, Luigi Antonio Fusco, Jose Busto, T. Gal, C. Distefano, Manuel Doerr, D. F. E. Samtleben, A. Hekalo, Christophe Lerouvillois, M.C. Bouwhuis, P. Timmer, J. Schmelling, T. Thakore, Imad El Bojaddaini, J. Zúñiga, M. Bouta, A. Martini, Jannik Hofestaedt, Markus Boettcher, Mancia Anguita, Lukas Hennig, H. Hamdaoui, Annarita Margiotta, Louis-Marie Rigalleau, Aurelien Marini, D. Tézier, Alice Paun, Pasquale Migliozzi, Joern Wilms, Els de Wolf, Dídac Diego-Tortosa, A. W. Chen, Jerome Laurence, Antoine Kouchner, Walid Idrissi Ibnsalih, Barbara Caiffi, Daniel Lopez Coto, Alexander Enzenhoefer, A. Zegarelli, G. Pellegrini, Ofelia Pisanti, Oleg Kalekin, Fabio Pratolongo, Nafis Rezwan Khan-Chowdhury, Michel André, Philippe Lagier, Salvatore Viola, Sébastien Le Stum, Juan Garcia Mendez, Mitchell O'Sullivan, Michael Kreter, Antonio Ambrosone, M. Anghinolfi, Rémy Le Breton, Antonio Rapicavoli, Raffaele Buompane, Irene Sgura, Vladimir Kulikovskiy, G. Vasileiadis, Antonio F. Díaz, J. Manczak, D. Elsaesser, M. Ardid, Antonio Marinelli, E. Buis, Giuseppe Grella, C. Boutonnet, Juan Paris P. Gonzalez, Sebastiano Aiello, Thomas Lipreau, Isabella Probst, Nicole Geisselbrecht, S. Theraube, Km NeT, M. D. Filipovic, G.E. Păvălaş, Corinne Donzaud, Riccardo Bruno, Maitha Alshamsi, D. Stavropoulos, Vincent van Beveren, Veronique Van Elewyck, Abdelilah Moussa, B. O'Fearraigh, Paolo Musico, Francesca Tatone, Francisco Salesa Greus, Doriane Drouhin, G. Papalashvili, Frank Kayzel, Ahmed Eddyamoui, Bernardino Spisso, C. Guidi, Jerome Royon, Hervé Carduner, Matthias Kadler, Gisela Anton, Thijs van Eeden, Rosanna Cocimano, Paul de Jong, Marco Circella, Suzan Basegmez du Pree, Gilles Bouvet, Joao Coelho, E. Tenllado, Giulia Illuminati, M. Mongelli, L. Nauta, E. Tzamariudaki, D. Tzanetatos, Giorgi Kistauri, Peter Jansweijer, Cristiano Bozza, Victor Espinosa Rosello, Robert Lahmann, P. Coyle, C. Pastore, Paolo Castaldi, Lilian Martin, Giacomo Ottonello, Giacomo Cuttone, Carlos LLorens Alvarez, Rezo Shanidze, Matteo Sanguineti, Stavroula Tsagkli, Julien Aublin, Diego Real, Roberto Cereseto, Alberto Rovelli, Fabio Marzaioli, Antonio Capone, Maurizio Spurio, F. Huang, A.J. Heijboer, Arnauld Albert, Zineb Aly, M. Perrin-Terrin, J. Seneca, Carlo Alessandro Nicolau, Hassnae Eljarrari, William Assal, Massimiliano Lincetto, V. Bertin, Martin Friedrich Schneider, L. Caillat, Valentin Pestel, Miguel Gutiérrez, C. Poirè, Patrick Lamare, Daniele Zito, Hans van Haren, Irene Di Palma, S. M. Stellacci, Stefano Mastroianni, Marc Labalme, Agustin Sanchez Losa, Andrea Santangelo, Bruny Baret, M. Ageron, Stefano Campion, Damien Dornic, Jos Steijger, Alfonso Andres Garcia Soto, Julia Haefner, Miles Lindsey Clark, S. Beurthey, M. Bendahman, C. Bagatelas, M. Billault, P.M. Kooijman, J.J. Hernández-Rey, Silvio Cherubini, Paolo Fermani, J. Schumann, Francesco Leone, Sara Pulvirenti, Vasileios Tsourapis, Benoit Guillon, Yahya Tayalati, Jean Lesrel, Natalia Zywucka, Claudia Valieri, Federico Versari, and Alin Ilioni
Subjects: Physics, Dense array, Particle physics, KM3NeT, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Phase (waves), High Energy Physics::Experiment, Sensitivity (control systems), Neutrino, Neutrino oscillation
Abstract: KM3NeT/ORCA is a dense array that constitutes the low-energy branch of the KM3NeT project with the main goal of resolving the question of the neutrino mass ordering. At present, the KM3NeT/ORCA Phase 1 has already been deployed, which means that six out of the planned 115 detection lines are operational. Even with this limited configuration, neutrino oscillations can already be measured and studied. In this contribution, the sensitivity to the neutrino Non-Standard Interactions (NSI) parameter $\epsilon_{\mu \tau}$ using the current stage of the KM3NeT/ORCA detector together with the projections for the final configuration are presented.
Published: 2021
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4. Real-time Multi-Messenger Analysis Framework of KM3NeT

Author: Salva Ardid, Martin Friedrich Schneider, Louis-Marie Rigalleau, Richard Dallier, Bianca De Martino, Uli Katz, Imad El Bojaddaini, M. Bouta, L. Caillat, Nadja Lessing, Walid Idrissi Ibnsalih, Lukas Hennig, Annarita Margiotta, Thijs van Eeden, Paolo Fermani, Miguel Gutiérrez, Jutta Schnabel, Jean-Paul Fransen, S. Reck, Riccardo Bruno, T. Gal, C. Distefano, Manuel Doerr, Tommaso Chiarusi, P. Coyle, Giacomo Cuttone, Carlos LLorens Alvarez, A. Martini, S. Colonges, Jannik Hofestaedt, Daniele Vivolo, D. F. E. Samtleben, A. Hekalo, J. Seneca, C. Poirè, Maarten De Jong, Ad van den Berg, G. Vannoye, Michel André, Sara Pulvirenti, Soebur Razzaque, G. Papalashvili, Stefano Ottonello, Ahmed Eddyamoui, Matthias Bissinger, Hassnae Eljarrari, William Assal, Tarik Yousfi, Nick Lumb, A. Creusot, Daan van Eijk, Davit Janezashvili, M. Taiuti, Emmanuel Le Guirriec, Carlos Maximiliano Mollo, Massimiliano Lincetto, Frank Kayzel, D. Stavropoulos, Vincent van Beveren, Piera Sapienza, R. Muller, S. R. Gozzini, Bouke Jisse Jung, Bernardino Spisso, C. Guidi, Aurelien Marini, Giovanna Ferrara, Angelo Orlando, Isabella Probst, S. Theraube, V. Chiarella, P. Timmer, J. Schmelling, C. Champion, Vasileios Tsourapis, Stefano Campion, Damien Dornic, Jos Steijger, S. Beurthey, Maitha Alshamsi, Hans van Haren, Gennaro Miele, Gregory Lehaut, Irene Di Palma, Jhilik Majumdar, Veronique Van Elewyck, Abdelilah Moussa, Paolo Musico, Francesca Tatone, Doriane Drouhin, Thierry Pradier, Marco Circella, M. Mongelli, L. Nauta, J. Brunner, M. Bendahman, C. Bagatelas, Matteo Sanguineti, M. D. Filipovic, G.E. Păvălaş, Francisco Salesa Greus, Julia Haefner, Andrea Santangelo, Jose Busto, Miles Lindsey Clark, Rémy Le Breton, M. Billault, Silvia Celli, Massimiliano Cresta, V. Carretero, P.M. Kooijman, B. O'Fearraigh, Carmelo Pellegrino, F. Garufi, Benoit Guillon, Manuel Bou Cabo, Fabio Longhitano, R. Coniglione, Alba Domi, D. Calvo, Clara Gatius Oliver, Raffaele Buompane, Irene Sgura, Antonio F. Díaz, Hervé Carduner, Gisela Anton, Dídac Diego-Tortosa, Natalia Zywucka, Alfonso Andres Garcia Soto, Claudia Valieri, Luis Salvador Miranda Palacios, Bhuti Nkosi, Patrick Lamare, Daniele Zito, T. Thakore, J. Zúñiga, Evelyne Garcon, V. Popa, J.D. Zornoza, Ornella Leonardi, Marta Colomer Molla, E. Berbee, Federico Versari, Horea Branzas, Oleg Kalekin, Fabio Pratolongo, Juan Garcia Mendez, D. Gajanana, L. Maderer, H. M. Schutte, J.A. Martínez-Mora, Alexis Coleiro, Jean Lesrel, Thomas Eberl, Fabrizio Ameli, Nhan Chau, Mancia Anguita, Jihad Boumaaza, Steffen Hallmann, Nafis Rezwan Khan Chowdhury, E. Tzamariudaki, Emidio Giorgio, Daniel Lopez Coto, Yahya Tayalati, Giorgio Riccobene, Gilles Quemener, Philippe Lagier, Anvil Cruz, Km NeT, Christos Markou, S. Biagi, Lucio Gialanella, Nunzio Randazzo, Alessandro Lonardo, Giuseppe Levi, Corinne Donzaud, F. Filippini, Frits van der Knaap, C. Boutonnet, Steven Tingay, C. Pieterse, Mathieu Lamoureux, Juan Paris P. Gonzalez, Zineb Aly, Markus Boettcher, Michael Kreter, C. W. James, Domenico Santonocito, D. Guderian, M. Anghinolfi, M.C. Bouwhuis, R. Bruijn, Juan José Hernández-Rey, Antonio Rapicavoli, M. Perrin-Terrin, Piotr Kalaczyński, Alfonso Lazo, Antonio Marinelli, Kay Graf, Karel Melis, Alice Paun, Emanuele Leonora, R. Wojaczyński, Chiara Filomena Lastoria, Mohamed Chabab, R. Gracia, Carlo Alessandro Nicolau, A. Cosquer, Piotr Mijakowski, Christophe Lerouvillois, Sébastien Le Stum, Stavroula Tsagkli, Riccardo Papaleo, Antoine Kouchner, G. Vasileiadis, G. Androulakis, Ankur Sharma, Andrey Romanov, Julien Aublin, A. Zegarelli, Sergio Alves Garre, Emilio Migneco, Giuseppina Larosa, Mauro De Palma, Jerome Royon, Salvatore Viola, Matthias Kadler, Paul de Jong, Suzan Basegmez du Pree, Gilles Bouvet, Joao Coelho, E. Tenllado, Mitchell O'Sullivan, Luigi Antonio Fusco, Diego Real, Giulia Illuminati, A. W. Chen, Roberto Cereseto, Giacomo Ottonello, Fabio Marzaioli, Rezo Shanidze, Alberto Rovelli, S. M. Stellacci, Arnauld Albert, Stefano Mastroianni, Marc Labalme, P. Keller, Rosanna Cocimano, Antonio Capone, Pasquale Migliozzi, Joern Wilms, Peter Jansweijer, Maurizio Spurio, F. Huang, Victor Espinosa Rosello, A.J. Heijboer, C. Pastore, Antonio Ambrosone, Ofelia Pisanti, D. Tzanetatos, Giorgi Kistauri, Cristiano Bozza, Paolo Piattelli, A. Sinopoulou, Gerd Puehlhofer, M. Ardid, Sandra Zavatarelli, Nicole Geisselbrecht, H. Hamdaoui, Barbara Caiffi, G. Pellegrini, Francesco Benfenati, Hannes Thiersen, Gwenhaël de Wasseige, Mario Musumeci, S. Henry, A. D'Amico, Robert Lahmann, Paolo Castaldi, Lilian Martin, Valentin Pestel, Agustin Sanchez Losa, Alin Ilioni, Bruny Baret, M. Ageron, Silvio Cherubini, J. Schumann, Francesco Leone, Vladimir Kulikovskiy, J. Manczak, D. Elsaesser, E. Buis, Giuseppe Grella, Sebastiano Aiello, Thomas Lipreau, Els de Wolf, S. Sánchez Navas, Jerome Laurence, Alexander Enzenhoefer, D. Tézier, V. Bertin, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), École normale supérieure de Lyon (ENS de Lyon), KM3NeT, École normale supérieure - Lyon (ENS Lyon), Bianca Keilhauer, Alexander Kappes, Assal, W., Dornic, D., Huang, F., Le Guirriec, E., Lincetto, M., Vannoye, G., Ageron, M., Aiello, S., Albert, A., Alshamsi, M., Alves Garre, S., Aly, Z., Ambrosone, A., Ameli, F., Andre, M., Androulakis, G., Anghinolfi, M., Anguita, M., Anton, G., Ardid, M., Ardid, S., Aublin, J., Bagatelas, C., Baret, B., Basegmez du Pree, S., Bendahman, M., Benfenati, F., Berbee, E., van den Berg, A. M., Bertin, V., Beurthey, S., van Beveren, V., Biagi, S., Billault, M., Bissinger, M., Boettcher, M., Bou Cabo, M., Boumaaza, J., Bouta, M., Boutonnet, C., Bouvet, G., Bouwhuis, M., Bozza, C., Branzas, H., Bruijn, R., Brunner, J., Bruno, R., Buis, E., Buompane, R., Busto, J., Caiffi, B., Caillat, L., Calvo, D., Campion, S., Capone, A., Carduner, H., Carretero, V., Castaldi, P., Celli, S., Cereseto, R., Chabab, M., Champion, C., Chau, N., Chen, A., Cherubini, S., Chiarella, V., Chiarusi, T., Circella, M., Cocimano, R., Coelho, J. A. B., Coleiro, A., Colomer Molla, M., Colonges, S., Coniglione, R., Cosquer, A., Coyle, P., Cresta, M., Creusot, A., Cruz, A., Cuttone, G., D'Amico, A., Dallier, R., De Martino, B., De Palma, M., Di Palma, I., Diaz, A. F., Diego-Tortosa, D., Distefano, C., Domi, A., Donzaud, C., Dorr, M., Drouhin, D., Eberl, T., Eddyamoui, A., van Eeden, T., van Eijk, D., El Bojaddaini, I., Eljarrari, H., Elsaesser, D., Enzenhofer, A., Espinosa, V., Fermani, P., Ferrara, G., Filipovic, M. D., Filippini, F., Fransen, J., Fusco, L. A., Gajanana, D., Gal, T., Garcia Mendez, J., Garcia Soto, A., Garcon, E., Garufi, F., Gatius, C., Geisselbrecht, N., Gialanella, L., Giorgio, E., Gozzini, S. R., Gracia, R., Graf, K., Grella, G., Guderian, D., Guidi, C., Guillon, B., Gutierrez, M., Haefner, J., Hallmann, S., Hamdaoui, H., van Haren, H., Heijboer, A., Hekalo, A., Hennig, L., Henry, S., Hernandez-Rey, J. J., Hofestadt, J., Idrissi Ibnsalih, W., Ilioni, A., Illuminati, G., James, C. W., Janezashvili, D., Jansweijer, P., de Jong, M., de Jong, P., Jung, B. J., Kadler, M., Kalaczynski, P., Kalekin, O., Katz, U. F., Kayzel, F., Keller, P., Khan Chowdhury, N. R., Kistauri, G., van der Knaap, F., Kooijman, P., Kouchner, A., Kreter, M., Kulikovskiy, V., Labalme, M., Lagier, P., Lahmann, R., Lamare, P., Lamoureux, M., Larosa, G., Lastoria, C., Laurence, J., Lazo, A., Le Breton, R., Le Stum, S., Lehaut, G., Leonardi, O., Leone, F., Leonora, E., Lerouvillois, C., Lesrel, J., Lessing, N., Levi, G., Lindsey Clark, M., Lipreau, T., LLorens Alvarez, C., Lonardo, A., Longhitano, F., Lopez-Coto, D., Lumb, N., Maderer, L., Majumdar, J., Manczak, J., Margiotta, A., Marinelli, A., Marini, A., Markou, C., Martin, L., Martinez-Mora, J. A., Martini, A., Marzaioli, F., Mastroianni, S., Melis, K. W., Miele, G., Migliozzi, P., Migneco, E., Mijakowski, P., Miranda, L. S., Mollo, C. M., Mongelli, M., Moussa, A., Muller, R., Musico, P., Musumeci, M., Nauta, L., Navas, S., Nicolau, C. A., Nkosi, B., Fearraigh, B. O., O'Sullivan, M., Orlando, A., Ottonello, G., Ottonello, S., Palacios Gonzalez, J., Papalashvili, G., Papaleo, R., Pastore, C., Paun, A. M., Pavalas, G. E., Pellegrini, G., Pellegrino, C., Perrin-Terrin, M., Pestel, V., Piattelli, P., Pieterse, C., Pisanti, O., Poire, C., Popa, V., Pradier, T., Pratolongo, F., Probst, I., Puhlhofer, G., Pulvirenti, S., Quemener, G., Randazzo, N., Rapicavoli, A., Razzaque, S., Real, D., Reck, S., Riccobene, G., Rigalleau, L., Romanov, A., Rovelli, A., Royon, J., Salesa Greus, F., Samtleben, D. F. E., Sanchez Losa, A., Sanguineti, M., Santangelo, A., Santonocito, D., Sapienza, P., Schmelling, J., Schnabel, J., Schneider, M. F., Schumann, J., Schutte, H. M., Seneca, J., Sgura, I., Shanidze, R., Sharma, A., Sinopoulou, A., Spisso, B., Spurio, M., Stavropoulos, D., Steijger, J., Stellacci, S. M., Taiuti, M., Tatone, F., Tayalati, Y., Tenllado, E., Tezier, D., Thakore, T., Theraube, S., Thiersen, H., Timmer, P., Tingay, S., Tsagkli, S., Tsourapis, V., Tzamariudaki, E., Tzanetatos, D., Valieri, C., Van Elewyck, V., Vasileiadis, G., Versari, F., Viola, S., Vivolo, D., de Wasseige, G., Wilms, J., Wojaczynski, R., de Wolf, E., Yousfi, T., Zavatarelli, S., Zegarelli, A., Zito, D., Zornoza, J. D., Zuniga, J., and Zywucka, N.
Subjects: data analysis method, accelerator, Computer science, Astrophysics::High Energy Astrophysical Phenomena, Real-time computing, FOS: Physical sciences, GeV, 01 natural sciences, 030218 nuclear medicine & medical imaging, High Energy Physics - Experiment, 03 medical and health sciences, High Energy Physics - Experiment (hep-ex), talk: online 2021/18/05, neutrino, 0302 clinical medicine, Observatory, 0103 physical sciences, supernova, optical, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], neutrino: supernova, 14. Life underwater, Neutrino oscillation, Instrumentation, KM3NeT, Mathematical Physics, Physics, 010308 nuclear & particles physics, Gravitational wave, Astrophysics::Instrumentation and Methods for Astrophysics, gravitational radiation, Astronomy, trigger, oscillation, observatory, monitoring, electromagnetic, neutrino: oscillation, proposed experiment, on-line
Abstract: KM3NeT is a multi-purpose cubic-kilometer neutrino observatory under construction in the Mediterranean Sea. It consists of ORCA and ARCA (for Oscillation and Astroparticle Research with Cosmics in the Abyss, respectively), currently both have a few detection lines in operation. Although having different primary goals, both detectors can be used for neutrino astronomy over a wide energy range, from a few tens of MeVs to a few tens of PeV. In view of the growing field of time-domain astronomy, it is crucial to be able to identify neutrino candidates in real-time. This online neutrino sample will allow triggered neutrino alerts that will be sent to the astronomy community and to look for time/space coincidences around external electromagnetic and multi-messenger triggers. These real-time searches can significantly increase the discovery potential of transient cosmic accelerators and refine the pointing directions in the case of poorly localized triggers, such as gravitational waves. In the field of core-collapse supernovae (CCSN), the detection of the MeV-scale CCSN neutrinos is crucial as an early warning of the electromagnetic follow-up. KM3NeT's digital optical modules act as good detectors for these supernovae neutrinos. This proceeding presents the status of KM3NeT's real-time multi-messenger activities, including online event reconstruction, event classification and selection, alert distribution, and supernova monitoring., 6 pages, 6 figures, VLVNT2021 conference proceedings
Published: 2021
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5. Architecture and performance of the KM3NeT front-end firmware

Author: Suzan Basegmez du Pree, Daan van Eijk, Silvia Celli, Francisco Salesa Greus, Fabrizio Raffaelli, Joao Coelho, E. Tenllado, M. Taiuti, Carlos Maximiliano Mollo, S. Mazzou, Gisela Anton, Diego Real, S. Biagi, Antonio D'Onofrio, Giulia Illuminati, Alessandro Lonardo, E. Tzamariudaki, Alfonso Andres Garcia Soto, Uli Katz, Thijs van Eeden, David Muñoz Pérez, M. Morganti, Jörn Wilms, Thierry Pradier, S. Rivoire, P. Coyle, Imad El Bojaddaini, Zineb Aly, Giacomo Cuttone, M. Perrin-Terrin, Carlo Alessandro Nicolau, H. Brânzaş, Thomas Eberl, Dídac Diego-Tortosa, M. Bouta, K. Pikounis, Paolo Fermani, Gwenhaël de Wasseige, Mario Musumeci, D. Stavropoulos, Vincent van Beveren, S. Colonges, Veronique Van Elewyck, Abdelilah Moussa, Paolo Musico, Tommaso Chiarusi, Miles Lindsey Clark, P.M. Kooijman, R. Muller, S. M. Stellacci, Emanuele Leonora, S. R. Gozzini, M. Ardid, Jose Busto, Bouke Jisse Jung, Michael Kreter, M. Anghinolfi, A. Martini, N. Geißelbrecht, Annarita Margiotta, A. D'Amico, Dario Grasso, T. Thakore, Sara Pulvirenti, Jean Lesrel, Stefano Mastroianni, A. W. Chen, Doriane Drouhin, H. Hamdaoui, Mohamed Chabab, Jutta Schnabel, Giovanna Ferrara, J.J. Hernández-Rey, Jürgen Brunner, Rémy Le Breton, Raffaele Buompane, Damien Dornic, Angelo Orlando, Jos Steijger, Rosanna Cocimano, Irene Sgura, Antonio F. Díaz, Andrea Biagioni, S. Reck, Corinne Donzaud, Barbara Caiffi, Piotr Mijakowski, G. Pellegrini, Michel André, Alin Ilioni, Francesco Simeone, Fabio Marzaioli, Giancarlo Barbarino, M. Richer, Paolo Piattelli, A. Sinopoulou, M. Bendahman, C. Bagatelas, Sandra Zavatarelli, Juan Paris P. Gonzalez, R. Wojaczyński, R. Bruijn, Arnauld Albert, Riccardo Papaleo, Julien Aublin, M. Dörr, G. Androulakis, R. Coniglione, T. Gal, R. Gracia, C. Distefano, Antoine Kouchner, Ofelia Pisanti, Richard Dallier, Daniele Vivolo, D. F. E. Samtleben, A. Hekalo, Mancia Anguita, Matthias Bissinger, A. Zegarelli, Robert Lahmann, J. Hofestädt, Paolo Castaldi, Lilian Martin, Bernardino Spisso, C. Guidi, Pasquale Migliozzi, Jihad Boumaaza, Mitchell O'Sullivan, L. Maderer, R. Donà, Y. Gatelet, Natalia Zywucka, O. Rabyang, Agustin Sanchez Losa, Els Koffeman, Federico Versari, A. Belias, Bruny Baret, Markus Boettcher, Rezo Shanidze, Silvio Cherubini, J. Schumann, Francesco Leone, D. Guderian, D. Tzanetatos, Giorgi Kistauri, Cristiano Bozza, Kay Graf, Karel Melis, Walid Idrissi Ibnsalih, Soebur Razzaque, Piera Sapienza, V. Chiarella, J. Schmelling, G. Pühlhofer, Fabio Longhitano, V. Carretero, Nhan Chau, Piotr Kalaczyński, Giuseppina Larosa, Mauro De Palma, G. Papalashvili, Karl Mannheim, D. Zaborov, Marco Circella, Ahmed Eddyamoui, L. Nauta, Victor Espinosa Rosell, Matteo Sanguineti, Christos Markou, Carmelo Pellegrino, F. Garufi, C. Pieterse, V. Bertin, C. W. James, Alice Paun, M. D. Filipovic, G.E. Păvălaş, C. Poirè, G. Vasileiadis, Daniele Zito, S. Viola, Ankur Sharma, Ornella Leonardi, Maarten De Jong, Marta Colomer Molla, E. Berbee, Sergio Alves Garre, Emilio Migneco, Imanol Corredoira, Ad van den Berg, Nafis Rezwan Khan Chowdhury, Oleg Kalekin, M. Organokov, B. Ó Fearraigh, A. Creusot, Antonio Marinelli, Gennaro Miele, Giorgio Riccobene, Lucio Gialanella, J.D. Zornoza, Nunzio Randazzo, Giuseppe Levi, F. Filippini, Frits van der Knaap, Steven Tingay, Domenico Santonocito, J. Seneca, Michael Moser, Alba Domi, D. Calvo, Massimiliano Lincetto, D. Lopez-Coto, V. Popa, Steffen Hallmann, Hans van Haren, Irene Di Palma, Andrea Santangelo, Yahya Tayalati, Matthias Kadler, Paul de Jong, Peter Jansweijer, C. Pastore, Luis Salvador Miranda Palacios, J. Zúñiga, J.A. Martínez-Mora, Alexis Coleiro, Fabrizio Ameli, Alberto Rovelli, Emidio Giorgio, Vladimir Kulikovskiy, Luigi Antonio Fusco, Antonio Capone, J. Manczak, D. Elsaesser, Maurizio Spurio, E. Buis, F. Huang, A.J. Heijboer, M.C. Bouwhuis, Giuseppe Grella, Sebastiano Aiello, Thomas Lipreau, Els de Wolf, S. Sánchez Navas, Alexander Enzenhoefer, O. Gabella, KM3NeT (IHEF, IoP, FNWI), Aiello, Sebastiano, Albert, Arnauld, Garre, Sergio Alve, Aly, Zineb, Ameli, Fabrizio, Andre, Michel, Androulakis, Giorgo, Anghinolfi, Marco, Anguita, Mancia, Anton, Gisela, Ardid, Miquel, Aublin, Julien, Bagatelas, Christo, Barbarino, Giancarlo, Baret, Bruny, Basegmez du Pree, Suzan, Belias, Anastasio, Bendahman, Meriem, Berbee, Edward, van den Berg, Ad M., Bertin, Vincent, van Beveren, Vincent, Biagi, Simone, Biagioni, Andrea, Bissinger, Matthia, Boettcher, Marku, Boumaaza, Jihad, Bouta, Mohammed, Bouwhuis, Mieke, Bozza, Cristiano, Brânzaş, Horea, Bruijn, Ronald, Brunner, Jurgen, Buis, Ernst-Jan, Buompane, Raffaele, Busto, Jose, Caiffi, Barbara, Calvo, David, Capone, Antonio, Carretero, Victor, Castaldi, Paolo, Celli, Silvia, Chabab, Mohamed, Chau, Nhan, Chen, Andrew W., Cherubini, Silvio, Chiarella, Vitaliano, Chiarusi, Tommaso, Circella, Marco, Cocimano, Rosanna, Coelho, Joao A. B., Coleiro, Alexi, Molla, Marta C., Colonges, Stephane, Coniglione, Rosa, Corredoira, Imanol, Coyle, Paschal, Creusot, Alexandre, Cuttone, Giacomo, Amico, Antonio D’, D’Onofrio, Antonio, Dallier, Richard, De Palma, Mauro, Di Palma, Irene, Díaz, Antonio F., Diego-Tortosa, Didac, Distefano, Carla, Domi, Alba, Donà, Roberto, Donzaud, Corinne, Dornic, Damien, Dörr, Manuel, Drouhin, Doriane, Eberl, Thoma, Eddyamoui, Ahmed, van Eeden, Thij, van Eijk, Daan, El Bojaddaini, Imad, Elsaesser, Dominik, Enzenhoefer, Alexander, Rosell, Victor Espinosa, Fermani, Paolo, Ferrara, Giovanna, Filipović, Miroslav D., Filippini, Francesco, Fusco, Luigi A., Gabella, Omar, Gal, Tama, Soto, Alfonso Andres Garcia, Garufi, Fabio, Gatelet, Yoann, Geißelbrecht, Nicole, Gialanella, Lucio, Giorgio, Emidio, Gozzini, Sara R., Gracia, Rodrigo, Graf, Kay, Grasso, Dario, Grella, Giuseppe, Guderian, Daniel, Guidi, Carlo, Hallmann, Steffen, Hamdaoui, Hassane, van Haren, Han, Heijboer, Aart, Hekalo, Amar, Hernández-Rey, Juan J., Hofestädt, Jannik, Huang, Feifei, Ibnsalih, Walid Idrissi, Ilioni, Alin, Illuminati, Giulia, James, Clancy W., Jansweijer, Peter, de Jong, Maartin, de Jong, Paul, Jung, Bouke Jisse, Kadler, Matthia, Kalaczyński, Piotr, Kalekin, Oleg, Katz, Uli F., Khan Chowdhury, Nafis R., Kistauri, Giorgi, van der Knaap, Frit, Koffeman, Els N., Kooijman, Paul, Kouchner, Antoine, Kreter, Michael, Kulikovskiy, Vladimir, Lahmann, Robert, Larosa, Giuseppina, Le Breton, Remy, Leonardi, Ornella, Leone, Francesco, Leonora, Emanuele, Lesrel, Jean, Levi, Giuseppe, Lincetto, Massimiliano, Lindsey Clark, Mile, Lipreau, Thoma, Lonardo, Alessandro, Longhitano, Fabio, Lopez-Coto, Daniel, Maderer, Luka, Mańczak, Jerzy M., Mannheim, Karl, Margiotta, Annarita, Marinelli, Antonio, Markou, Christo, Martin, Lilian, Martínez-Mora, Juan A., Martini, Agnese, Marzaioli, Fabio, Mastroianni, Stefano, Mazzou, Safaa, Melis, Karel W., Miele, Gennaro, Migliozzi, Pasquale, Migneco, Emilio, Mijakowski, Piotr, Miranda Palacios, Luis S., Mollo, Carlos M., Morganti, Mauro, Moser, Michael, Moussa, Abdelilah, Muller, Rasa, Pérez, David Muñoz, Musico, Paolo, Musumeci, Mario, Nauta, Lodewijk, Navas, Sergio, Nicolau, Carlo A., Fearraigh, Brian Ó., O’Sullivan, Mitchell, Organokov, Mukharbek, Orlando, Angelo, González, Juan Palacio, Papalashvili, Gogita, Papaleo, Riccardo, Pastore, Cosimo, Păun, Alice M., Păvălaş, Gabriela E., Pellegrini, Giuliano, Pellegrino, Carmelo, Perrin-Terrin, Mathieu, Piattelli, Paolo, Pieterse, Camiel, Pikounis, Konstantino, Pisanti, Ofelia, Poirè, Chiara, Popa, Vlad, Pradier, Thierry, Pühlhofer, Gerd, Pulvirenti, Sara, Rabyang, Omphile, Raffaelli, Fabrizio, Randazzo, Nunzio, Razzaque, Soebur, Real, Diego, Reck, Stefan, Riccobene, Giorgio, Richer, Marc, Rivoire, Stephane, Rovelli, Alberto, Salesa Greus, Francisco, Samtleben, Dorothea F. E., Sánchez Losa, Agustin, Sanguineti, Matteo, Santangelo, Andrea E., Santonocito, Domenico, Sapienza, Piera, Schmelling, Jan-Willem, Schnabel, Jutta, Schumann, Johanne, Seneca, Jordan, Sgura, Irene, Shanidze, Rezo, Sharma, Ankur, Simeone, Francesco, Sinopoulou, Anna, Spisso, Bernardino, Spurio, Maurizio, Stavropoulos, Dimitri, Steijger, Jo, Stellacci, Simona Maria, Taiuti, Mauro, Tayalati, Yahya, Tenllado, Enrique, Thakore, Tarak, Tingay, Steven, Tzamariudaki, Ekaterini, Tzanetatos, Dimitrio, Van Elewyck, Veronique, Vasileiadis, George, Versari, Federico, Viola, Salvo, Vivolo, Daniele, de Wasseige, Gwenhael, Wilms, Joern, Wojaczyński, Rafa, de Wolf, El, Zaborov, Dmitry, Zavatarelli, Sandra, Zegarelli, Angela, Zito, Daniele, de Dios Zornoza, Juan, Zúñiga, Juan, Zywucka, Natalia, Aiello, S., Albert, A., Garre, S. A., Aly, Z., Ameli, F., Andre, M., Androulakis, G., Anghinolfi, M., Anguita, M., Anton, G., Ardid, M., Aublin, J., Bagatelas, C., Barbarino, G., Baret, B., Du Pree, S. B., Belias, A., Bendahman, M., Berbee, E., Van Den Berg, A. M., Bertin, V., Van Beveren, V., Biagi, S., Biagioni, A., Bissinger, M., Boettcher, M., Boumaaza, J., Bouta, M., Bouwhuis, M., Bozza, C., Branzas, H., Bruijn, R., Brunner, J., Buis, E. -J., Buompane, R., Busto, J., Caiffi, B., Calvo, D., Capone, A., Carretero, V., Castaldi, P., Celli, S., Chabab, M., Chau, N., Chen, A., Cherubini, S., Chiarella, V., Chiarusi, T., Circella, M., Cocimano, R., Coelho, J. A. B., Coleiro, A., Molla, M. C., Colonges, S., Coniglione, R., Corredoira, I., Coyle, P., Creusot, A., Cuttone, G., Amico, A. D., D'Onofrio, A., Dallier, R., De Palma, M., Di Palma, I., Diaz, A. F., Diego-Tortosa, D., Distefano, C., Domi, A., Dona, R., Donzaud, C., Dornic, D., Doerr, M., Drouhin, D., Eberl, T., Eddyamoui, A., Van Eeden, T., Van Eijk, D., El Bojaddaini, I., Elsaesser, D., Enzenhoefer, A., Rosell, V. E., Fermani, P., Ferrara, G., Filipovic, M. D., Filippini, F., Fusco, L. A., Gabella, O., Gal, T., Soto, A. A. G., Garufi, F., Gatelet, Y., Geisselbrecht, N., Gialanella, L., Giorgio, E., Gozzini, S. R., Gracia, R., Graf, K., Grasso, D., Grella, G., Guderian, D., Guidi, C., Hallmann, S., Hamdaoui, H., Van Haren, H., Heijboer, A., Hekalo, A., Hernandez-Rey, J. J., Hofestadt, J., Huang, F., Ibnsalih, W. I., Ilioni, A., Illuminati, G., James, C. W., Jansweijer, P., De Jong, M., De Jong, P., Jung, B. J., Kadler, M., Kalaczynski, P., Kalekin, O., Katz, U. F., Chowdhury, N. R. K., Kistauri, G., Van Der Knaap, F., Koffeman, E. N., Kooijman, P., Kouchner, A., Kreter, M., Kulikovskiy, V., Lahmann, R., Larosa, G., Le Breton, R., Leonardi, O., Leone, F., Leonora, E., Lesrel, J., Levi, G., Lincetto, M., Clark, M. L., Lipreau, T., Lonardo, A., Longhitano, F., Lopez-Coto, D., Maderer, L., Manczak, J. M., Mannheim, K., Margiotta, A., Marinelli, A., Markou, C., Martin, L., Martinez-Mora, J. A., Martini, A., Marzaioli, F., Mastroianni, S., Mazzou, S., Melis, K. W., Miele, G., Migliozzi, P., Migneco, E., Mijakowski, P., Palacios, L. S. M., Maximiliano Mollo, C., Morganti, M., Moser, M., Moussa, A., Muller, R., Perez, D. M., Musico, P., Musumeci, M., Nauta, L., Navas, S., Nicolau, C. A., Fearraigh, B. O., O'Sullivan, M., Organokov, M., Orlando, A., Gonzalez, J. P., Papalashvili, G., Papaleo, R., Pastore, C., Paun, A. M., Pavalas, G. E., Pellegrini, G., Pellegrino, C., Perrin-Terrin, M., Piattelli, P., Pieterse, C., Pikounis, K., Pisanti, O., Poire, C., Popa, V., Pradier, T., Puhlhofer, G., Pulvirenti, S., Rabyang, O., Raffaelli, F., Randazzo, N., Razzaque, S., Real, D., Reck, S., Riccobene, G., Richer, M., Rivoire, S., Rovelli, A., Salesa Greus, F., Samtleben, D. F. E., Losa, A. S., Sanguineti, M., Santangelo, A. E., Santonocito, D., Sapienza, P., Schmelling, J. -W., Schnabel, J., Schumann, J., Seneca, J., Sgura, I., Shanidze, R., Sharma, A., Simeone, F., Sinopoulou, A., Spisso, B., Spurio, M., Stavropoulos, D., Steijger, J., Stellacci, S. M., Taiuti, M., Tayalati, Y., Tenllado, E., Thakore, T., Tingay, S., Tzamariudaki, E., Tzanetatos, D., Van Elewyck, V., Vasileiadis, G., Versari, F., Viola, S., Vivolo, D., De Wasseige, G., Wilms, J., Wojaczynski, R., De Wolf, E., Zaborov, D., Zavatarelli, S., Zegarelli, A., Zito, D., De Dios Zornoza, J., Zuniga, J., Zywucka, N., Groupe de Recherche en Physique des Hautes Energies (GRPHE), Institut Universitaire de Technologie de Colmar-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Laboratoire de physique subatomique et des technologies associées (SUBATECH), Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Laboratoire Univers et Particules de Montpellier (LUPM), Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Montpellier 2 - Sciences et Techniques (UM2), Institut Universitaire de France (IUF), Ministère de l'Education nationale, de l’Enseignement supérieur et de la Recherche (M.E.N.E.S.R.), KM3NeT, Research unit Astroparticle Physics, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-IUT de Colmar, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique et Atmosphères = Laboratory for Studies of Radiation and Matter in Astrophysics and Atmospheres (LERMA), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-CY Cergy Paris Université (CY), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT)-Nantes université - UFR des Sciences et des Techniques (Nantes univ - UFR ST), Nantes Université - pôle Sciences et technologie, Nantes Université (Nantes Univ)-Nantes Université (Nantes Univ)-Nantes Université - pôle Sciences et technologie, Nantes Université (Nantes Univ)-Nantes Université (Nantes Univ), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), ANR-15-CE31-0020,DAEMONS,Démonstration de la possibilité d'établir l'ordonnancement des masses de neutrinos dans la mer(2015), ANR-10-LABX-0023,UnivEarthS,Earth - Planets - Universe: observation, modeling, transfer(2010), ANR-18-IDEX-0001,Université de Paris,Université de Paris(2018), Centre Tecnològic de Vilanova i la Geltrú, and Universitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques
Subjects: Astrofísica, acquisition firmware, KM3NeT, neutrino telescope, time to digital converters, Computer science, data acquisition, Physics::Instrumentation and Detectors, time-to-digital converter, computer.software_genre, Astrophysics, Neutrino telescope, 01 natural sciences, Front and back ends, Time-to-digital converter, Atmospheric Cherenkov telescopes, time to digital converter, 010303 astronomy & astrophysics, Instrumentation, FPGA, Clocks, photomultiplier, Firmware, 4. Education, Physics, Electrical engineering, Astrophysics::Instrumentation and Methods for Astrophysics, Electronic, Optical and Magnetic Materials, Acquisition firmware, Neutrino, performance, Photomultiplier, Logic, Astrophysics::High Energy Astrophysical Phenomena, Physique [physics]/Physique [physics], Partícules (Física nuclear), 010309 optics, 0103 physical sciences, Quantization, 14. Life underwater, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Field-programmable gate array, Cherenkov radiation, Particles (Nuclear physics), Detectors òptics, Time to digital converters, Optical detectors, Control systems, Photons, Física [Àrees temàtiques de la UPC], Telescopis, business.industry, Mechanical Engineering, Data acquisition, Field programmable gate arrays, Astronomy and Astrophysics, Physique [physics]/Physique des Hautes Energies - Expérience [hep-ex], Space and Planetary Science, Control and Systems Engineering, FISICA APLICADA, electronics: readout, business, computer, Telescopes, electronics: design
Abstract: The authors acknowledge the financial support of the funding agencies: Agence Nationale de la Recherche (contract ANR-15-CE31-0020), Centre National de la Recherche Scientifique (CNRS), Commission Europeenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), LabEx UnivEarthS (ANR-10-LABX-0023 and ANR-18-IDEX-0001), Paris Ile-de-France Region, France; Shota Rustaveli National Science Foundation of Georgia (SRNSFG, FR-18-1268), Georgia; Deutsche Forschungsgemeinschaft (DFG), Germany; The General Secretariat of Research and Technology (GSRT), Greece; Istituto Nazionale di Fisica Nucleare (INFN), Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR), PRIN 2017 program (Grant NAT-NET 2017W4HA7S) Italy; Ministry of Higher Education Scientific Research and Professional Training, ICTP through Grant AF-13, Morocco; Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; The National Science Centre, Poland (2015/18/E/ST2/00758); National Authority for Scientific Research (ANCS), Romania; Ministerio de Ciencia, Innovacion, Investigacion y Universidades (MCIU): Programa Estatal de Generacion de Conocimiento (refs. PGC2018-096663-B-C41, -A-C42, -B-C43, -B-C44) (MCIU/FEDER), Severo Ochoa Centre of Excellence and MultiDark Consolider (MCIU), Junta de Andalucia (ref. SOMM17/6104/UGR), Generalitat Valenciana: Grisolia (ref. GRISOLIA/2018/119) and GenT (ref. CIDEGENT/2018/034) programs, La Caixa Foundation (ref. LCF/BQ/IN17/11620019), EU: MSC program (ref. 713673), Spain., The KM3NeT infrastructure consists of two deep-sea neutrino telescopes being deployed in the Mediterranean Sea. The telescopes will detect extraterrestrial and atmospheric neutrinos by means of the incident photons induced by the passage of relativistic charged particles through the seawater as a consequence of a neutrino interaction. The telescopes are configured in a three-dimensional grid of digital optical modules, each hosting 31 photomultipliers. The photomultiplier signals produced by the incident Cherenkov photons are converted into digital information consisting of the integrated pulse duration and the time at which it surpasses a chosen threshold. The digitization is done by means of time to digital converters (TDCs) embedded in the field programmable gate array of the central logic board. Subsequently, a state machine formats the acquired data for its transmission to shore. We present the architecture and performance of the front-end firmware consisting of the TDCs and the state machine., French National Research Agency (ANR) ANR-15-CE31-0020, Centre National de la Recherche Scientifique (CNRS), Commission Europeenne (FEDER fund), France, Commission Europeenne (Marie Curie Program), France, Institut Universitaire de France (IUF), France, LabEx UnivEarthS, France ANR-10-LABX-0023 ANR-18-IDEX-0001, Paris Ile-de-France Region, France, Shota Rustaveli National Science Foundation of Georgia (SRNSFG), Georgia FR-18-1268, German Research Foundation (DFG), Greek Ministry of Development-GSRT, Istituto Nazionale di Fisica Nucleare (INFN) NAT-NET 2017W4HA7S, Ministry of Education, Universities and Research (MIUR) NAT-NET 2017W4HA7S, PRIN 2017 program Italy NAT-NET 2017W4HA7S, Ministry of Higher Education Scientific Research and Professional Training, ICTP, Morocco AF-13, Netherlands Organization for Scientific Research (NWO) Netherlands Government, National Science Centre, Poland 2015/18/E/ST2/00758, National Authority for Scientific Research (ANCS), Romania, Ministerio de Ciencia, Innovacion, Investigacion y Universidades (MCIU): Programa Estatal de Generacion de Conocimiento (MCIU/FEDER), Spain PGC2018-096663-B-C41 PGC2018-096663-A-C42 PGC2018-096663-B-C43 PGC2018-096663-B-C44, Severo Ochoa Centre of Excellence and MultiDark Consolider (MCIU), Spain, Junta de Andalucia European Commission SOMM17/6104/UGR, Generalitat Valenciana: Grisolia program, Spain GRISOLIA/2018/119, Generalitat Valenciana: GenT program, Spain CIDEGENT/2018/034, La Caixa Foundation LCF/BQ/IN17/11620019, EU: MSC program, Spain 713673
Published: 2021
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6. Pulsars with NenuFAR: backend and pipelines

Author: Cyril Tasse, A. Possenti, Serge Yerin, Siyuan Chen, L. Bondonneau, C. Viou, M. Serylak, G. Shaifullah, Richard Dallier, J. W. McKee, Z. Wu, Julien N. Girard, Baptiste Cecconi, J.-M. Grießmeier, V. I. Kondratiev, M. Tagger, L. Guillemot, M. Brionne, Maura Pilia, R. A. Main, A. Loh, Ismaël Cognard, P. Zarka, Joris P. W. Verbiest, Caterina Tiburzi, Lilian Martin, Carine Briand, Stephane Corbel, A. V. Bilous, G. Theureau, Olaf Wucknitz, Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Unité Scientifique de la Station de Nançay (USN), Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Univers et Théories (LUTH (UMR_8102)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7), Laboratoire de physique subatomique et des technologies associées (SUBATECH), Université de Nantes - Faculté des Sciences et des Techniques, Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Galaxies, Etoiles, Physique, Instrumentation (GEPI), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO), Netherlands Institute for Radio Astronomy (ASTRON), Max-Planck-Institut für Radioastronomie (MPIFR), INAF - Osservatorio Astronomico di Cagliari (OAC), Istituto Nazionale di Astrofisica (INAF), Universität Bielefeld = Bielefeld University, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Rhodes University, Grahamstown, Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Université de Nantes (UN)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique (IMT Atlantique), Bondonneau, L, Griessmeier, J, Theureau, G, Cognard, I, Brionne, M, Kondratiev, V, Bilous, A, Mckee, J, Zarka, P, Viou, C, Guillemot, L, Chen, S, Main, R, Pilia, M, Possenti, A, Serylak, M, Shaifullah, G, Tiburzi, C, Verbiest, J, Wu, Z, Wucknitz, O, Yerin, S, Briand, C, Cecconi, B, Corbel, S, Dallier, R, Girard, J, Loh, A, Martin, L, Tagger, M, Tasse, C, Université d'Orléans (UO)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)
Subjects: Physics - Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics, 4/3, 01 natural sciences, frequency: high, Radio telescope, High Energy Physics - Phenomenology (hep-ph), Pulsar, Millisecond pulsar, Observatory, pulsars: general, 0103 physical sciences, site, Instrumentation (computer programming), structure, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010303 astronomy & astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), pulsar, Physics, radio wave, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], 010308 nuclear & particles physics, Crab Pulsar, Astrophysics::Instrumentation and Methods for Astrophysics, resolution, Astronomy and Astrophysics, LOFAR, Instrumentation and Detectors (physics.ins-det), sensitivity, coherence, observatory, High Energy Physics - Phenomenology, frequency: low, Space and Planetary Science, [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph], dispersion, methods: observational, Astrophysics - Instrumentation and Methods for Astrophysics, performance, Radio wave
Abstract: NenuFAR (New extension in Nan\c{c}ay upgrading LoFAR) is a new radio telescope developed and built on the site of the Nan\c{c}ay Radio Observatory. It is designed to observe the largely unexplored frequency window from 10 to 85\,MHz, offering a high sensitivity across its full bandwidth. NenuFAR has started its "early science" operation in July 2019, with 58\% of its final collecting area being available. Pulsars are one of the major topics for the scientific exploitation of this frequency range and represent an important challenge in terms of instrumentation. Designing instrumentation at these frequencies is complicated by the need to compensate for the effects of both the interstellar medium and the ionosphere on the observed signal. Our real-time pipeline LUPPI (Low frequency Ultimate Pulsar Processing Instrumentation) is able to cope with a high data rate and to provide real-time coherent de-dispersion down to the lowest frequencies reached by NenuFAR (10\,MHz). The full backend functionality is described, as well as the main pulsar observing modes (folded, single-pulse, waveform, and dynamic spectrum). This instrumentation allowed us to detect 172 pulsars in our first targeted search below 85\,MHz, including 10 millisecond pulsars (6 of which detected for the first time below 100 MHz). We also present some of the "early science" results of NenuFAR on pulsars: a high frequency resolution mapping of PSR B1919$+$21's emission profile and a detailed observation of single-pulse sub-structures from PSR~B0809$+$74 down to 16\,MHz, the high rate of giant-pulse emission from the Crab pulsar detected at 68.7\,MHz (43 events/min), and the illustration of the very good timing performance of the instrumentation, allowing us to study dispersion measure variations in great detail., Comment: 13 pages, 14 figures, submitted to A&A
Published: 2020
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7. Implicaciones de los datos paleomagnéticos sobre la edad de la Sierra de Chichinautzin, cuenca de México

Author: Jaime Urrutia-Fucugauchi and Ana Lilian Martin del Pozzo
Subjects: paleomagnetismo, estratigrafía volcánica, grupo chichinautzin, cuenca de méxico, cuaternario, Geophysics. Cosmic physics, QC801-809
Abstract: La polaridad geomagnética normal documentada para el Grupo Chichinautzin correlaciona con el Cron normal Brunhes de la Escala Geomagnética de Polaridades, lo que indica una edad más joven que 0.78-0.79 Ma. Para estimar la edad de inicio de la actividad y su distribución temporal y espacial se requiere sin embargo de estudios más detallados de carácter multidisciplinario (geocronológicos y de estratigrafía volcánica). Implicaciones sobre el cierre del drenaje y formación de la cuenca deben también de analizarse críticamente. Las unidades muestreadas provienen de la parte más joven (expuesta) de la Sierra (considerada probablemente como más joven de 40-60,000 años, dentro del rango de fechamiento por C-14) y por lo tanto no representa un muestreo sin sesgo representativo para el Grupo. Ello resalta la necesidad de contar con datos de muestras del subsuelo, así como de las secciones basales de la sierra. Resultados preliminares de la porción sureste de Chichinautzin (hacia el valle de Cuernavaca) indican polaridad reversa y por lo tanto sugieren que la actividad volcánica en la región podría haberse iniciado antes de 0.78-0.79 Ma (o bien durante un sub-cron dentro de Brunhes). Los datos disponibles no proporcionan información sobre el carácter continuo o discreto de la actividad. Los datos paleomagnéticos para el complejo volcánico del Ajusco indican polaridad reversa y normal y reversa, respectivamente, lo que sugiere que la actividad volcánica ocurrió en periodos transicionales y excursiones del campo geomagnético probablemente durante el Cron de Brunhes. doi: https://doi.org/10.22201/igeof.00167169p.1993.32.3.527
Published: 1993
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8. KM3NeT front-end and readout electronics system: hardware, firmware and software

Author: Sebastiano Aiello, Annarita Margiotta, Antonio Marinelli, Christos Markou, Gregory Martignac, Lilian Martin, Juan A. Martínez-Mora, Agnese Martini, Fabio Marzaioli, Safaa Mazzou, Rosa Mele, Karel W. Melis, Pasquale Migliozzi, Emilio Migneco, Piotr Mijakowski, Luis S. Miranda, Carlos M. Mollo, Mauro Morganti, Michael Moser, Abdelilah Moussa, Rasa Muller, Paolo Musico, Mario Musumeci, Lodewijk Nauta, Sergio Navas, Carlo A. Nicolau, Christine Nielsen, Brian Ó Fearraigh, Mukharbek Organokov, Angelo Orlando, Gogita Papalashvili, Riccardo Papaleo, Cosimo Pastore, Gabriela E. Păvălaş, Giuliano Pellegrini, Carmelo Pellegrino, Mathieu Perrin-Terrin, Paolo Piattelli, Camiel Pieterse, Konstantinos Pikounis, Ofelia Pisanti, Chiara Poirè, Georgia Polydefki, Vlad Popa, Maarten Post, Thierry Pradier, Gerd Pühlhofer, Sara Pulvirenti, Liam Quinn, Fabrizio Raffaelli, Nunzio Randazzo, Antonio Rapicavoli, Soebur Razzaque, Diego Real, Stefan Reck, Jonas Reubelt, Giorgio Riccobene, Marc Richer, Louis Rigalleau, Alberto Rovelli, Ilenia Salvadori, Dorothea F. E. Samtleben, Agustin Sánchez Losa, Matteo Sanguineti, Andrea Santangelo, Domenico Santonocito, Piera Sapienza, Jan-Willem Schmelling, Jutta Schnabel, Virginia Sciacca, Jordan Seneca, Irene Sgura, Rezo Shanidze, Ankur Sharma, Francesco Simeone, Anna Sinopoulou, Bernardino Spisso, Maurizio Spurio, Dimitris Stavropoulos, Jos Steijger, Simona M. Stellacci, Bruno Strandberg, Dominik Stransky, Mauro Taiuti, Yahya Tayalati, Enrique Tenllado, Tarak Thakore, Paul Timmer, Steven Tingay, Ekaterini Tzamariudaki, Dimitrios Tzanetatos, Veronique Van Elewyck, Federico Versari, Salvo Viola, Daniele Vivolo, Gwenhael de Wasseige, Joern Wilms, Rafał Wojaczyński, Els de Wolf, Dmitry Zaborov, Angela Zegarelli, Juan D. Zornoza, Juan Zúñiga, Vasilis Panagopoulos, Fabrizio Ameli, Michel Andre, Giorgos Androulakis, Marco Anghinolfi, Gisela Anton, Miquel Ardid, Julien Aublin, Christos Bagatelas, Giancarlo Barbarino, Bruny Baret, Suzan Basegmez du Pree, Anastasios Belias, Meriem Bendahman, Edward Berbee, Ad M. van den Berg, Vincent Bertin, Vincent van Beveren, Simone Biagi, Andrea Biagioni, Matthias Bissinger, Pascal Bos, Jihad Boumaaza, Simon Bourret, Mohammed Bouta, Gilles Bouvet, Mieke Bouwhuis, Cristiano Bozza, Horea Brânzaş, Max M. Briel, Marc Bruchner, Ronald Bruijn, Jurgen Brunner, Ernst-Jan Buis, Raffaele Buompane, Jose Busto, David Calvo, Antonio Capone, Silvia Celli, Mohamed Chabab, Nhan Chau, Silvio Cherubini, Vitaliano Chiarella, Tommaso Chiarusi, Marco Circella, Rosanna Cocimano, Joao A. B. Coelho, Alexis Coleiro, Marta C. Molla, Stephane Colonges, Rosa Coniglione, Paschal Coyle, Alexandre Creusot, Giacomo Cuttone, Antonio D’Amico, Antonio D’Onofrio, Richard Dallier, Mauro De Palma, Irene Di Palma, Antonio F. Díaz, Didac Diego-Tortosa, Carla Distefano, Alba Domi, Roberto Donà, Corinne Donzaud, Damien Dornic, Manuel Dörr, Mora Durocher, Thomas Eberl, Thijs van Eeden, Imad El Bojaddaini, Hassnae Eljarrari, Dominik Elsaesser, Alexander Enzenhöfer, Paolo Fermani, Giovanna Ferrara, Miroslav D. Filipović, Luigi A. Fusco, Deepak Gajanana, Tamas Gal, Alfonso Garcia Soto, Fabio Garufi, Lucio Gialanella, Emidio Giorgio, Sara R. Gozzini, Rodrigo Gracia, Kay Graf, Dario Grasso, Timothee Grégoire, Giuseppe Grella, Daniel Guderian, Carlo Guidi, Steffen Hallmann, Hassane Hamdaoui, Hans van Haren, Aart Heijboer, Amar Hekalo, Juan J. Hernández-Rey, Jannik Hofestädt, Feifei Huang, Enrique H. Santiago, Giulia Illuminati, Clancy W. James, Peter Jansweijer, Martijn Jongen, Maarten de Jong, Paul de Jong, Matthias Kadler, Piotr Kalaczyński, Oleg Kalekin, Uli F. Katz, Nafis R. Khan Chowdhury, Frits van der Knaap, Els N. Koffeman, Paul Kooijman, Antoine Kouchner, Michael Kreter, Vladimir Kulikovskiy, Robert Lahmann, Giuseppina Larosa, Remy Le Breton, Francesco Leone, Emanuele Leonora, Giuseppe Levi, Massimiliano Lincetto, Miles Lindsey Clark, Alessandro Lonardo, Fabio Longhitano, Daniel Lopez-Coto, Giuliano Maggi, Jerzy Mańczak, Karl Mannheim, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre de Physique des Particules de Marseille (CPPM), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Laboratoire de physique subatomique et des technologies associées (SUBATECH), Université de Nantes - Faculté des Sciences et des Techniques, Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Institut de Recherches Subatomiques (IReS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Cancéropôle du Grand Est-Centre National de la Recherche Scientifique (CNRS), Institut Universitaire de France (IUF), Ministère de l'Education nationale, de l’Enseignement supérieur et de la Recherche (M.E.N.E.S.R.), KM3NeT, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT)-Nantes université - UFR des Sciences et des Techniques (Nantes univ - UFR ST), Nantes Université - pôle Sciences et technologie, Nantes Université (Nantes Univ)-Nantes Université (Nantes Univ)-Nantes Université - pôle Sciences et technologie, Nantes Université (Nantes Univ)-Nantes Université (Nantes Univ), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Aiello, Sebastiano, Margiotta, Annarita, Marinelli, Antonio, Markou, Christo, Martignac, Gregory, Martin, Lilian, Martínez-Mora, Juan A., Martini, Agnese, Marzaioli, Fabio, Mazzou, Safaa, Mele, Rosa, Melis, Karel W., Migliozzi, Pasquale, Migneco, Emilio, Mijakowski, Piotr, Miranda, Luis S., Mollo, Carlos M., Morganti, Mauro, Moser, Michael, Moussa, Abdelilah, Muller, Rasa, Musico, Paolo, Musumeci, Mario, Nauta, Lodewijk, Navas, Sergio, Nicolau, Carlo A., Nielsen, Christine, Fearraigh, Brian Ó, Organokov, Mukharbek, Orlando, Angelo, Papalashvili, Gogita, Papaleo, Riccardo, Pastore, Cosimo, Păvălaş, Gabriela E., Pellegrini, Giuliano, Pellegrino, Carmelo, Perrin-Terrin, Mathieu, Piattelli, Paolo, Pieterse, Camiel, Pikounis, Konstantino, Pisanti, Ofelia, Poirè, Chiara, Polydefki, Georgia, Popa, Vlad, Post, Maarten, Pradier, Thierry, Pühlhofer, Gerd, Pulvirenti, Sara, Quinn, Liam, Raffaelli, Fabrizio, Randazzo, Nunzio, Rapicavoli, Antonio, Razzaque, Soebur, Real, Diego, Reck, Stefan, Reubelt, Jona, Riccobene, Giorgio, Richer, Marc, Rigalleau, Loui, Rovelli, Alberto, Salvadori, Ilenia, Samtleben, Dorothea F. E., Sánchez Losa, Agustin, Sanguineti, Matteo, Santangelo, Andrea, Santonocito, Domenico, Sapienza, Piera, Schmelling, Jan-Willem, Schnabel, Jutta, Sciacca, Virginia, Seneca, Jordan, Sgura, Irene, Shanidze, Rezo, Sharma, Ankur, Simeone, Francesco, Sinopoulou, Anna, Spisso, Bernardino, Spurio, Maurizio, Stavropoulos, Dimitri, Steijger, Jo, Stellacci, Simona M., Strandberg, Bruno, Stransky, Dominik, Taiuti, Mauro, Tayalati, Yahya, Tenllado, Enrique, Thakore, Tarak, Timmer, Paul, Tingay, Steven, Tzamariudaki, Ekaterini, Tzanetatos, Dimitrio, Van Elewyck, Veronique, Versari, Federico, Viola, Salvo, Vivolo, Daniele, de Wasseige, Gwenhael, Wilms, Joern, Wojaczyński, Rafał, de Wolf, El, Zaborov, Dmitry, Zegarelli, Angela, Zornoza, Juan D., Zúñiga, Juan, Panagopoulos, Vasili, Ameli, Fabrizio, Andre, Michel, Androulakis, Giorgo, Anghinolfi, Marco, Anton, Gisela, Ardid, Miquel, Aublin, Julien, Bagatelas, Christo, Barbarino, Giancarlo, Baret, Bruny, Basegmez du Pree, Suzan, Belias, Anastasio, Bendahman, Meriem, Berbee, Edward, van den Berg, Ad M., Bertin, Vincent, van Beveren, Vincent, Biagi, Simone, Biagioni, Andrea, Bissinger, Matthia, Bos, Pascal, Boumaaza, Jihad, Bourret, Simon, Bouta, Mohammed, Bouvet, Gille, Bouwhuis, Mieke, Bozza, Cristiano, Brânzaş, Horea, Briel, Max M., Bruchner, Marc, Bruijn, Ronald, Brunner, Jurgen, Buis, Ernst-Jan, Buompane, Raffaele, Busto, Jose, Calvo, David, Capone, Antonio, Celli, Silvia, Chabab, Mohamed, Chau, Nhan, Cherubini, Silvio, Chiarella, Vitaliano, Chiarusi, Tommaso, Circella, Marco, Cocimano, Rosanna, Coelho, Joao A. B., Coleiro, Alexi, Molla, Marta C., Colonges, Stephane, Coniglione, Rosa, Coyle, Paschal, Creusot, Alexandre, Cuttone, Giacomo, D’Amico, Antonio, D’Onofrio, Antonio, Dallier, Richard, De Palma, Mauro, Di Palma, Irene, Díaz, Antonio F., Diego-Tortosa, Didac, Distefano, Carla, Domi, Alba, Donà, Roberto, Donzaud, Corinne, Dornic, Damien, Dörr, Manuel, Durocher, Mora, Eberl, Thoma, van Eeden, Thij, El Bojaddaini, Imad, Eljarrari, Hassnae, Elsaesser, Dominik, Enzenhöfer, Alexander, Fermani, Paolo, Ferrara, Giovanna, Filipović, Miroslav D., Fusco, Luigi A., Gajanana, Deepak, Gal, Tama, Garcia Soto, Alfonso, Garufi, Fabio, Gialanella, Lucio, Giorgio, Emidio, Gozzini, Sara R., Gracia, Rodrigo, Graf, Kay, Grasso, Dario, Grégoire, Timothee, Grella, Giuseppe, Guderian, Daniel, Guidi, Carlo, Hallmann, Steffen, Hamdaoui, Hassane, van Haren, Han, Heijboer, Aart, Hekalo, Amar, Hernández-Rey, Juan J., Hofestädt, Jannik, Huang, Feifei, Santiago, Enrique H., Illuminati, Giulia, James, Clancy W., Jansweijer, Peter, Jongen, Martijn, de Jong, Maarten, de Jong, Paul, Kadler, Matthia, Kalaczyński, Piotr, Kalekin, Oleg, Katz, Uli F., Khan Chowdhury, Nafis R., van der Knaap, Frit, Koffeman, Els N., Kooijman, Paul, Kouchner, Antoine, Kreter, Michael, Kulikovskiy, Vladimir, Lahmann, Robert, Larosa, Giuseppina, Le Breton, Remy, Leone, Francesco, Leonora, Emanuele, Levi, Giuseppe, Lincetto, Massimiliano, Lindsey Clark, Mile, Lonardo, Alessandro, Longhitano, Fabio, Lopez-Coto, Daniel, Maggi, Giuliano, Mańczak, Jerzy, Mannheim, Karl, Centre Tecnològic de Vilanova i la Geltrú, Universitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques, Sebastiano Aiello, Fabrizio Ameli, Michel Andre, Giorgos Androulaki, Marco Anghinolfi, Gisela Anton, Miquel Ardid, Julien Aublin, Christos Bagatela, Giancarlo Barbarino, Bruny Baret, Suzan Basegmez du Pree, Anastasios Belia, Meriem Bendahman, Edward Berbee, Ad M. van den Berg, Vincent Bertin, Vincent van Beveren, Simone Biagi, Andrea Biagioni, Matthias Bissinger, Pascal Bo, Jihad Boumaaza, Simon Bourret, Mohammed Bouta, Gilles Bouvet, Mieke Bouwhui, Cristiano Bozza, Horea Brânza, Max M. Briel, Marc Bruchner, Ronald Bruijn, Jurgen Brunner, Ernst-Jan Bui, Raffaele Buompane, Jose Busto, David Calvo, Antonio Capone, Silvia Celli, Mohamed Chabab, Nhan Chau, Silvio Cherubini, Vitaliano Chiarella, Tommaso Chiarusi, Marco Circella, Rosanna Cocimano, Joao A. B. Coelho, Alexis Coleiro, Marta C. Molla, Stephane Colonge, Rosa Coniglione, Paschal Coyle, Alexandre Creusot, Giacomo Cuttone, Antonio D’Amico, Antonio D’Onofrio, Richard Dallier, Mauro De Palma, Irene Di Palma, Antonio F. Díaz, Didac Diego-Tortosa, Carla Distefano, Alba Domi, Roberto Donà, Corinne Donzaud, Damien Dornic, Manuel Dörr, Mora Durocher, Thomas Eberl, Thijs van Eeden, Imad El Bojaddaini, Hassnae Eljarrari, Dominik Elsaesser, Alexander Enzenhöfer, Paolo Fermani, Giovanna Ferrara, Miroslav D. Filipovic ́, Luigi A. Fusco, Deepak Gajanana, Tamas Gal, Alfonso Garcia Soto, Fabio Garufi, Lucio Gialanella, Emidio Giorgio, Sara R. Gozzini, Rodrigo Gracia, Kay Graf, Dario Grasso, Timothee Grégoire, Giuseppe Grella, Daniel Guderian, Carlo Guidi, Steffen Hallmann, Hassane Hamdaoui, Hans van Haren, Aart Heijboer, Amar Hekalo, Juan J. Hernández-Rey, Jannik Hofestädt, Feifei Huang, Enrique H. Santiago, Giulia Illuminati, Clancy W. Jame, Peter Jansweijer, Martijn Jongen, Maarten de Jong, Paul de Jong, Matthias Kadler, Piotr Kalaczynski, Oleg Kalekin, Uli F. Katz, Nafis R. Khan Chowdhury, Frits van der Knaap, Els N. Koffeman, Paul Kooijman, Antoine Kouchner, Michael Kreter, Vladimir Kulikovskiy, Robert Lahmann, Giuseppina Larosa, Remy Le Breton, Francesco Leone, Emanuele Leonora, Giuseppe Levi, Massimiliano Lincetto, Miles Lindsey Clark, Alessandro Lonardo, Fabio Longhitano, Daniel Lopez-Coto, Giuliano Maggi, Jerzy Ma ́nczak, Karl Mannheim, Annarita Margiotta, Antonio Marinelli, Christos Markou, Gregory Martignac, Lilian Martin, Juan A. Martínez-Mora, Agnese Martini, Fabio Marzaioli, Safaa Mazzou, Rosa MeleKarel W. Meli, Pasquale Migliozzi, Emilio Migneco, Piotr Mijakowski, Luis S. Miranda, Carlos M. Mollo, Mauro Morganti, Michael Moser, Abdelilah Moussa, Rasa Muller, Paolo Musico, Mario Musumeci, Lodewijk Nauta, Sergio Nava, Carlo A. Nicolau, Christine Nielsen, Brian Ó Fearraigh, Mukharbek Organokov, Angelo Orlando, Vasilis Panagopoulo, Gogita Papalashvili, Riccardo Papaleo, Cosimo Pastore, Gabriela E. Păvăla ̧, Giuliano Pellegrini, Carmelo Pellegrino, Mathieu Perrin-Terrin, Paolo Piattelli, Camiel Pieterse, Konstantinos Pikouni, Ofelia Pisanti, Chiara Poirè, Georgia Polydefki, Vlad Popa, Maarten Post, Thierry Pradier, Gerd Pühlhofer, Sara Pulvirenti, Liam Quinn, Fabrizio Raffaelli, Nunzio Randazzo, Antonio Rapicavoli, Soebur Razzaque, Diego Real, Stefan Reck, Jonas Reubelt, Giorgio Riccobene, Marc Richer, Louis Rigalleau, Alberto Rovelli, Ilenia Salvadori, Dorothea F. E. Samtleben, Agustin Sánchez Losa, Matteo Sanguineti, Andrea Santangelo, Domenico Santonocito, Piera Sapienza, Jan-Willem Schmelling, Jutta Schnabel, Virginia Sciacca, Jordan Seneca, Irene Sgura, Rezo Shanidze, Ankur Sharma, Francesco Simeone, Anna Sinopoulou, Bernardino Spisso, Maurizio Spurio, Dimitris Stavropoulo, Jos Steijger, Simona M. Stellacci, Bruno Strandberg, Dominik Stransky, Mauro Taiuti, Yahya Tayalati, Enrique Tenllado, Tarak Thakore, Paul Timmer, Steven Tingay, Ekaterini Tzamariudaki, Dimitrios Tzanetato, Veronique Van Elewyck, Federico Versari, Salvo Viola, Daniele Vivolo, Gwenhael de Wasseige, Joern Wilm, Rafał Wojaczy ́nski, Els de Wolf, Dmitry Zaborov, Angela Zegarelli, Juan D. Zornoza, Juan Zúñiga, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Ministerio de Economía y Competitividad (España), Ministerio de Ciencia, Innovación y Universidades (España), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université de Nantes (UN)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Research unit Astroparticle Physics, and 33379009 - Kreter, Michael
Subjects: Astrofísica, data acquisition, Computer science, Physics::Instrumentation and Detectors, readout electronics, sensors, Astrophysics, Neutrino telescope, computer.software_genre, 7. Clean energy, 01 natural sciences, Signal, Synchronization (alternating current), Front and back ends, Front-end electronics, readout electronics, neutrino telescope, KM3NeT, Front-end electronics, KM3NeT, Readout electronics, 010303 astronomy & astrophysics, Instrumentation, field programmable gate arrays, Firmware, electronics, 4. Education, Electrical engineering, Astrophysics::Instrumentation and Methods for Astrophysics, front-end electronics, Electronic, Optical and Magnetic Materials, Astrophysics - Instrumentation and Methods for Astrophysics, Photomultiplier, clocks, front-end electronic, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Partícules (Física nuclear), 010309 optics, 0103 physical sciences, Neutrins, readout electronic, 14. Life underwater, Electronics, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Instrumentation and Methods for Astrophysics (astro-ph.IM), Cherenkov radiation, Particles (Nuclear physics), Detectors òptics, logic, Optical detectors, Física [Àrees temàtiques de la UPC], Telescopis, business.industry, Mechanical Engineering, neutrino telescope, Astronomy and Astrophysics, Space and Planetary Science, Control and Systems Engineering, FISICA APLICADA, business, computer, Telescopes
Abstract: [EN] The KM3NeT research infrastructure being built at the bottom of the Mediterranean Sea will host water-Cherenkov telescopes for the detection of cosmic neutrinos. The neutrino telescopes will consist of large volume three-dimensional grids of optical modules to detect the Cherenkov light from charged particles produced by neutrino-induced interactions. Each optical module houses 31 3-in. photomultiplier tubes, instrumentation for calibration of the photomultiplier signal and positioning of the optical module, and all associated electronics boards. By design, the total electrical power consumption of an optical module has been capped at seven Watts. We present an overview of the front-end and readout electronics system inside the optical module, which has been designed for a 1-ns synchronization between the clocks of all optical modules in the grid during a life time of at least 20 years., The authors acknowledge financial support from the funding agencies: Agence Nationale de la Recherche (Grant No. ANR-15-CE31-0020), Centre National de la Recherche Scientifique (CNRS), Commission Europeenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), IdEx program and UnivEarthS Labex program at Sorbonne Paris Cite (Grant Nos. ANR-10-LABX-0023 and ANR-11-IDEX-0005-02), Paris Ile-de-France Region, France; Shota Rustaveli National Science Foundation of Georgia (SRNSFG, Grant No. FR-18-1268), Georgia; Deutsche Forschungsgemeinschaft (DFG), Germany; The General Secretariat of Research and Technology (GSRT), Greece; Istituto Nazionale di Fisica Nucleare (INFN), Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR), PRIN 2017 program (Grant NAT-NET 2017W4HA7S) Italy; Ministry of Higher Education, Scientific Research and Professional Training, Morocco; Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; The National Science Centre, Poland (2015/18/E/ST2/00758); National Authority for Scientific Research (ANCS), Romania; Plan Estatal de Investigacion [refs. FPA2015-65150-C3-1-P, -2-P and -3-P, (MINECO/FEDER)], Severo Ochoa Centre of Excellence program (MINECO), Red Consolider MultiDark (ref. FPA2017-90566-REDC, MINECO), and Prometeo and Grisolia programs (Generalitat Valenciana), "la Caixa" Foundation (ID 100010434) through the fellowship LCF/BQ/IN17/11620019, and the European Union's Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie Grant Agreement No. 713673, Spain.
Published: 2019
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9. Deep-sea deployment of the KM3NeT neutrino telescope detection units by self-unrolling

Author: Jose Busto, T. Hillebrand, Matthias Kadler, Piotr Kalaczyński, F. Garufi, T. Thakore, E. Tenllado, B. Baret, Joao A B Coelho, A. Cosquer, Mancia Anguita, L. Maderer, E. G. Anassontzis, Dominik Elsaesser, Y. Gatelet, Gennaro Miele, Alba Domi, D. Calvo, D. Lopez-Coto, Ornella Leonardi, V. Popa, Rosanna Cocimano, M. Mongelli, Emanuele Leonora, L. Nauta, Steffen Hallmann, Jutta Schnabel, Lucio Gialanella, J.D. Zornoza, S. Reck, E. Berbee, G. Pühlhofer, R. Wojaczyński, G. Ferrara, Steven Tingay, Robert Lahmann, Domenico Santonocito, Michael Moser, Giuseppina Larosa, R. Le Breton, R. Gracia, Matteo Sanguineti, F. Versari, A. Enzenhöfer, Mohamed Chabab, Natalia Zywucka, A. Marinelli, O. Kalekin, M. Billault, Alessia Capone, A. Creusot, M. Lindsey Clark, A. Sánchez Losa, R. Donà, H. Hamdaoui, O. Rabyang, P.M. Kooijman, M. De Palma, Tommaso Chiarusi, S. Alves Garre, A. W. Chen, Lilian Martin, Daniele Vivolo, M.C. Bouwhuis, Paolo Fermani, Matthias Bissinger, R. Bakker, G. Riccobene, Riccardo Papaleo, A. Grmek, S. Basegmez du Pree, Miroslav Filipovic, A. Martini, M. Ardid, Patrick Lamare, Daniele Zito, G. Androulakis, P. Migliozzi, Dídac Diego-Tortosa, S. Viola, Arnauld Albert, N. Chau, F. Huang, Soebur Razzaque, Sara Pulvirenti, C. Pellegrino, M. Bouta, C. Pastore, R. Coniglione, Damien Dornic, Jos Steijger, S. Colonges, S.F. Biagi, E. A. De Wolf, Paolo Sapienza, G. C. Barbarino, D. Muñoz Pérez, Silvio Cherubini, M. Circella, M. Bendahman, C. Bagatelas, S. Mazzou, Gisela Anton, P. Mijakowski, Annarita Margiotta, D. Tzanetatos, Giorgi Kistauri, Cristiano Bozza, Nicole Geisselbrecht, V. Bertin, D. Drouhin, Els Koffeman, Francesco Leone, J. Hofestädt, T. Gal, F. Filippini, Fabio Marzaioli, J. Zúñiga, F. Raffaelli, L. Caillat, Markus Boettcher, V. Espinosa, Richard Dallier, D. Guderian, J.A. Martínez-Mora, Alexis Coleiro, C. Distefano, Dario Grasso, Fabrizio Ameli, D. F. E. Samtleben, A. Hekalo, J. Schumann, M. de Jong, M. Morganti, Jihad Boumaaza, Emidio Giorgio, P. Coyle, I. Corredoira, I. Sgura, Antonio D'Onofrio, E. Tzamariudaki, Kay Graf, Karel Melis, Giacomo Cuttone, T. Lipreau, M. Taiuti, Vitaliano Chiarella, P. de Jong, D. Stavropoulos, C. Poirè, Michel André, Angelo Orlando, P. Piattelli, D. van Eijk, Carlos Maximiliano Mollo, Zineb Aly, Jörn Wilms, G. Cacopardo, Alin Ilioni, M. Perrin-Terrin, A. Rovelli, Barbara Caiffi, Abdelilah Moussa, A.M. van den Berg, V. Van Elewyck, J. Brunner, Carlo Alessandro Nicolau, F. van der Knaap, Luigi Antonio Fusco, Thierry Pradier, S. Rivoire, M. Laan, C. Markou, J. Seneca, U. Katz, Diego Real, S. R. Gozzini, C. D'Amato, Fabio Longhitano, H. Brânzaş, J. van Heerwaarden, C. Donzaud, Massimiliano Lincetto, Ofelia Pisanti, V. Carretero, M. Colomer Molla, Mario Musumeci, Michael Kreter, N. Randazzo, M. Anghinolfi, Maurizio Spurio, A.J. Heijboer, E. Migneco, I. El Bojaddaini, B. Spisso, M. Richer, S. Henry, L. S. Miranda, H. van Haren, Andrea Santangelo, A. Sinopoulou, Antoine Kouchner, Julien Aublin, G. Illuminati, A. Zegarelli, Sandra Zavatarelli, C. Pieterse, T. van Eeden, C. W. James, Mitchell O'Sullivan, Raffaele Buompane, Alice Paun, I. Di Palma, Antonio F. Díaz, Francesco Simeone, L. Gostiaux, Rezo Shanidze, M. Dörr, Paolo Castaldi, G. Vasileiadis, F. Salesa Greus, R. Bruijn, Silvia Celli, Thomas Eberl, A. Sharma, R. Muller, Bouke Jisse Jung, C. Guidi, K. Pikounis, Vladimir Kulikovskiy, J. Manczak, E. Buis, J.J. Hernández-Rey, Yahya Tayalati, Sebastiano Aiello, G. Grella, O. Gabella, Giuseppe Levi, G. Papalashvili, D. Tézier, G. de Wasseige, S. Sánchez Navas, Jerome Laurence, Karl Mannheim, Ahmed Eddyamoui, S. Mastroianni, M. Organokov, B. Ó Fearraigh, N. R. Khan Chowdhury, W. Idrissi Ibnsalih, Simona Maria Stellacci, G.E. Păvălaş, A. Garcia Soto, J. Palacios González, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Laboratoire de Mecanique des Fluides et d'Acoustique (LMFA), École Centrale de Lyon (ECL), Université de Lyon-Université de Lyon-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Institut National des Sciences Appliquées de Lyon (INSA Lyon), Université de Lyon-Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-Centre National de la Recherche Scientifique (CNRS), KM3NeT, ANR-18-IDEX-0001,Université de Paris,Université de Paris(2018), Centre Tecnològic de Vilanova i la Geltrú, Universitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques, Institut Pluridisciplinaire Hubert Curien (IPHC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Groupe de Recherche en Physique des Hautes Energies (GRPHE), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut Universitaire de Technologie de Colmar, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Laboratoire de physique subatomique et des technologies associées (SUBATECH), Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Laboratoire Univers et Particules de Montpellier (LUPM), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Institut Universitaire de France (IUF), Ministère de l'Education nationale, de l’Enseignement supérieur et de la Recherche (M.E.N.E.S.R.), Aiello S., Albert A., Alves Garre S., Aly Z., Ameli F., Anassontzis E.G., Andre M., Androulakis G., Anghinolfi M., Anguita M., Anton G., Ardid M., Aublin J., Bagatelas C., Bakker R., Barbarino G., Baret B., Basegmez du Pree S., Bendahman M., Berbee E., van den Berg A.M., Bertin V., Biagi S., Billault M., Bissinger M., Boettcher M., Boumaaza J., Bouta M., Bouwhuis M., Bozza C., Branzas H., Bruijn R., Brunner J., Buis E., Buompane R., Busto J., Cacopardo G., Caiffi B., Caillat L., Calvo D., Capone A., Carretero V., Castaldi P., Celli S., Chabab M., Chau N., Chen A., Cherubini S., Chiarella V., Chiarusi T., Circella M., Cocimano R., Coelho J.A.B., Coleiro A., Colomer Molla M., Colonges S., Coniglione R., Corredoira I., Cosquer A., Coyle P., Creusot A., Cuttone G., D'Amato C., D'Onofrio A., Dallier R., de Palma M., Di Palma I., Diaz A.F., Diego-Tortosa D., Distefano C., Domi A., Dona R., Donzaud C., Dornic D., Dorr M., Drouhin D., Eberl T., Eddyamoui A., van Eeden T., van Eijk D., El Bojaddaini I., Elsaesser D., Enzenhofer A., Espinosa V., Fermani P., Ferrara G., Filipovic M.D., Filippini F., Fusco L.A., Gabella O., Gal T., Garcia Soto A., Garufi F., Gatelet Y., Geisselbrecht N., Gialanella L., Giorgio E., Gostiaux L., Gozzini S.R., Gracia R., Graf K., Grasso D., Grella G., Grmek A., Guderian D., Guidi C., Hallmann S., Hamdaoui H., van Haren H., van Heerwaarden J., Heijboer A., Hekalo A., Henry S., Hernandez-Rey J.J., Hillebrand T., Hofestadt J., Huang F., Idrissi Ibnsalih W., Ilioni A., Illuminati G., James C.W., de Jong M., de Jong P., Jung B.J., Kadler M., Kalaczynski P., Kalekin O., Katz U.F., Khan Chowdhury N.R., Kistauri G., van der Knaap F., Koffeman E.N., Kooijman P., Kouchner A., Kreter M., Kulikovskiy V., Laan M., Lahmann R., Lamare P., Larosa G., Laurence J., Le Breton R., Leonardi O., Leone F., Leonora E., Levi G., Lincetto M., Lindsey Clark M., Lipreau T., Longhitano F., Lopez-Coto D., Maderer L., Manczak J., Mannheim K., Margiotta A., Marinelli A., Markou C., Martin L., Martinez-Mora J.A., Martini A., Marzaioli F., Mastroianni S., Mazzou S., Melis K.W., Miele G., Migliozzi P., Migneco E., Mijakowski P., Miranda L.S., Mollo C.M., Mongelli M., Morganti M., Moser M., Moussa A., Muller R., Munoz Perez D., Musumeci M., Nauta L., Navas S., Nicolau C.A., O Fearraigh B., O'Sullivan M., Organokov M., Orlando A., Palacios Gonzalez J., Papalashvili G., Papaleo R., Pastore C., Paun A.M., Pavalas G.E., Pellegrino C., Perrin-Terrin M., Piattelli P., Pieterse C., Pikounis K., Pisanti O., Poire C., Popa V., Pradier T., Puhlhofer G., Pulvirenti S., Rabyang O., Raffaelli F., Randazzo N., Razzaque S., Real D., Reck S., Riccobene G., Richer M., Rivoire S., Rovelli A., Salesa Greus F., Samtleben D.F.E., Sanchez Losa A., Sanguineti M., Santangelo A., Santonocito D., Sapienza P., Schnabel J., Schumann J., Seneca J., Sgura I., Shanidze R., Sharma A., Simeone F., Sinopoulou A., Spisso B., Spurio M., Stavropoulos D., Steijger J., Stellacci S.M., Taiuti M., Tayalati Y., Tenllado E., Tezier D., Thakore T., Tingay S., Tzamariudaki E., Tzanetatos D., van Elewyck V., Vasileiadis G., Versari F., Viola S., Vivolo D., de Wasseige G., Wilms J., Wojaczynski R., de Wolf E., Zavatarelli S., Zegarelli A., Zito D., Zornoza J.D., Zuniga J., Zywucka N., Aiello, S., Albert, A., Alves Garre, S., Aly, Z., Ameli, F., Anassontzis, E. G., Andre, M., Androulakis, G., Anghinolfi, M., Anguita, M., Anton, G., Ardid, M., Aublin, J., Bagatelas, C., Bakker, R., Barbarino, G., Baret, B., Basegmez du Pree, S., Bendahman, M., Berbee, E., van den Berg, A. M., Bertin, V., Biagi, S., Billault, M., Bissinger, M., Boettcher, M., Boumaaza, J., Bouta, M., Bouwhuis, M., Bozza, C., Branzas, H., Bruijn, R., Brunner, J., Buis, E., Buompane, R., Busto, J., Cacopardo, G., Caiffi, B., Caillat, L., Calvo, D., Capone, A., Carretero, V., Castaldi, P., Celli, S., Chabab, M., Chau, N., Chen, A., Cherubini, S., Chiarella, V., Chiarusi, T., Circella, M., Cocimano, R., Coelho, J. A. B., Coleiro, A., Colomer Molla, M., Colonges, S., Coniglione, R., Corredoira, I., Cosquer, A., Coyle, P., Creusot, A., Cuttone, G., D'Amato, C., D'Onofrio, A., Dallier, R., de Palma, M., Di Palma, I., Diaz, A. F., Diego-Tortosa, D., Distefano, C., Domi, A., Dona, R., Donzaud, C., Dornic, D., Dorr, M., Drouhin, D., Eberl, T., Eddyamoui, A., van Eeden, T., van Eijk, D., El Bojaddaini, I., Elsaesser, D., Enzenhofer, A., Espinosa, V., Fermani, P., Ferrara, G., Filipovic, M. D., Filippini, F., Fusco, L. A., Gabella, O., Gal, T., Garcia Soto, A., Garufi, F., Gatelet, Y., Geisselbrecht, N., Gialanella, L., Giorgio, E., Gostiaux, L., Gozzini, S. R., Gracia, R., Graf, K., Grasso, D., Grella, G., Grmek, A., Guderian, D., Guidi, C., Hallmann, S., Hamdaoui, H., van Haren, H., van Heerwaarden, J., Heijboer, A., Hekalo, A., Henry, S., Hernandez-Rey, J. J., Hillebrand, T., Hofestadt, J., Huang, F., Idrissi Ibnsalih, W., Ilioni, A., Illuminati, G., James, C. W., de Jong, M., de Jong, P., Jung, B. J., Kadler, M., Kalaczynski, P., Kalekin, O., Katz, U. F., Khan Chowdhury, N. R., Kistauri, G., van der Knaap, F., Koffeman, E. N., Kooijman, P., Kouchner, A., Kreter, M., Kulikovskiy, V., Laan, M., Lahmann, R., Lamare, P., Larosa, G., Laurence, J., Le Breton, R., Leonardi, O., Leone, F., Leonora, E., Levi, G., Lincetto, M., Lindsey Clark, M., Lipreau, T., Longhitano, F., Lopez-Coto, D., Maderer, L., Manczak, J., Mannheim, K., Margiotta, A., Marinelli, A., Markou, C., Martin, L., Martinez-Mora, J. A., Martini, A., Marzaioli, F., Mastroianni, S., Mazzou, S., Melis, K. W., Miele, G., Migliozzi, P., Migneco, E., Mijakowski, P., Miranda, L. S., Mollo, C. M., Mongelli, M., Morganti, M., Moser, M., Moussa, A., Muller, R., Munoz Perez, D., Musumeci, M., Nauta, L., Navas, S., Nicolau, C. A., O Fearraigh, B., O'Sullivan, M., Organokov, M., Orlando, A., Palacios Gonzalez, J., Papalashvili, G., Papaleo, R., Pastore, C., Paun, A. M., Pavalas, G. E., Pellegrino, C., Perrin-Terrin, M., Piattelli, P., Pieterse, C., Pikounis, K., Pisanti, O., Poire, C., Popa, V., Pradier, T., Puhlhofer, G., Pulvirenti, S., Rabyang, O., Raffaelli, F., Randazzo, N., Razzaque, S., Real, D., Reck, S., Riccobene, G., Richer, M., Rivoire, S., Rovelli, A., Salesa Greus, F., Samtleben, D. F. E., Sanchez Losa, A., Sanguineti, M., Santangelo, A., Santonocito, D., Sapienza, P., Schnabel, J., Schumann, J., Seneca, J., Sgura, I., Shanidze, R., Sharma, A., Simeone, F., Sinopoulou, A., Spisso, B., Spurio, M., Stavropoulos, D., Steijger, J., Stellacci, S. M., Taiuti, M., Tayalati, Y., Tenllado, E., Tezier, D., Thakore, T., Tingay, S., Tzamariudaki, E., Tzanetatos, D., van Elewyck, V., Vasileiadis, G., Versari, F., Viola, S., Vivolo, D., de Wasseige, G., Wilms, J., Wojaczynski, R., de Wolf, E., Zavatarelli, S., Zegarelli, A., Zito, D., Zornoza, J. D., Zuniga, J., Zywucka, N., Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université de Nantes (UN)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), KM3NeT (IHEF, IoP, FNWI), ATLAS (IHEF, IoP, FNWI), IoP (FNWI), and Research unit Astroparticle Physics
Subjects: Astrofísica, Overall mechanics design (support structures and materials, vibration analysis etc), Dispositius optoelectrònics, Física::Física de partícules [Àrees temàtiques de la UPC], cherenkov, Astrophysics, 01 natural sciences, String (physics), 030218 nuclear medicine & medical imaging, 0302 clinical medicine, Underwater, Special cables, Instrumentation, KM3NeT, Mathematical Physics, glass, 4. Education, charged particle, neutrino: detector, Neutrino detector, Cherenkov counters, Neutrino, Astrophysics - Instrumentation and Methods for Astrophysics, Optoelectrònica, Geology, Marine engineering, Cherenkov detector, sea, Cherenkov detectors, Manufacturing, tube, FOS: Physical sciences, Baikal, Physique [physics]/Physique [physics], Optoelectronic devides, 03 medical and health sciences, 0103 physical sciences, surface, 14. Life underwater, Neutrins, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Optoelectronics, detector: optical, copper: wire, Instrumentation and Methods for Astrophysics (astro-ph.IM), Cherenkov radiation, Detectors òptics, Optical detectors, ANTARES, Telescopis, 010308 nuclear & particles physics, Mooring, radiation: Cherenkov, vibration analysis etc), Overall mechanics design (support structures and materials, monitoring, astro-ph.IM, FISICA APLICADA, string, sphere, Telescopes
Abstract: KM3NeT is a research infrastructure being installed in the deep Mediterranean Sea. It will house a neutrino telescope comprising hundreds of networked moorings — detection units or strings — equipped with optical instrumentation to detect the Cherenkov radiation generated by charged particles from neutrino-induced collisions in its vicinity. In comparison to moorings typically used for oceanography, several key features of the KM3NeT string are different: the instrumentation is contained in transparent and thus unprotected glass spheres; two thin Dyneema® ropes are used as strength members; and a thin delicate backbone tube with fibre-optics and copper wires for data and power transmission, respectively, runs along the full length of the mooring. Also, compared to other neutrino telescopes such as ANTARES in the Mediterranean Sea and GVD in Lake Baikal, the KM3NeT strings are more slender to minimise the amount of material used for support of the optical sensors. Moreover, the rate of deploying a large number of strings in a period of a few years is unprecedented. For all these reasons, for the installation of the KM3NeT strings, a custom-made, fast deployment method was designed. Despite the length of several hundreds of metres, the slim design of the string allows it to be compacted into a small, re-usable spherical launching vehicle instead of deploying the mooring weight down from a surface vessel. After being lowered to the seafloor, the string unfurls to its full length with the buoyant launching vehicle rolling along the two ropes. The design of the vehicle, the loading with a string, and its underwater self-unrolling are detailed in this paper., French National Research Agency (ANR) ANR-15-CE31-0020, Centre National de la Recherche Scientifique (CNRS), European Union (EU), Institut Universitaire de France (IUF), LabEx UnivEarthS ANR-10-LABX-0023 ANR-18-IDEX-0001, Paris Ile-de-France Region, France, Shota Rustaveli National Science Foundation of Georgia (SRNSFG), Georgia FR-18-1268, German Research Foundation (DFG), Greek Ministry of Development-GSRT, Istituto Nazionale di Fisica Nucleare (INFN), Ministero dell'Universita e della Ricerca (MUR), PRIN Italy NAT-NET 2017W4HA7S, Ministry of Higher Education, Scientific Research and Professional Training, Morocco, Netherlands Organization for Scientific Research (NWO) Netherlands Government, National Science Center, Poland National Science Centre, Poland 2015/18/E/ST2/00758, National Authority for Scientific Research (ANCS), Romania, Ministerio de Ciencia, Innovación, Investigación y Universidades (MCIU): Programa Estatal de Generación de Conocimiento (MCIU/FEDER) PGC2018-096663-B-C41 PGC2018-096663-B-A-C42 PGC2018-096663-B-BC43 PGC2018-096663-B-B-C44, Severo Ochoa Centre of Excellence and MultiDark Consolider (MCIU), Junta de Andalucía SOMM17/6104/UGR, Generalitat Valenciana GRISOLIA/2018/119 CIDEGENT/2018/034, La Caixa Foundation LCF/BQ/IN17/11620019, EU: MSC program, Spain 713673
Published: 2020
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10. From the Observation of UHECR Radio Signal in [1-200] MHz to the Composition: CODALEMA and EXTASIS Status Report

Author: Alain Lecacheux, Didier Charrier, Lilian Martin, Richard Dallier, Antony Escudie, Benoît Revenu, Daniel García-Fernández, Laboratoire de physique subatomique et des technologies associées (SUBATECH), Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Observatoire de Paris, Université Paris sciences et lettres (PSL), CEA-Direction des Energies (ex-Direction de l'Energie Nucléaire) (CEA-DES (ex-DEN)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), CODALEMA/EXTASIS, Université de Nantes (UN)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique (IMT Atlantique), Unité Scientifique de la Station de Nançay (USN), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO), Observatoire de Paris - Site de Paris (OP), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)
Subjects: air, Cosmic ray, Radiation, Sudden death, 030218 nuclear medicine & medical imaging, 03 medical and health sciences, 0302 clinical medicine, Electric field, Calibration, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], activity report, Physics, radio wave, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astronomy, showers, calibration, mass dependence, electric field, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], cosmic radiation: primary, observatory, Air shower, quality, Antenna (radio), [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Energy (signal processing), on-line
Abstract: International audience; Over the years, significant efforts have been devoted to the understanding of the radio emission of extensive air shower (EAS) in the range [20-80] MHz but, despite some studies led until the nineties, the [1-10] MHz band has remained unused for nearly 30 years. The EXTASIS experiment, located within the radio astronomy observatory of Nançay and supported by the CO-DALEMA instrument, aims to reinvestigate the [1-10] MHz band, and to study the so-called "Sudden Death" contribution, the expected radiation electric field created by the particles that are stopped upon arrival to the ground. We present the instrumental setup and the results obtained with EXTASIS. Moreover, CODALEMA has demonstrated that in [20-80] MHz, the commonly used band, the electric field profile of extensive air showers is well understood, and contains all the information needed for the reconstruction of extensive air showers. An analysis pipeline was developed to set up an online reconstruction of the primary cosmic ray properties. Combining the antenna and acquisition system capabilities, CODALEMA extended the observation window up to 200 MHz, permitting to improve the quality of the reconstruction of the primary cosmic ray properties thanks to a fine calibration procedure. We present the results obtained on a large batch of cosmic ray events, notably a first estimate of their mass dependence with energy.
Published: 2019
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11. Exploration of the Potential of the Radio-Detection Technique for the Detection of High-Energy Gamma Rays

Author: Julien N. Girard, Jean-Mathias Grießmeier, Stephane Corbel, Alan Loh, Cedric Dumez-Viou, Laurent Denis, Antony Escudie, Richard Dallier, M. Pandey-Pommier, Philippe Zarka, L. Bondonneau, Didier Charrier, Daniel García-Fernández, Lilian Martin, A. Coffre, Leon Koopmans, Benoît Revenu, Laboratoire de physique subatomique et des technologies associées (SUBATECH), Université de Nantes - Faculté des Sciences et des Techniques, Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Unité Scientifique de la Station de Nançay (USN), Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Kapteyn Astronomical Institute [Groningen], University of Groningen [Groningen], Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), CODALEMA, Laboratoire d’Océanologie et de Géosciences (LOG) - UMR 8187 (LOG), Institut national des sciences de l'Univers (INSU - CNRS)-Université du Littoral Côte d'Opale (ULCO)-Université de Lille-Centre National de la Recherche Scientifique (CNRS), Département d'Astrophysique (ex SAP) (DAP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, CEA-Direction des Energies (ex-Direction de l'Energie Nucléaire) (CEA-DES (ex-DEN)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Centre de Recherche Astrophysique de Lyon (CRAL), École normale supérieure - Lyon (ENS Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université d'Orléans (UO)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Université de Nantes (UN)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique (IMT Atlantique), Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Subjects: Physics, High energy, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astrophysics::High Energy Astrophysical Phenomena, Gamma ray, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Direction of arrival, Cosmic ray, 7. Clean energy, Radio spectrum, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Radio telescope, Observatory, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Radio detection
Abstract: International audience; The radio detection of atmospheric particle showers initiated by ultra-high energy cosmic rays is today a proven technique that allows to reconstruct their properties (direction of arrival, energy, nature). Among the precursors of this method, the CODALEMA experiment installed at the Nançay radio-astronomy Observatory has contributed to several major technological innovations relevant for the radio detection technique (autonomous triggering, hybrid reconstruction, very wide frequency bands) and its high-performance antennas are also used on the NenuFAR radio telescope in Nançay. We propose to exploit the unique environment of the Nan\c cay Observatory through the CODALEMA experiment and the NenuFAR radio-telescope to explore the possibilities of radio-detection of atmospheric showers initiated by very high energy photons. The central idea is to phase a large set of antennas (several tens) in the direction of known sources emitting gamma (catalogs H.E.S.S., MAGIC, VERITAS, Fermi-LAT ...) to significantly increase the sensitivity of detection and to use the triggering capabilities on ultra fast transients controlled within the framework of CODALEMA. This would make it possible to observe the sources with a useful cycle close to 100 %. We present here the intended instrumental scheme as well as the expected signal level and some first results obtained on the observation of cosmic ray air showers with NenuFAR.
Published: 2019
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12. Electric field emitted by a particle track in two semi-infinite media

Author: Lilian Martin, Antony Escudie, Richard Dallier, Daniel García-Fernández, Benoît Revenu, Laboratoire de physique subatomique et des technologies associées (SUBATECH), Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Unité Scientifique de la Station de Nançay (USN), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO), Deutsches Elektronen-Synchrotron [Zeuthen] (DESY), Helmholtz-Gemeinschaft = Helmholtz Association, Erlangen Centre for Astroparticle Physics (ECAP), and Friedrich-Alexander Universität Erlangen-Nürnberg (FAU)
Subjects: Physics, Field (physics), [PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th], Astrophysics::High Energy Astrophysical Phenomena, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Detector, Boundary (topology), Cosmic ray, Charged particle, Computational physics, Air shower, [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph], Electric field, Particle, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: International audience; The radio technique for the detection of cosmic rays is nowadays a well-established experimental technique, and several projects intend to adapt it for the detection of neutrinos. When a primary particle interacts with a target particle in a medium, a shower containing electrically charged particles is created, and an electric field is emitted. The measurement and analysis of this electric field can reveal the properties of the primary particle. In order to be able to produce an accurate reconstruction of the properties of the primary particle, a reliable calculation of the electric field is needed. Although almost every current radio detection experiment is located near a boundary (e.g. ground), the effect of this boundary on the calculation of the electric field is either not taken into account or the field is decomposed into direct, reflected and transmitted components, which is a correct description in the far-field approximation only. When the emitting shower and the detector are close to the boundary with respect to the observation wavelength, this approximation breaks down, as it is the case for the EXTASIS experiment when the particles are near ground level. We present in this work a frequency-domain calculation of the electric field from a charged particle track lying in two semi-infinite media separated by a planar boundary. We also give an estimate of the expected signal from a full air shower using a toy model.
Published: 2019
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13. Influence of a planar boundary on the electric field emitted by a particle shower

Author: Lilian Martin, Antony Escudie, D. García-Fernández, Benoît Revenu, Laboratoire de physique subatomique et des technologies associées (SUBATECH), Université de Nantes - Faculté des Sciences et des Techniques, Université de Nantes (UN)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Unité Scientifique de la Station de Nançay (USN), Université d'Orléans (UO)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)
Subjects: Field (physics), air, Astrophysics::High Energy Astrophysical Phenomena, ice, pole, FOS: Physical sciences, Context (language use), Cosmic ray, 01 natural sciences, Particle shower, Electric field, 0103 physical sciences, 010306 general physics, Monte Carlo, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, radio wave, showers: atmosphere, 010308 nuclear & particles physics, tracks, Computational physics, electric field, cosmic radiation: primary, Air shower, frequency: low, [SDU]Sciences of the Universe [physics], interface, Antenna (radio), Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Radio wave, Astrophysics and astroparticle physics
Abstract: International audience; The radio detection of cosmic rays consists in the estimation of the properties of a primary cosmic ray by observing the electric field emitted by the extensive air shower (EAS) created when the primary cosmic ray enters the atmosphere. This technique is fully operative nowadays and presents a good degree of maturity. In addition, several projects intend to employ this technique for the detection of neutrinos. In order for the technique to be useful, accurate methods for computing the electric field created by a particle shower in the context of a particular experiment must exist. Although current ground-based radio experiments lie on the air-soil interface and some planned experiments on the South Pole envision antennas near the air-ice interface, most of the analytical approaches and Monte Carlo codes used for calculating the electric field either do not take into account the effect of the boundary or calculate the radiation fields only (direct, reflected and transmitted radiation fields). When the particle shower and the antenna are close to the boundary, compared to the observation wavelength, the far-field approximation breaks down, which is the case for the low-frequency EXTASIS experiment, for instance. We present in this work a new formula for calculating the exact field emitted by a particle track in two semi-infinite media separated by a planar boundary. We also explore the validity of the far-field approximation and make some predictions for EAS using a simple shower model.
Published: 2019
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14. Multi-wavelength observation of cosmic-ray air-showers with CODALEMA/EXTASIS

Author: Benoît Revenu, Richard Dallier, Daniel García-Fernández, Didier Charrier, Antony Escudie, Alain Lecacheux, Lilian Martin, Laboratoire de physique subatomique et des technologies associées (SUBATECH), Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Unité Scientifique de la Station de Nançay (USN), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO), Observatoire de Paris - Site de Meudon (OBSPM), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Université de Nantes - Faculté des Sciences et des Techniques, Université de Nantes (UN)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Université d'Orléans (UO)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), and PSL Research University (PSL)-PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Frequency band, air, QC1-999, FOS: Physical sciences, Cosmic ray, Astrophysics, 01 natural sciences, Sudden death, Observatory, Electric field, 0103 physical sciences, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, electric field: high, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, radio wave, showers: atmosphere, 010308 nuclear & particles physics, electric field: atmosphere, observatory, cosmic radiation: primary, Air shower, Amplitude, frequency, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Radio wave
Abstract: Since 2003, significant efforts have been devoted to the understanding of the radio emission of extensive air shower in the range [20-200] MHz. Despite some studies led until the early nineties, the [1-10] MHz band has remained unused for 20 years. However, it has been measured by some pioneering experiments that extensive air shower emit a strong electric field in this band and that there is evidence of a large increase in the amplitude of the radio pulse at lower frequencies. The EXTASIS experiment, located within the Nan\c{c}ay Radioastronomy Observatory and supported by the CODALEMA experiment, aims to reinvestigate the [1-10] MHz band, and especially to study the so-called "Sudden Death" contribution, the expected electric field emitted by shower front when hitting the ground level. Currently, EXTASIS has confirmed some results obtained by the pioneering experiments, and tends to bring explanations to the other ones, for instance the role of the underlying atmospheric electric field. Moreover, CODALEMA has demonstrated that in the most commonly used frequency band ([20-80] MHz) the electric field profile of EAS can be well sampled, and contains all the information needed for the reconstruction of EAS: an automatic comparison between the SELFAS3 simulations and data has been developed, allowing us to reconstruct in an almost real time the primary cosmic ray characteristics., Comment: arXiv admin note: substantial text overlap with arXiv:1903.02792; text overlap with arXiv:1903.02889
Published: 2018
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15. Computing the electric field from Extensive Air Showers using a realistic description of the atmosphere

Author: Lilian Martin, Benoît Revenu, F. Gaté, V. Marin, Richard Dallier, Daniel García-Fernández, A. Escudié, Laboratoire de physique subatomique et des technologies associées (SUBATECH), Université de Nantes - Faculté des Sciences et des Techniques, Université de Nantes (UN)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Unité Scientifique de la Station de Nançay (USN), Université d'Orléans (UO)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)
Subjects: atmosphere: model, Field (physics), air, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, Atmospheric model, 01 natural sciences, Secondary electrons, Atmosphere, Radio signal, Electric field, positron: secondary, 0103 physical sciences, Extensive air showers, cosmic radiation: UHE, 010306 general physics, Cosmic rays, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Range (particle radiation), radio wave, showers: atmosphere, 010308 nuclear & particles physics, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, electron: secondary, GDAS, Computational physics, electric field, cosmic radiation: primary, 85-08, 13. Climate action, Duty cycle, Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Energy (signal processing), Radio wave
Abstract: The composition of ultra-high energy cosmic rays is still poorly known and constitutes a very important topic in the field of high-energy astrophysics. Detection of ultra-high energy cosmic rays is carried out via the extensive air showers they create after interacting with the atmosphere constituents. The secondary electrons and positrons within the showers emit a detectable electric field in the kHz-GHz range. It is possible to use this radio signal for the estimation of the atmospheric depth of maximal development of the showers \xmax, with a good accuracy and a duty cycle close to $100\%$. This value of \xmax\ is strongly correlated to the nature of the primary cosmic ray that initiated the shower. We show in this paper the importance of using a realistic atmospheric model in order to correct for systematic errors that can prevent a correct and unbiased estimation of~\xmax., Comment: 36 pages, 18 figures
Published: 2018
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16. Calculations of low-frequency radio emission by cosmic ray-induced particle showers

Author: D. García-Fernández, Antony Escudie, Benoît Revenu, Lilian Martin, Richard Dallier, Didier Charrier, Laboratoire de physique subatomique et des technologies associées (SUBATECH), Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Unité Scientifique de la Station de Nançay (USN), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO), Université de Nantes - Faculté des Sciences et des Techniques, Université d'Orléans (UO)-Observatoire des Sciences de l'Univers en région Centre (OSUC), PSL Research University (PSL)-PSL Research University (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Astrophysics::High Energy Astrophysical Phenomena, cosmic radiation: energy, FOS: Physical sciences, Cosmic ray, Dielectric, Low frequency, 01 natural sciences, Sudden death, Electric field, Askaryan radio emission, 0103 physical sciences, extensive air showers, 010306 general physics, dielectric, Monte Carlo, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, radio wave, energy: high, high energy cosmic rays, showers: atmosphere, 010308 nuclear & particles physics, deceleration, tracks, 3. Good health, Computational physics, electric field, coherence, cosmic radiation: primary, Air shower, Classical mechanics, frequency: low, Transition radiation, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - High Energy Astrophysical Phenomena, Radio wave
Abstract: The radio technique for the detection of high energy cosmic rays consists in measuring the electric field created by the particle showers created inside a medium by the primary cosmic ray. The electric field is then used to infer the properties of the primary particle. Nowadays, the radio technique is a standard, well-established technique. While most current experiments measure the field at frequencies above $20$ MHz, several experiments have reported a large emission at low frequencies, below $10$ MHz. The EXTASIS experiment aims at measuring again and understand this low-frequency electric field. Since at low frequencies the standard far-field approximation for the calculation of the electric field does not necessarily hold, in order to comprehend the low-frequency emission we need to go beyond the far-field approximation. We present in this work a formula for the electric field created by a particle track inside a dielectric medium that is valid for all frequencies. We then implement this formula in the SELFAS Monte Carlo code and calculate the low-frequency electric field of EAS. We also introduce the sudden death pulse (SDP), an emission caused by the coherent deceleration of the shower front, and study its properties., 42 pages, 18 figures
Published: 2017
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17. On timing accuracy in observing radio impulses associated with Extensive Air Showers

Author: Benoît Revenu, Daniel García-Fernández, Richard Dallier, Alain Lecacheux, Didier Charrier, Antony Escudie, Lilian Martin, Observatoire de Paris - Site de Meudon (OBSPM), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de physique subatomique et des technologies associées (SUBATECH), Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), PSL Research University (PSL)-PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Université de Nantes - Faculté des Sciences et des Techniques, and Université de Nantes (UN)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique)
Subjects: Wavefront, Physics, air, detector: surface, 010308 nuclear & particles physics, Plane (geometry), Detector, trigger, showers, Radius, radio wave: detector, Geodesy, Curvature, 01 natural sciences, Signal, Core (optical fiber), curvature, atmosphere, 0103 physical sciences, Range (statistics), [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], 010306 general physics
Abstract: International audience; A large subset of EAS radio observations by CODALEMA experiment in Nançay was used to measure the departure from a plane of the signal arrival times to the antennas. The study was done at two different scales in terms of range to the EAS axis. Below about 300m, by using a 10 antennas array triggered by neighbouring surface detectors, the average departure was found to be negligible (i.e. lower than the measurement incertitude of about 2-3 ns), leading to an equivalent "wave front curvature" radius larger than 30 km. Above the 300m range, and within the first kilometre, an extended array of several tens of self-triggered antennas was used. The measurements suggest the existence of significant time departures (of order 10 ns at 1 km range), which corresponds to an apparent curvature radius much larger than the atmosphere thickness. The main limitation of the method, in addition to the inferior time precision due to self-triggering, was the lack of accurate knowledge of corresponding EAS core locations, especially when those cores are located well outside the surface detector extent.
Published: 2017
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18. Direct measurement of the vertical component of the electric field from EAS

Author: Richard Dallier, Daniel García-Fernández, Benoît Revenu, Laurent Denis, Antony Escudie, Alain Lecacheux, Lilian Martin, Didier Charrier, Hervé Carduner, Laboratoire de physique subatomique et des technologies associées (SUBATECH), Université de Nantes - Faculté des Sciences et des Techniques, Université de Nantes (UN)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Unité Scientifique de la Station de Nançay (USN), Université d'Orléans (UO)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Observatoire de Paris - Site de Paris (OP), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS), Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Physics, 010308 nuclear & particles physics, business.industry, Astrophysics::Instrumentation and Methods for Astrophysics, Measure (physics), Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Particle detector, Optics, Air shower, Electric field, Component (UML), 0103 physical sciences, Antenna (radio), [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], 010306 general physics, business, Physics::Atmospheric and Oceanic Physics, Radio detection
Abstract: International audience; A three-fold antenna system has been installed nearby the center of the CODALEMA particle detector. Its goal is to measure the complete electric field produced by air showers, i.e. along the 3 polarizations East-West (EW), North-South (NS) and vertical. Indeed on all currently operating radio detection arrays, only the horizontal NS and EW polarizations or their projections are measured. This allows the vertical electric field component to be reconstructed, provided that the far-field assumption is valid, but though strong hints based on the theories of air shower radio emission tend to validate this hypothesis, it has never been verified experimentally. We present the 3D antenna and its acquisition system, and the first results obtained.
Published: 2017
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19. Near-field radio emission induced by extensive air showers

Author: Alain Lecacheux, Richard Dallier, Benoît Revenu, Lilian Martin, Didier Charrier, Daniel García Fernández, M. Tueros, Antony Escudie, Laboratoire de physique subatomique et des technologies associées (SUBATECH), Université de Nantes - Faculté des Sciences et des Techniques, Université de Nantes (UN)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Unité Scientifique de la Station de Nançay (USN), Université d'Orléans (UO)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Observatoire de Paris - Site de Meudon (OBSPM), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Physics, Work (thermodynamics), Field (physics), Monte carlo code, Electric field, Radio signal, Particle, Near and far field, Low frequency, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Computational physics
Abstract: International audience; The measurement of the electric field created by cosmic-ray induced air showers is nowadays a well-established technique. Due to technical limitations, the low-end part of the frequency spec- trum of the field has not been thoroughly exploited or understood, even though some experiments have indicated a large electric field at low frequencies. In this work, we present a new equation for the electric field of a particle track in time-domain valid for all frequencies, and therefore suited for the treatment of the near-field regime. After that, we calculate the low frequency radio signal of extensive air showers in the far-field and near-field regimes using a new version of the SELFAS Monte Carlo code that includes our equation.
Published: 2017
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20. Low frequency observations of cosmic ray air shower radio emission by CODALEMA/EXTASIS

Author: Antony Escudie, Richard Dallier, Alain Lecacheux, Benoît Revenu, Daniel García-Fernández, Lilian Martin, Didier Charrier, Laboratoire de physique subatomique et des technologies associées (SUBATECH), Université de Nantes - Faculté des Sciences et des Techniques, Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Unité Scientifique de la Station de Nançay (USN), Université d'Orléans (UO)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Observatoire de Paris - Site de Meudon (OBSPM), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Université de Nantes (UN)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT), Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Laboratoire SUBATECH Nantes (SUBATECH), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Mines Nantes (Mines Nantes), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Physics, [PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th], 010308 nuclear & particles physics, Astronomy, Cosmic ray, Low frequency, Radiation, 01 natural sciences, Radio astronomy observatory, Sudden death, Amplitude, Air shower, [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph], Electric field, 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], 010306 general physics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: International audience; Over the years, significant efforts have been devoted to the understanding of the radio emission of extensive air shower (EAS) in the range [20-200] MHz. Despite some studies led until the early nineties, the [1-10] MHz band has remained unused for 20 years. However, it has been measured by these pioneering experiments and suggested by theoretical calculations that EAS emit a strong electric field in this band and that there is evidence of a large increase in the amplitude of the radio pulse at lower frequencies. The EXTASIS project, located within the radio astronomy observatory of Nançay and supported by the CODALEMA instrument, aims to study the [1-10] MHz band, and especially the so-called "Sudden Death" contribution, the expected radiation electric field created by the particles that are stopped upon arrival to the ground. We present our instrumental setup, the objectives of the EXTASIS project and our first results.
Published: 2017
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21. Main features of cosmic ray induced air showers measured by the CODALEMA experiment

Author: Lilian Martin, Florian Gaté, Antony Escudie, Richard Dallier, Benoît Revenu, Daniel García-Fernández, Alain Lecacheux, Laboratoire de physique subatomique et des technologies associées (SUBATECH), Université de Nantes - Faculté des Sciences et des Techniques, Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Unité Scientifique de la Station de Nançay (USN), Université d'Orléans (UO)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), and Université de Nantes (UN)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique)
Subjects: air, Astrophysics::High Energy Astrophysical Phenomena, cosmic radiation: energy, Cosmic ray, Astrophysics, 01 natural sciences, Radio observatory, Observatory, 0103 physical sciences, Wide band, Ultra-high-energy cosmic ray, 010303 astronomy & astrophysics, Physics, energy: high, radio wave, polarization, showers: atmosphere, 010308 nuclear & particles physics, Astrophysics::Instrumentation and Methods for Astrophysics, Polarization (waves), sensitivity, observatory, cosmic radiation: primary, Dual-polarization interferometry, duality, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Radio wave
Abstract: International audience; The radio signals produced by extensive air showers initiated in the atmosphere by high energy cosmic rays are routinely observed and registered by the various instruments of the CODALEMA experiment located at the Nançay radio observatory and notably by the large array of self-triggering stations equipped with wide band and dual polarization antennas. Precise comparisons between observed radio signals and simulations performed with the SELFAS code allow most of the main features of the primary cosmic ray to be determined: arrival direction, energy and $X_{max}$ estimates from which a the composition in the energy range covered by CODALEMA may be derived. After a presentation of the analysis methods, its sensitivity will be discussed and the results obtained over a significant set of experimental events will be detailed.
Published: 2017
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22. Erratum: Global polarization measurement in Au + Au collisions [Phys. Rev. C 76 , 024915 (2007)]

Author: SUDHIR BHARDWAJ, Lee Barnby, Thomas Peitzmann, Lilian Martin, Sonia Kabana, Adam Kisiel, and Jun Takahashi
Subjects: Physics, 010308 nuclear & particles physics, 0103 physical sciences, Atomic physics, 010306 general physics, Polarization (waves), 01 natural sciences
Published: 2017
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23. Investigating the extensive air shower properties: Tackling the challenges of the next generation cosmic ray observatory with the CODALEMA experiment

Author: Lilian Martin, Unité Scientifique de la Station de Nançay (USN), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO), Laboratoire SUBATECH Nantes (SUBATECH), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), and ROUCHON, Nathalie
Subjects: Physics, Nuclear and High Energy Physics, Scope (project management), Cosmic ray, Astrophysics, 7. Clean energy, [SDU] Sciences of the Universe [physics], Time line, Upgrade, Air shower, [SDU]Sciences of the Universe [physics], 13. Climate action, Observatory, Systems engineering, Extensive air showers, Radio detection, Cosmic-ray observatory, Cosmic rays, Instrumentation
Abstract: Conférence; International audience; Our knowledge on ultra-high energy cosmic rays and their underlying sources and acceleration mechanisms is steadily improving thanks to the large observatories nowadays in operation. However the need for a next generation instrument is emerging from their experimental limitations and the scientific questions currently out of reach within a reasonable time line. Within this scope, the main features of the radio detection of extensive air showers are investigated and confronted to these challenging requirements. CODALEMA is the last experiment currently running in Europe dedicated to the cosmic ray detection using the observation of its induced radio electric field. The latest experimental upgrade and the synthesis of its operation features and the upcoming technical developments are presented. The main results of CODALEMA will be presented with special emphasis put on some of the new aspects of the data analysis offered by the CODALEMA3 autonomous station array. Finally, the opportunities provided by the Nancay observatory for efficient R&D activities and especially the upcoming technical developments are listed. (C) 2013 Elsevier B.V. All rights reserved.
Published: 2014
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24. Volcán de Colima

Author: Ana Lilian Martin del Pozzo
Subjects: volcán colima, geología, geofísica, Geophysics. Cosmic physics, QC801-809
Abstract: Volcán Colima is currently one of the most dangerous volcanoes in Mexico. It presents hazards at various scales. It has a history of frequent eruptions during the past 450 years, for which there are written records. To better understand the nature of the volcano and predict its future activity, the level of scientific investigation has greatly increased in recent years. The articles in this volume summarize current information on a variety of topics related to the geology and geophysics of the Colima. They vere assembled as part of a co-operative scientific project to analyze and mitigate the risk at this volcano.
Published: 1993
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25. Reconstruction of the parameters of cosmic ray induced extensive air showers using radio detection and simulation

Author: Lilian Martin, Benoît Revenu, Richard Dallier, and Florian Gaté
Subjects: Physics, Photon, Air shower, Astrophysics::High Energy Astrophysical Phenomena, Detector, Cosmic ray, Context (language use), Electron, Scintillator, Charged particle, Computational physics
Abstract: Cosmic rays have a wide energy spectrum and their flux decreases quickly with the energy. For the most energetic events (above 10 17 eV), the mass composition is not well known, due to shower to shower fluctuations. The knowledge of the mass composition would allow us to constrain theoretical models which predict different types of source and acceleration mechanism according to the mass of the particle. The only way to study such rare events is to observe the extensive air shower (EAS), composed of the secondary particles produced in the atmosphere after the interaction between the primary cosmic ray and the atmosphere’s constituents. The EAS is mainly composed of electrons, positrons and photons. Different ways of detection exist to determine the EAS parameters. The fluorescence detectors receive the light emitted by the atmosphere constituents after being excited by the EAS charged particles. Cerenkov tanks and plastic scintillators sample the particles on the ground. Radio antennas record the electric field emitted by the electrons and positrons of the shower. These detection methods are able to reconstruct some of the EAS parameters such as the energy of the primary particle, its arrival direction, the EAS core position on the ground and the atmospheric depth at which the number of particles is maximum (Xmax). The radio signal is now quite well understood and its description via the simulation is successful. In this context, the reconstruction method described in this contribution is based on a detailed comparison between the simulated radio footprint and the one sampled by an array of antennas. The method is sensitive to the Xmax value which is strongly correlated to the primary mass. We finally show how the radio detection is able to reconstruct all the EAS parameters on its own.
Published: 2016
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26. Ultimate precision in cosmic-ray radio detection — the SKA

Author: Tobias Winchen, Richard Dallier, David Butler, Frank G. Schröder, Lilian Martin, Stijn Buitink, K. Mulrey, Anne Zilles, Benoît Revenu, Tim Huege, Heino Falcke, Torsten A. Enßlin, Steven Tingay, Andreas Haungs, C. W. James, Anna Nelles, Pragati Mitra, Ronald D. Ekers, Justin D. Bray, Olaf Scholten, Laboratoire de physique subatomique et des technologies associées (SUBATECH), Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Unité Scientifique de la Station de Nançay (USN), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO), Université de Nantes - Faculté des Sciences et des Techniques, Université d'Orléans (UO)-Observatoire des Sciences de l'Univers en région Centre (OSUC), PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Université de Nantes (UN)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Research unit Astroparticle Physics, Laboratoire de physique subatomique et des technologies associées ( SUBATECH ), IMT Atlantique Bretagne-Pays de la Loire ( IMT Atlantique ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ) -Université de Nantes ( UN ), Unité Scientifique de la Station de Nançay ( USN ), Institut national des sciences de l'Univers ( INSU - CNRS ) -Observatoire de Paris-Université d'Orléans ( UO ) -Centre National de la Recherche Scientifique ( CNRS ), Physics, and Astronomy and Astrophysics Research Group
Subjects: air, QC1-999, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, engineering, FOS: Physical sciences, Cosmic ray, Physics and Astronomy(all), 01 natural sciences, 7. Clean energy, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), [ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex], Observatory, 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Instrumentation and Methods for Astrophysics (astro-ph.IM), [ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010303 astronomy & astrophysics, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries), High Energy Astrophysical Phenomena (astro-ph.HE), Physics, density, radio wave, showers: atmosphere, 010308 nuclear & particles physics, Astrophysics::Instrumentation and Methods for Astrophysics, resolution, observatory, Square kilometre array, Homogeneous, cosmic radiation, Antenna (radio), Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Radio detection, Energy (signal processing), on-line
Abstract: As of 2023, the low-frequency part of the Square Kilometre Array will go online in Australia. It will constitute the largest and most powerful low-frequency radio-astronomical observatory to date, and will facilitate a rich science programme in astronomy and astrophysics. With modest engineering changes, it will also be able to measure cosmic rays via the radio emission from extensive air showers. The extreme antenna density and the homogeneous coverage provided by more than 60,000 antennas within an area of one km$^2$ will push radio detection of cosmic rays in the energy range around 10$^{17}$ eV to ultimate precision, with superior capabilities in the reconstruction of arrival direction, energy, and an expected depth-of-shower-maximum resolution of 6~g/cm${^2}$., To be published in the Proceedings of the ARENA2016 conference, Groningen, The Netherlands; replaced with final published version in v3
Published: 2016
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27. Recent results from CODALEMA and the Nançay radio facilities related to cosmic-ray measurements

Author: Richard Dallier, Alain Lecacheux, Antony Escudie, Didier Charrier, Florian Gaté, Lilian Martin, L. Denis, Benoît Revenu, Laboratoire SUBATECH Nantes (SUBATECH), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Unité Scientifique de la Station de Nançay (USN), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Région Pays de la Loire, Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Physics, 010308 nuclear & particles physics, Frequency band, QC1-999, Cosmic ray, Astrophysics, 01 natural sciences, Signal, Radio observatory, Air shower, Nançay Observatory, Radiodetection of cosmic ray air showers, [SDU]Sciences of the Universe [physics], Electric field, Radio signal, 0103 physical sciences, Antenna (radio), [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], 010303 astronomy & astrophysics, EXTASIS, Codalema
Abstract: International audience; Since 2003, the Nançay Radio Observatory hosts the CODALEMA experiment, dedicated to radio detection of cosmic ray induced extensive air showers. CODALEMA also features the R&D EXTASIS project, aiming at detecting the low- frequency signal ([2-6] MHz) produced at the sudden disappearance of the air shower particles hitting the ground. The 3 current antenna arrays present different antenna den- sity and extent, and can be operated in a joint mode to record simultaneously the radio signal coming from air showers. Therefore, the Nançay facilities may offer a complete description of the air shower induced electric field at small, medium and large scale, and over an unique and very wide frequency band (from ∼ 2 to 200 MHz).
Published: 2016
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28. A dedicated antenna array for radio detection of Extended Air Showers

Author: Lecacheux, A., Didier Charrier, Richard Dallier, Loic Denis, Lilian Martin, Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire SUBATECH Nantes (SUBATECH), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Unité Scientifique de la Station de Nançay (USN), Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO), and Dallier, Richard
Subjects: cosmic rays, codalema, [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph], compact array, antennas, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], radio-detection
Abstract: International audience; Radio pulses associated with Extended Air Showers (EAS) produced in terrestrial atmosphere by High EnergyCosmic Rays (UHECR) of energy 10^17 eV and above, are now routinely observed by dedicated radioinstruments on ground. This may offer a new and appealing way for elucidating the nature and origin ofinvolved primary particles, an open question still unsolved.Unfortunately, the high occupancy of the electromagnetic spectrum by undesired signals from natural andanthropogenic origins has made unambiguous EAS radio detection a challenging problem. Former attemptsbased on timing coincidences from several independent radio antennas, or using auxiliary triggering byconventional particle detectors, are still not fully satisfying.We present here a solution based on real time, coherent radio detection by using a small array of 10x2 crosspolarized dipoles, distributed over a 150m x 150m surface area and operated in continuous sky surveyingmode.Preliminary results obtained with the new system are briefly reviewed and discussed.The final detection scheme will be achieved by using on line, fast computing software based on a dedicatedunsupervised recognition algorithm.The new array is a part of the CODALEMA experiment located in Nançay radio astronomy observatory(France).
Published: 2014

29. Explosive volcanism: inception, evolution and hazard / National Research Council, Geophysics Study Committee

Author: J. Urrutia Fucugauchi and Ana Lilian Martin del Pozzo
Subjects: vulcanismo explosivo, geofísica, volcanismo, Geophysics. Cosmic physics, QC801-809
Abstract: Este libro sobre "Volcanismo Explosivo" está formado por una colección de trece capítulos o artículos que, desde diferentes enfoques y disciplinas discuten uno de los fenómenos volcánicos de más alta peligrosidad. Las erupciones cataclísmicas del volcán El Chichón, al sur de México, durante marzo-abril de 1982 y las del volcán Santa Helena, noroeste de Estados Unidos, de mayo de 1980, pusieron de manifiesto la importancia de estudios sobre el volcanismo explosivo, no solo dentro de la comunidad de ciencias de la tierra, sino además a los gobiernos y la población en general. Este libro forma parte de la Serie de Geofísica publicada por la Academia Nacional de Ciencias de los Estados Unidos y constituye un ejemplo del creciente interés sobre estos estudios. El libro no solo está dirigido a especialistas en volcanología, sino que además (y ello es una de las intenciones de la Serie) intenta ser de interés para los encargados de la organización y toma de decisiones en situaciones, fenómenos, problemas, etcetera, que involucren la geofísica.
Published: 1989
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30. Searches for Large-Scale Anisotropy in the Arrival Directions of Cosmic Rays Detected above Energy of $10^{19}$ eV at the Pierre Auger Observatory and the Telescope Array

Author: Telescope, Array, Pierre Auger Collaborations (Alexander Aab, Pedro, Abreu, Marco, Aglietta, Eun Joo Ahn, Imen Al Samarai, Ivone, Albuquerque, Ingomar, Allekotte, Jeff, Allen, Patrick, Allison, Alejandro, Almela, Jesus Alvarez Castillo, Jaime Alvarez Muñiz, Rafael Alves Batista, Michelangelo, Ambrosio, Amin, Aminaei, Luis, Anchordoqui, Sofia, Andringa, Carla, Aramo, Victor Manuel Aranda, Fernando, Arqueros, Hernán Gonzalo Asorey, Pedro, Assis, Julien, Aublin, Maximo, Ave, Michel, Avenier, Gualberto, Avila, Nafiun, Awal, Alina Mihaela Badescu, Barber, Kerri B., Julia, Bäuml, Colin, Baus, Jim, Beatty, Karl Heinz Becker, Bellido, Jose A., Corinne, Berat, Mario Edoardo Bertania, Xavier, Bertou, Peter, Biermann, Pierre, Billoir, Blaess, Simon G., Miguel, Blanco, Carla, Bleve, Hans, Blümer, Martina, Boháčová, Denise, Boncioli, Carla, Bonifazi, Raffaella, Bonino, Nataliia, Borodai, Jeffrey, Brack, Iliana, Brancus, Ariel, Bridgeman, Pedro, Brogueira, Brown, William C., Peter, Buchholz, Antonio, Bueno, Stijn, Buitink, Buscemi, Mario, Caballero Mora, Karen S., Barbara, Caccianiga, Lorenzo, Caccianiga, Marina, Candusso, Laurentiu, Caramete, Caruso, Rossella, Antonella, Castellina, Gabriella, Cataldi, Lorenzo, Cazon, Rosanna, Cester, Chavez, Alan G., Andrea, Chiavassa, Jose Augusto Chinellato, Jiri, Chudoba, Marco, Cilmo, Clay, Roger W., Giuseppe, Cocciolo, Roberta, Colalillo, Alan, Coleman, Laura, Collica, Maria Rita Coluccia, Ruben, Conceição, Fernando, Contreras, Cooper, Mathew J., Alain, Cordier, Stephane, Coutu, Corbin, Covault, James, Cronin, Alex, Curutiu, Richard, Dallier, Bruno, Daniel, Sergio, Dasso, Kai, Daumiller, Dawson, Bruce R., de Almeida, Rogerio M., Manlio De Domenico, de Jong, Sijbrand J., Joao de Mello Neto, Ivan De Mitri, Jaime de Oliveira, Vitor de Souza, Luis del Peral, Olivier, Deligny, Hans, Dembinski, Niraj, Dhital, Claudio Di Giulio, Armando Di Matteo, Johana Chirinos Diaz, Mary Lucia Díaz Castro, Francisco, Diogo, Carola, Dobrigkeit, Wendy, Docters, Juan Carlos D'Olivo, Alexei, Dorofeev, Qader Dorosti Hasankiadeh, Maria Teresa Dova, Jan, Ebr, Ralph, Engel, Martin, Erdmann, Mona, Erfani, Escobar, Carlos O., Joao, Espadanal, Alberto, Etchegoyen, Pedro Facal San Luis, Heino, Falcke, Fang, Ke, Glennys, Farrar, Anderson, Fauth, Norberto, Fazzini, Ferguson, Andrew P., Mateus, Fernandes, Brian, Fick, Juan Manuel Figueira, Alberto, Filevich, Andrej, Filipčič, Brendan, Fox, Octavian, Fratu, Uwe, Fröhlich, Benjamin, Fuchs, Toshihiro, Fujii, Romain, Gaior, Beatriz, García, Sayri Tupac Garcia Roca, Diego Garcia Gamez, Diego Garcia Pinto, Gianpaolo, Garilli, Alberto Gascon Bravo, Florian, Gate, Hartmut, Gemmeke, Piera Luisa Ghia, Ugo, Giaccari, Marco, Giammarchi, Maria, Giller, Christian, Glaser, Henry, Glass, Mariano Gómez Berisso, Gómez Vitale, Primo F., Patrícia, Gonçalves, Gonzalez, Javier G., Nicolás, González, Ben, Gookin, Jacob, Gordon, Alessio, Gorgi, Peter, Gorham, Philippe, Gouffon, Stefan, Grebe, Nathan, Griffith, Aurelio, Grillo, Grubb, Trent D., Fausto, Guarino, Germano, Guedes, Matías Rolf Hampel, Patricia, Hansen, Diego, Harari, Harrison, Thomas A., Sebastian, Hartmann, John, Harton, Andreas, Haungs, Thomas, Hebbeker, Dieter, Heck, Philipp, Heimann, Herve, Alexander E., Hill, Gary C., Carlos, Hojvat, Nicholas, Hollon, Ewa, Holt, Piotr, Homola, Jörg, Hörandel, Pavel, Horvath, Miroslav, Hrabovský, Daniel, Huber, Tim, Huege, Antonio, Insolia, Paula Gina Isar, Ingolf, Jandt, Stefan, Jansen, Cecilia, Jarne, Mariela, Josebachuili, Alex, Kääpä, Olga, Kambeitz, Karl Heinz Kampert, Peter, Kasper, Igor, Katkov, Balazs, Kégl, Bianca, Keilhauer, Azadeh, Keivani, Ernesto, Kemp, Roger, Kieckhafer, Hans, Klages, Matthias, Kleifges, Jonny, Kleinfeller, Raphael, Krause, Nicole, Krohm, Oliver, Krömer, Daniel Kruppke Hansen, Daniel, Kuempel, Norbert, Kunka, Danielle, Lahurd, Luca, Latronico, Robert, Lauer, Markus, Lauscher, Pascal, Lautridou, Sandra Le Coz, Milton, Leão, Didier, Lebrun, Paul, Lebrun, Marcelo Augusto Leigui de Oliveira, Antoine Letessier Selvon, Isabelle Lhenry Yvon, Katrin, Link, Rebeca, López, Angeles Lopez Agüera, Karim, Louedec, Julio Lozano Bahilo, Lu, Lu, Agustin, Lucero, Marianne, Ludwig, Max, Malacari, Simone, Maldera, Manuela, Mallamaci, Jennifer, Maller, Dusan, Mandat, Paul, Mantsch, Analisa, Mariazzi, Vincent, Marin, Ioana, Mariş, Giovanni, Marsella, Daniele, Martello, Lilian, Martin, Humberto, Martinez, Oscar Martínez Bravo, Diane, Martraire, Jimmy Masías Meza, Hermann Josef Mathes, Sebastian, Mathys, James, Matthews, John, Matthews, Giorgio, Matthiae, Detlef, Maurel, Daniela, Maurizio, Eric, Mayotte, Peter, Mazur, Carlos, Medina, Gustavo Medina Tanco, Rebecca, Meissner, Maximilien, Melissas, Diego, Melo, Alexander, Menshikov, Stefano, Messina, Rishi, Meyhandan, Saša, Mićanović, Maria Isabel Micheletti, Lukas, Middendorf, Minaya, Ignacio A., Lino, Miramonti, Bogdan, Mitrica, Laura Molina Bueno, Silvia, Mollerach, Maria, Monasor, Delphine Monnier Ragaigne, François, Montanet, Carlo, Morello, Miguel, Mostafá, Moura, Celio A., Marcio Aparecido Muller, Gero, Müller, Sarah, Müller, Moritz, Münchmeyer, Roberto, Mussa, Gianni, Navarra, Sergio, Navas, Petr, Necesal, Lukas, Nellen, Anna, Nelles, Jens, Neuser, Nguyen, Phong H., Marcus, Niechciol, Lukas, Niemietz, Tim, Niggemann, Dave, Nitz, Dalibor, Nosek, Vladimir, Novotny, Lyberis, Nožka, Livingstone, Ochilo, Angela, Olinto, Micael, Oliveira, Noelia, Pacheco, Daniel Pakk Selmi Dei, Miroslav, Palatka, Juan, Pallotta, Nunzia, Palmieri, Philipp, Papenbreer, Gonzalo, Parente, Alejandra, Parra, Thomas, Paul, Miroslav, Pech, Jan, Pękala, Rodrigo, Pelayo, Iuri, Pepe, Lorenzo, Perrone, Emily, Petermann, Christine, Peters, Sergio, Petrera, Yevgeniy, Petrov, Jamyang, Phuntsok, Ricardo, Piegaia, Tanguy, Pierog, Pablo, Pieroni, Mário, Pimenta, Valerio, Pirronello, Manuel, Platino, Matthias, Plum, Alessio, Porcelli, Czeslaw, Porowski, Raul Ribeiro Prado, Paolo, Privitera, Michael, Prouza, Victor, Purrello, Quel, Eduardo J., Sven, Querchfeld, Sean, Quinn, Julian, Rautenberg, Olivier, Ravel, Diego, Ravignani, Benoît, Revenu, Jan, Ridky, Simone, Riggi, Markus, Risse, Pablo, Ristori, Vincenzo, Rizi, Washington Rodrigues de Carvalho, Iago Rodriguez Cabo, Gonzalo Rodriguez Fernandez, Jorge Rubén Rodriguez Rojo, Maria Dolores Rodríguez Frías, Dmytro, Rogozin, Germán, Ros, Jaime, Rosado, Tomas, Rossler, Markus, Roth, Esteban, Roulet, Adrian, Rovero, Saffi, Steven J., Alexandra, Saftoiu, Francesco, Salamida, Humberto, Salazar, Ahmed, Saleh, Francisco Salesa Greus, Gaetano, Salina, Federico, Sánchez, Patricia Sanchez Lucas, Santo, Catarina E., Edivaldo Moura Santos, Eva, Santos, Fred, Sarazin, Biswaijt, Sarkar, Raul, Sarmento, Ricardo, Sato, Nils, Scharf, Viviana, Scherini, Harald, Schieler, Peter, Schiffer, David, Schmidt, Olaf, Scholten, Harm, Schoorlemmer, Petr, Schovánek, Alexander, Schulz, Johannes, Schulz, Johannes, Schumacher, Sergio, Sciutto, Alberto, Segreto, Mariangela, Settimo, Amir, Shadkam, Shellard, Ronald C., Iván, Sidelnik, Guenter, Sigl, Octavian, Sima, Andrzej, Śmiałkowski, Radomir, Šmída, Gregory, Snow, Paul, Sommers, Sorokin, J., Ruben, Squartini, Srivastava, Yogendra N., Samo, Stanič, James, Stapleton, Jaroslaw, Stasielak, Maurice, Stephan, Anne, Stutz, Federico, Suarez, Tiina, Suomijärvi, Daniel Supanitsky, A., Michael, Sutherland, John, Swain, Zbigniew, Szadkowski, Marek, Szuba, Oscar Alejandro Taborda, Alex, Tapia, Mathieu, Tartare, Andreas, Tepe, Vanessa Menezes Theodoro, Charles, Timmermans, Todero Peixoto, Carlos J., Gabriel, Toma, Lenka, Tomankova, Bernardo, Tomé, Aurelio, Tonachini, Guillermo Torralba Elipe, Diego Torres Machado, Petr, Travnicek, Enrica, Trovato, Matias, Tueros, Ralf, Ulrich, Michael, Unger, Martin, Urban, Valdés Galicia, Jose F., Ines, Valiño, Laura, Valore, Guus van Aar, Patrick van Bodegom, van den Berg, Ad M., Sjoert van Velzen, Arjen van Vliet, Enrique, Varela, Bernardo Vargas Cárdenas, Gary, Varner, Vázquez, Jose R., Ricardo, Vázquez, Darko, Veberič, Valerio, Verzi, Jakub, Vicha, Mariela, Videla, Luis, Villaseñor, Brian, Vlcek, Serguei, Vorobiov, Hernan, Wahlberg, Oscar, Wainberg, David, Walz, Alan, Watson, Marc, Weber, Klaus, Weidenhaupt, Andreas, Weindl, Felix, Werner, Allan, Widom, Lawrence, Wiencke, Barbara, Wilczyńska, Henryk, Wilczyński, Martin, Will, Christopher, Williams, Tobias, Winchen, David, Wittkowski, Brian, Wundheiler, Sarka, Wykes, Tokonatsu, Yamamoto, Tolga, Yapici, Guofeng, Yuan, Alexey, Yushkov, Bruno, Zamorano, Enrique, Zas, Danilo, Zavrtanik, Marko, Zavrtanik, Ingyin, Zaw, Arnulfo, Zepeda, Jing, Zhou, Yue, Zhu, Marcelo Zimbres Silva, Michael, Ziolkowski, Francesca, Zuccarello, Rasha, Abbasi, Michihiko, Abe, Tareq Abu Zayyad, Monica, Allen, Robyn, Anderson, Ryuji, Azuma, Elliott, Barcikowski, Belz, John W., Bergman, Douglas R., Samuel Adam Blake, Robert, Cady, Min Jung Chae, Byung Gu Cheon, Junsei, Chiba, Michiyuki, Chikawa, Woo Ram Cho, Masaki, Fukushima, Takashi, Goto, William, Hanlon, Yoshio, Hayashi, Naoaki, Hayashida, Kinya, Hibino, Ken, Honda, Daisuke, Ikeda, Naoya, Inoue, Takaaki, Ishii, Rie, Ishimori, Hideo Ito (Utah, U., Riken, Dmitri, Ivanov, Jui, Charles C. H., Kenichi, Kadota, Fumio, Kakimoto, Oleg, Kalashev, Katsuaki, Kasahara, Hideyuki, Kawai, Saburo, Kawakami, Shingo, Kawana, Kazumasa, Kawata, Eiji, Kido, Hang Bae Kim, Ji Hee Kim, Ji Hyun Kim, Seiji, Kitamura, Yuki, Kitamura, Vadim, Kuzmin, Young Joon Kwon, Jian, Lan, Sun In Lim, Jon Paul Lundquist, Kazuhiro, Machida, Kai, Martens, Takeshi, Matsuda, Toshio, Matsuyama, Matthews, John N., Mayuko, Minamino, Keijiro, Mukai, Isaac, Myers, Keisuke, Nagasawa, Shigehiro, Nagataki, Toru, Nakamura, Toshiyuki, Nonaka, Asuka, Nozato, Shoichi, Ogio, Jun, Ogura, Munehiro, Ohnishi, Hideyuki, Ohoka, Kaoru, Oki, Takeshi, Okuda, Masaomi, Ono, Akitoshi, Oshima, Shunsuke, Ozawa, Park, Il H., Pshirkov, Maxim S., Douglas Chase Rodriguez, Grigory, Rubtsov, Dongsu, Ryu, Hiroyuki, Sagawa, Nobuyuki, Sakurai, Sampson, Amanda L., Scott, Lauren M., Priti Dhanesh Shah, Fumiya, Shibata, Tatsunobu, Shibata, Hideaki, Shimodaira, Bok Kyun Shin, Smith, Jeremy D., Pierre, Sokolsky, Wayne Springer, R., Benjamin Taylor Stokes, Stratton, Sean R., Thomas, Stroman, Takumi, Suzawa, Mai, Takamura, Masahiro, Takeda, Ryuji, Takeishi, Akimichi, Taketa, Masato, Takita, Yuichiro, Tameda, Hideki, Tanaka, Koichi, Tanaka, Manobu, Tanaka, Thomas, Stanton B., Thomson, Gordon B., Peter, Tinyakov, Igor, Tkachev, Hisao, Tokuno, Takayuki, Tomida, Sergey, Troitsky, Yoshiki, Tsunesada, Kazuki, Tsutsumi, Yukio, Uchihori, Shigeharu, Udo, Federico, Urban, Gina, Vasiloff, Tiffany, Wong, Hiroshi, Yamaoka, Katsuya, Yamazaki, Jongmann, Yang, Kenta, Yashiro, Shigeru, Yoshida, Hisashi, Yoshii, Rhett, Zollinger, Zachary, Zundel, Shogo, Konishi, Shingo, Wachi, Yoshiki, Nishimoto, Heungsu, Shin, Mai, Tsujimoto, Tomoya, Matsuhira, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire SUBATECH Nantes (SUBATECH), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Unité Scientifique de la Station de Nançay (USN), Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire d'Orsay (IPNO), PIERRE AUGER, Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), A., Aab, P., Abreu, M., Aglietta, E. J., Ahn, I., Al Samarai, I. F. M., Albuquerque, I., Allekotte, J., Allen, P., Allison, A., Almela, J., Alvarez Castillo, J., Alvarez Mu?iz, R., Alves Batista, M., Ambrosio, A., Aminaei, L., Anchordoqui, S., Andringa, Aramo, Carla, F., Arquero, H., Asorey, P., Assi, J., Aublin, M., Ave, M., Avenier, G., Avila, A. M., Badescu, K. B., Barber, J., B?uml, C., Bau, J. J., Beatty, K. H., Becker, J. A., Bellido, C., Berat, M. E., Bertaina, X., Bertou, P. L., Biermann, P., Billoir, M., Blanco, C., Bleve, H., Bl?mer, M., Boh??ov?, D., Boncioli, C., Bonifazi, R., Bonino, N., Borodai, J., Brack, I., Brancu, P., Brogueira, W. C., Brown, P., Buchholz, A., Bueno, S., Buitink, Buscemi, Mario, K. S., Caballero Mora, B., Caccianiga, L., Caccianiga, M., Candusso, L., Caramete, R., Caruso, A., Castellina, G., Cataldi, L., Cazon, R., Cester, A. G., Chavez, A., Chiavassa, J. A., Chinellato, J., Chudoba, Cilmo, Marco, R. W., Clay, G., Cocciolo, Colalillo, Roberta, A., Coleman, L., Collica, M. R., Coluccia, R., Concei??o, F., Contrera, M. J., Cooper, A., Cordier, S., Coutu, C. E., Covault, J., Cronin, A., Curutiu, R., Dallier, B., Daniel, S., Dasso, K., Daumiller, B. R., Dawson, R. M., de Almeida, M., De Domenico, S. J., de Jong, J. R. T., de Mello Neto, I., De Mitri, J., de Oliveira, V., de Souza, L., del Peral, O., Deligny, H., Dembinski, N., Dhital, C., Di Giulio, A., Di Matteo, J. C., Diaz, M. L., D?az Castro, F., Diogo, C., Dobrigkeit, W., Docter, J. C., D'Olivo, A., Dorofeev, Q., Dorosti Hasankiadeh, M. T., Dova, J., Ebr, R., Engel, M., Erdmann, M., Erfani, C. O., Escobar, J., Espadanal, A., Etchegoyen, P., Facal San Lui, H., Falcke, K., Fang, G., Farrar, A. C., Fauth, N., Fazzini, A. P., Ferguson, M., Fernande, B., Fick, J. M., Figueira, A., Filevich, A., Filip?i?, B. D., Fox, O., Fratu, U., Fr?hlich, B., Fuch, T., Fuji, R., Gaior, B., Garc?a, S. T., Garcia Roca, D., Garcia Gamez, D., Garcia Pinto, G., Garilli, A., Gascon Bravo, F., Gate, H., Gemmeke, P. L., Ghia, U., Giaccari, M., Giammarchi, M., Giller, C., Glaser, H., Gla, M., G?mez Berisso, P. F., G?mez Vitale, P., Gon?alve, J. G., Gonzalez, N., Gonz?lez, B., Gookin, A., Gorgi, P., Gorham, P., Gouffon, S., Grebe, N., Griffith, A. F., Grillo, T. D., Grubb, Y., Guardincerri, Guarino, Fausto, G. P., Guede, M. R., Hampel, P., Hansen, D., Harari, T. A., Harrison, S., Hartmann, J. L., Harton, A., Haung, T., Hebbeker, D., Heck, P., Heimann, A. E., Herve, G. C., Hill, C., Hojvat, N., Hollon, E., Holt, P., Homola, J. R., H?randel, P., Horvath, M., Hrabovsk?, D., Huber, T., Huege, A., Insolia, P. G., Isar, K., Islo, I., Jandt, S., Jansen, C., Jarne, M., Josebachuili, A., K??p?, O., Kambeitz, K. H., Kampert, P., Kasper, I., Katkov, B., K?gl, B., Keilhauer, A., Keivani, E., Kemp, R. M., Kieckhafer, H. O., Klage, M., Kleifge, J., Kleinfeller, R., Krause, N., Krohm, O., Kr?mer, D., Kruppke Hansen, D., Kuempel, N., Kunka, G., La Rosa, D., Lahurd, L., Latronico, R., Lauer, M., Lauscher, P., Lautridou, S., Le Coz, M. S. A. B., Le?o, D., Lebrun, P., Lebrun, M. A., Leigui de Oliveira, A., Letessier Selvon, I., Lhenry Yvon, K., Link, R., L?pez, A., Lopez Ag?era, K., Louedec, J., Lozano Bahilo, L., Lu, A., Lucero, M., Ludwig, M. C., Maccarone, M., Malacari, S., Maldera, M., Mallamaci, J., Maller, D., Mandat, P., Mantsch, A. G., Mariazzi, V., Marin, I. C., Mari?, G., Marsella, D., Martello, L., Martin, H., Martinez, O., Mart?nez Bravo, D., Martraire, J. J., Mas?as Meza, H. J., Mathe, S., Mathy, J. A. J., Matthew, J., Matthew, G., Matthiae, D., Maurel, D., Maurizio, E., Mayotte, P. O., Mazur, C., Medina, G., Medina Tanco, M., Melissa, D., Melo, E., Menichetti, A., Menshikov, S., Messina, R., Meyhandan, S., Mi?anovi?, M. I., Micheletti, L., Middendorf, I. A., Minaya, L., Miramonti, B., Mitrica, L., Molina Bueno, S., Mollerach, M., Monasor, D., Monnier Ragaigne, F., Montanet, C., Morello, M., Mostaf?, C. A., Moura, M. A., Muller, G., M?ller, M., M?nchmeyer, R., Mussa, G., Navarra, S., Nava, P., Necesal, L., Nellen, A., Nelle, J., Neuser, M., Niechciol, L., Niemietz, T., Niggemann, D., Nitz, D., Nosek, V., Novotny, L., No?ka, L., Ochilo, A., Olinto, M., Oliveira, N., Pacheco, D., Pakk Selmi Dei, M., Palatka, J., Pallotta, N., Palmieri, P., Papenbreer, G., Parente, A., Parra, T., Paul, M., Pech, J., P?kala, R., Pelayo, I. M., Pepe, L., Perrone, R., Pesce, E., Petermann, C., Peter, S., Petrera, A., Petrolini, Y., Petrov, J., Phuntsok, R., Piegaia, T., Pierog, P., Pieroni, M., Pimenta, V., Pirronello, M., Platino, M., Plum, A., Porcelli, C., Porowski, R. R., Prado, P., Privitera, M., Prouza, V., Purrello, E. J., Quel, S., Querchfeld, S., Quinn, J., Rautenberg, O., Ravel, D., Ravignani, B., Revenu, J., Ridky, S., Riggi, M., Risse, P., Ristori, V., Rizi, J., Robert, W., Rodrigues de Carvalho, I., Rodriguez Cabo, G., Rodriguez Fernandez, J., Rodriguez Rojo, M. D., Rodr?guez Fr?a, G., Ro, J., Rosado, T., Rossler, M., Roth, E., Roulet, A. C., Rovero, S. J., Saffi, A., Saftoiu, F., Salamida, H., Salazar, A., Saleh, F., Salesa Greu, G., Salina, F., S?nchez, P., Sanchez Luca, C. E., Santo, E., Santo, E. M., Santo, F., Sarazin, B., Sarkar, R., Sarmento, R., Sato, N., Scharf, V., Scherini, H., Schieler, P., Schiffer, O., Scholten, H., Schoorlemmer, P., Schov?nek, A., Schulz, J., Schulz, J., Schumacher, S. J., Sciutto, A., Segreto, M., Settimo, A., Shadkam, R. C., Shellard, I., Sidelnik, G., Sigl, O., Sima, A., ?mia?kowski, R., ?m?da, G. R., Snow, P., Sommer, J., Sorokin, R., Squartini, Y. N., Srivastava, S., Stani?, J., Stapleton, J., Stasielak, M., Stephan, A., Stutz, F., Suarez, T., Suomij?rvi, A. D., Supanitsky, M. S., Sutherland, J., Swain, Z., Szadkowski, M., Szuba, O. A., Taborda, A., Tapia, M., Tartare, V. M., Theodoro, C., Timmerman, C. J., Todero Peixoto, G., Toma, L., Tomankova, B., Tom?, A., Tonachini, G., Torralba Elipe, D., Torres Machado, P., Travnicek, E., Trovato, M., Tuero, R., Ulrich, M., Unger, M., Urban, Galicia, J. F. Vald?s., I., Vali?o, Valore, Laura, G., van Aar, A. M., van den Berg, S., van Velzen, A., van Vliet, E., Varela, B., Vargas C?rdena, G., Varner, J. R., V?zquez, R. A., V?zquez, D., Veberi?, V., Verzi, J., Vicha, M., Videla, L., Villase?or, B., Vlcek, S., Vorobiov, H., Wahlberg, O., Wainberg, D., Walz, A. 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P., Lundquist, K., Machida, K., Marten, T., Matsuda, T., Matsuyama, J. N., Matthew, M., Minamino, K., Mukai, I., Myer, K., Nagasawa, S., Nagataki, T., Nakamura, T., Nonaka, A., Nozato, S., Ogio, J., Ogura, M., Ohnishi, H., Ohoka, K., Oki, T., Okuda, M., Ono, A., Oshima, S., Ozawa, I. H., Park, M. S., Pshirkov, D. C., Rodriguez, G., Rubtsov, D., Ryu, H., Sagawa, N., Sakurai, A. L., Sampson, L. M., Scott, P. D., Shah, F., Shibata, T., Shibata, H., Shimodaira, B. K., Shin, J. D., Smith, P., Sokolsky, R. W., Springer, B. T., Stoke, S. R., Stratton, T. A., Stroman, T., Suzawa, M., Takamura, M., Takeda, R., Takeishi, A., Taketa, M., Takita, Y., Tameda, H., Tanaka, K., Tanaka, M., Tanaka, S. B., Thoma, G. 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Honda, D. Ikeda, N. Inoue, T. Ishii, R. Ishimori, H. Ito, D. Ivanov, C. C. H., K. Kadota, F. Kakimoto, O. Kalashev, K. Kasahara, H. Kawai, S. Kawakami, S. Kawana, K. Kawata, E. Kido, H. B. Kim, J. H. Kim, S. Kitamura, Y. Kitamura, V. Kuzmin, Y. J. Kwon, J. Lan, S. I. Lim, J. P. Lundquist, K. Machida, K. Marten, T. Matsuda, T. Matsuyama, J. N. Matthew, M. Minamino, K. Mukai, I. Myer, K. Nagasawa, S. Nagataki, T. Nakamura, T. Nonaka, A. Nozato, S. Ogio, J. Ogura, M. Ohnishi, H. Ohoka, K. Oki, T. Okuda, M. Ono, A. Oshima, S. Ozawa, I. H. Park, M. S. Pshirkov, D. C. Rodriguez, G. Rubtsov, D. Ryu, H. Sagawa, N. Sakurai, A. L. Sampson, L. M. Scott, P. D. Shah, F. Shibata, T. Shibata, H. Shimodaira, B. K. Shin, J. D. Smith, P. Sokolsky, R. W. Springer, B. T. Stoke, S. R. Stratton, T. A. Stroman, T. Suzawa, M. Takamura, M. Takeda, R. Takeishi, A. Taketa, M. Takita, Y. Tameda, H. Tanaka, K. Tanaka, M. Tanaka, S. B. Thoma, G. B. Thomson, P. Tinyakov, I. Tkachev, H. Tokuno, T. Tomida, S. Troitsky, Y. Tsunesada, K. Tsutsumi, Y. Uchihori, S. Udo, F. Urban, G. Vasiloff, T. Wong, R. Yamane, H. Yamaoka, K. Yamazaki, J. Yang, K. Yashiro, Y. Yoneda, S. Yoshida, H. Yoshii, R. Zollinger, Z. Zundel, T. T. Array, and Research unit Astroparticle Physics
Subjects: Ciencias Físicas, Astronomy, Rays, Astrophysics, Astroparticle physics, Cosmic rays, 01 natural sciences, law.invention, Pierre, law, Anisotropy, Telescope, 010303 astronomy & astrophysics, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, [PHYS]Physics [physics], Energy, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astrophysics::Instrumentation and Methods for Astrophysics, astroparticle physic, Radiación cósmica, Auger, Cosmic, Arrival, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Física nuclear, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, CIENCIAS NATURALES Y EXACTAS, High, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, SURFACE DETECTOR, ICECUBE, AIR-SHOWER ARRAY, Directions, cosmic rays, 0103 physical sciences, Instrumentation and Methods for Astrophysics (astro-ph.IM), Ciencias Exactas, Pierre Auger Observatory, SPECTRUM, 010308 nuclear & particles physics, Array, Spectral density, Spherical harmonics, Física, Astronomy and Astrophysics, ASTROFÍSICA, Ultra, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Astronomía, Dipole, RESOLUTION, Space and Planetary Science, Experimental High Energy Physics, Quadrupole, Observatory, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: Spherical harmonic moments are well-suited for capturing anisotropy at any scale in the flux of cosmic rays. An unambiguous measurement of the full set of spherical harmonic coefficients requires full-sky coverage. This can be achieved by combining data from observatories located in both the northern and southern hemispheres. To this end, a joint analysis using data recorded at the Telescope Array and the Pierre Auger Observatory above 1019 eV is presented in this work. The resulting multipolar expansion of the flux of cosmic rays allows us to perform a series of anisotropy searches, and in particular to report on the angular power spectrum of cosmic rays above 1019 eV. No significant deviation from isotropic expectations is found throughout the analyses performed. Upper limits on the amplitudes of the dipole and quadrupole moments are derived as a function of the direction in the sky, varying between 7% and 13% for the dipole and between 7% and 10% for a symmetric quadrupole., Facultad de Ciencias Exactas
Published: 2014
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31. Highlights from the Pierre Auger Observatory

Author: antoine letessier selvon, For The Pierre Auger Collaboration, Aab, A., Abreu, P., Aglietta, M., Ahlers, M., Ahn, E. J., Albuquerque, I. F. M., Allekotte, I., Allen, J., Allison, P., Almela, A., Alvarez Castillo, J., Alvarez-Muniz, J., Alves Batista, R., Ambrosio, M., Aminaei, A., Anchordoqui, L., Andringa, S., Antivcic, T., Aramo, C., Arqueros, F., Asorey, H., Assis, P., Aublin, J., Ave, M., Avenier, M., Avila, G., Badescu, A. M., Barber, K. B., Bardenet, R., Baeuml, J., Baus, C., Beatty, J. J., Becker, K. H., Belletoile, A., Bellido, J. A., Benzvi, S., Berat, C., Bertou, X., Biermann, P. L., Billoir, P., Blanco, F., Blanco, M., Bleve, C., Blumer, H., Bohacova, M., Boncioli, D., Bonifazi, C., Bonino, R., Borodai, N., Brack, J., Brancus, I., Brogueira, P., Brown, W. C., Buchholz, P., Bueno, A., Burton, R. E., Buscemi, M., Caballero-Mora, K. S., Caccianiga, B., Caccianiga, L., Candusso, M., Caramete, L., Caruso, R., Castellina, A., Cataldi, G., Cazon, L., Cester, R., Cheng, S. H., Chiavassa, A., Chinellato, J. A., Chudoba, J., Cilmo, M., Clay, R. W., Cocciolo, G., Colalillo, R., Collica, L., Coluccia, M. R., Conceicao, R., Contreras, F., Cook, H., Cooper, M. J., Coutu, S., Covault, C. E., Criss, A., Cronin, J., Curutiu, A., Richard Dallier, Daniel, B., Dasso, S., Daumiller, K., Dawson, B. R., Almeida, R. M., Domenico, M., Jong, S. J., La Vega, G., Mello Junior, W. J. M., Mello Neto, J. R. T., Mitri, I., Souza, V., Vries, K. D., Del Peral, L., Deligny, O., Dembinski, H., Dhital, N., Di Giulio, C., Diaz, J. C., Diaz Castro, M. L., Diep, P. N., Diogo, F., Dobrigkeit, C., Docters, W., Olivo, J. C. D., Dong, P. N., Dorofeev, A., Dos Anjos, J. C., Dova, M. T., Ebr, J., Engel, R., Erdmann, M., Escobar, C. O., Espadanal, J., Etchegoyen, A., Facal San Luis, P., Falcke, H., Fang, K., Farrar, G., Fauth, A. C., Fazzini, N., Ferguson, A. P., Fick, B., Figueira, J. M., Filevich, A., Filipcic, A., Foerster, N., Fox, B. D., Fracchiolla, C. E., Fraenkel, E. D., Fratu, O., Frohlich, U., Fuchs, B., Gaior, R., Gamarra, R. F., Gambetta, S., Garcia, B., Garcia Roca, S. T., Garcia-Gamez, D., Garcia-Pinto, D., Garilli, G., Gascon Bravo, A., Gemmeke, H., Ghia, P. L., Giller, M., Gitto, J., Glaser, C., Glass, H., Gomez Albarracin, F., Gomez Berisso, M., Gomez Vitale, P. F., Goncalves, P., Gonzalez, J. G., Gookin, B., Gorgi, A., Gorham, P., Gouffon, P., Grebe, S., Griffith, N., Grillo, A. F., Grubb, T. D., Guardincerri, Y., Guarino, F., Guedes, G. P., Hansen, P., Harari, D., Harrison, T. A., Harton, J. L., Haungs, A., Hebbeker, T., Heck, D., Herve, A. E., Hill, G. C., Hojvat, C., Hollon, N., Homola, P., Hoerandel, J. R., Horvath, P., Hrabovsky, M., Huber, D., Huege, T., Insolia, A., Isar, P. G., Jansen, S., Jarne, C., Josebachuili, M., Kadija, K., Kambeitz, O., Kampert, K. H., Karhan, P., Kasper, P., Katkov, I., Kegl, B., Keilhauer, B., Keivani, A., Kemp, E., Kieckhafer, R. M., Klages, H. O., Kleifges, M., Kleinfeller, J., J. Knapp D, Krause, R., Krohm, N., Kroemer, O., Kruppke-Hansen, D., Kuempel, D., Kunka, N., La Rosa, G., Lahurd, D., Latronico, L., Lauer, R., Lauscher, M., Pascal Lautridou, Le Coz, S., Leao, M. S. A. B., Lebrun, D., Lebrun, P., Leigui Oliveira, M. A., Lhenry-Yvon, I., Link, K., Lopez, R., Lopez Aguera, A., Louedec, K., Lozano Bahilo, J., Lu, L., Lucero, A., Ludwig, M., Lyberis, H., Maccarone, M. C., Macolino, C., Malacari, M., Maldera, S., Maller, J., Mandat, D., Mantsch, P., Mariazzi, A. G., Marin, V., Maris, I. C., Marquez Falcon, H. R., Marsella, G., Martello, D., Lilian Martin, Martinez, H., Martinez Bravo, O., Martraire, D., Masias Meza, J. J., Mathes, H. J., Matthews, J., Matthews, J. A. J., Matthiae, G., Maurel, D., Maurizio, D., Mayotte, E., Mazur, P. O., Medina, C., Medina-Tanco, G., Melissas, M., Melo, D., Menichetti, E., Menshikov, A., Messina, S., Meyhandan, R., Micanovic, S., Micheletti, M. I., Middendorf, L., Minaya, I. A., Miramonti, L., Mitrica, B., Molina-Bueno, L., Mollerach, S., Monasor, M., Monnier Ragaigne, D., Montanet, F., Morales, B., Morello, C., Moreno, J. C., Mostafa, M., Moura, C. A., Muller, M. A., Muller, G., Munchmeyer, M., Mussa, R., Navarra, G., Navarro, J. L., Navas, S., Necesal, P., Nellen, L., Nelles, A., Neuser, J., Nhung, P. T., Niechciol, M., Niemietz, L., Niggemann, T., Nitz, D., Nosek, D., Novzka, L., Oehlschlager, J., Olinto, A., Oliveira, M., Ortiz, M., Pacheco, N., Pakk Selmi-Dei, D., Palatka, M., Pallotta, J., Palmieri, N., Parente, G., Parra, A., Pastor, S., Paul, T., Pech, M., Pekala, J., Pelayo, R., Pepe, I. M., Perrone, L., Pesce, R., Petermann, E., Petrera, S., Petrolini, A., Petrov, Y., Piegaia, R., Pierog, T., Pieroni, P., Pimenta, M., Pirronello, V., Platino, M., Plum, M., Pontz, M., Porcelli, A., Preda, T., Privitera, P., Prouza, M., Quel, E. J., Querchfeld, S., Quinn, S., Rautenberg, J., Ravel, O., Ravignani, D., Benoît Revenu, Ridky, J., Riggi, S., Risse, M., Ristori, P., Rivera, H., Rizi, V., Roberts, J., Rodrigues Carvalho, W., Rodriguez Cabo, I., Rodriguez Fernandez, G., Rodriguez Martino, J., Rodriguez Rojo, J., Rodriguez-Frias, M. D., Ros, G., Rosado, J., Rossler, T., Roth, M., Rouille-D Orfeuil, B., Roulet, E., Rovero, A. C., Ruhle, C., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Salesa Greus, F., Salina, G., Sanchez, F., Sanchez-Lucas, P., Santo, C. E., Santos, E., Santos, E. M., Sarazin, F., Sarkar, B., Sato, R., Scharf, N., Scherini, V., Schieler, H., Schiffer, P., Schmidt, A., Scholten, O., Schoorlemmer, H., Schovanek, P., Schroeder, F. G., Schulz, A., Schulz, J., Sciutto, S. J., Scuderi, M., Segreto, A., Settimo, M., Shadkam, A., Shellard, R. C., Sidelnik, I., Sigl, G., Sima, O., Smialkowski, A., Smida, R., Snow, G. R., Sommers, P., Sorokin, J., Spinka, H., Squartini, R., Srivastava, Y. N., Stanic, S., Stapleton, J., Stasielak, J., Stephan, M., Straub, M., Stutz, A., Suarez, F., Suomijarvi, T., Supanitsky, A. D., Susa, T., Sutherland, M. S., Swain, J., Szadkowski, Z., Szuba, M., Tapia, A., Tartare, M., Tacscuau, O., Tcaciuc, R., Thao, N. T., Tiffenberg, J., Timmermans, C., Tkaczyk, W., Todero Peixoto, C. J., Toma, G., Tomankova, L., Tome, B., Tonachini, A., Torralba Elipe, G., Torres Machado, D., Travnicek, P., Tridapalli, D. B., Trovato, E., Tueros, M., Ulrich, R., Unger, M., Valdes Galicia, J. F., Valino, I., Valore, L., Aar, G., Den Berg, A. M., Velzen, S., Vliet, A., Varela, E., Vargas Cardenas, B., Varner, G., Vazquez, J. R., Vazquez, R. A., Veberic, D., Verzi, V., Vicha, J., Videla, M., Villasenor, L., Wahlberg, H., Wahrlich, P., Wainberg, O., Walz, D., Watson, A. A., Weber, M., Weidenhaupt, K., Weindl, A., Felix Werner, Westerhoff, S., Whelan, B. J., Widom, A., Wieczorek, G., Wiencke, L., Wilczynska, B., Wilczynski, H., Will, M., Williams, C., Winchen, T., Wundheiler, B., Wykes, S., Yamamoto, T., Yapici, T., Younk, P., Yuan, G., Yushkov, A., Zamorano, B., Zas, E., Zavrtanik, D., Zavrtanik, M., Zaw, I., Zepeda, A., Zhou, J., Zhu, Y., Zimbres Silva, M., Ziolkowski, M., Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire SUBATECH Nantes (SUBATECH), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Institut de Physique Nucléaire d'Orsay (IPNO), PIERRE AUGER, Research unit Nuclear & Hadron Physics, Research unit Astroparticle Physics, Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Subjects: [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astronomy, Astrophysics::High Energy Astrophysical Phenomena, General Physics and Astronomy, FOS: Physical sciences, Cosmic ray, 7. Clean energy, Auger, Observatory, Energy spectrum, ddc:530, Cosmic-ray observatory, Pierre Auger Observatory, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Detector, Astrophysics::Instrumentation and Methods for Astrophysics, RAYS, Highlights, Data quality, Experimental High Energy Physics, Ultrahigh-energy cosmic rays, Astrophysics - High Energy Astrophysical Phenomena
Abstract: The Pierre Auger Observatory is the world's largest cosmic ray observatory. Our current exposure reaches nearly 40,000 km$^2$ str and provides us with an unprecedented quality data set. The performance and stability of the detectors and their enhancements are described. Data analyses have led to a number of major breakthroughs. Among these we discuss the energy spectrum and the searches for large-scale anisotropies. We present analyses of our X$_{max}$ data and show how it can be interpreted in terms of mass composition. We also describe some new analyses that extract mass sensitive parameters from the 100% duty cycle SD data. A coherent interpretation of all these recent results opens new directions. The consequences regarding the cosmic ray composition and the properties of UHECR sources are briefly discussed., Comment: 9 pages, 12 figures, talk given at the 33rd International Cosmic Ray Conference, Rio de Janeiro 2013
Published: 2013
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32. Adrenal lymphoma: presentation, management and prognosis

Author: Bruno Vergès, Lilian Martin, Lm. Fornecker, Herve Ghesquieres, G. Aussedat, Benjamin Bouillet, Sophie Borot, Adrien Chauchet, Serge Bologna, J-M Petit, K Laurent, Olivier Casasnovas, Camille Laurent, Service d'Endocrinologie, Diabétologie et Maladies Métaboliques (CHU de Dijon), Centre Hospitalier Universitaire de Dijon - Hôpital François Mitterrand (CHU Dijon), Service d'Hématologie Clinique (CHU de Dijon), Service de Pathologie [CHU de Dijon], Service d'hématologie, Centre Hospitalier Régional Universitaire de Besançon (CHRU Besançon), Service d’Hématologie [Centre Hospitalier Lyon Sud - HCL], Centre Hospitalier Lyon Sud [CHU - HCL] (CHLS), Hospices Civils de Lyon (HCL)-Hospices Civils de Lyon (HCL), Département d'Oncologie et Hématologie [Strasbourg], Les Hôpitaux Universitaires de Strasbourg (HUS), Service d'Hématologie [CHRU Nancy], Centre Hospitalier Régional Universitaire de Nancy (CHRU Nancy), and Service de Diabétologie - Endocrinologie [CHRU Besançon]
Subjects: Male, Abdominal pain, Masses, Survival, medicine.medical_treatment, Adrenal Gland Neoplasms, 0302 clinical medicine, Antineoplastic Combined Chemotherapy Protocols, Adrenocortical Carcinoma, Adrenocortical carcinoma, 030212 general & internal medicine, B-cell lymphoma, Aged, 80 and over, medicine.diagnostic_test, Lymphoma, Non-Hodgkin, General Medicine, Middle Aged, Prognosis, Magnetic Resonance Imaging, humanities, 3. Good health, Positron emission tomography, 030220 oncology & carcinogenesis, Female, France, Radiology, medicine.symptom, B-Cell Lymphoma, medicine.drug, Adult, medicine.medical_specialty, 03 medical and health sciences, Non-Hodgkins-Lymphoma, medicine, Adrenal insufficiency, Plus Rituximab, Humans, Aged, Retrospective Studies, Fluorodeoxyglucose, business.industry, Adrenalectomy, Acvbp, medicine.disease, Lymphoma, Surgery, Chop Chemotherapy, Insufficiency, Of-The-Literature, Positron-Emission Tomography, Tomography, X-Ray Computed, business, [SDV.MHEP]Life Sciences [q-bio]/Human health and pathology, Adrenal Insufficiency
Abstract: International audience; Aim:This study aimed to identify the clinical, radiological and prognostic features of primary adrenal lymphoma (PAL) in order to diagnose the disease more accurately.Materials and methods:A retrospective multi-centre study was conducted on the clinical, biological and radiological features as well as the treatment and overall survival outcomes in PAL.Results:Between 1994 and 2014, 28 patients from five regions of eastern France were diagnosed with primary adrenal lymphoma. The revealing symptoms were a worsening general state (77%), weight loss (77%) and abdominal pain (42%). Biological features of PAL were almost omnipresent: increased LDH, β2 microglobulin, CRP or ferritinaemia levels. The PAL was bilateral in 20 cases (71%), adrenal insufficiency was searched for in 11 patients and found in eight (73%). CT scans showed masses of various sizes measuring up to 180 mm. On MRI, the lesions were hypointense in T1 and hyperintense in T2. When done, positron emission tomography with fluorodeoxyglucose (FDG-PET) showed locations not seen on the CT and revealed extra-adrenal locations in 70% of examinations. Adrenalectomy brought no benefit. The overall survival rate was poor (61.9% at 2 years) despite polychemotherapy.Conclusion:The clinical presentation of PAL comprised major general symptoms. Adrenal insufficiency was very common in patients with bilateral involvement but was not systematically tested. PET was an efficient examination to visualize extra-adrenal locations. The preliminary results of MRI to distinguish between PAL and adrenocortical carcinoma should be confirmed. Further studies are needed to establish an optimal strategy for the management of these primary adrenal lymphomas
Published: 2016
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33. Geomagnetic origin of the radio emission from cosmic ray induced air showers observed by CODALEMA

Author: C. Fabrice, L. Denis, Benoît Revenu, X. Garrido, D. Breton, C. Dumez-Viou, A. Sourice, Pascal Lautridou, F. Meyer, K. Payet, F. Haddad, D.H. Koang, Nicole Meyer-Vernet, M. Chendeb, Didier Charrier, J. Chauvin, D. Monnier-Ragaigne, Thierry Gousset, François Lefeuvre, E. Meyer, S. Valcares, Lilian Martin, S. Dagoret-Campagne, O. Ravel, T. Saugrin, G. Plantier, A. Stutz, N. Gautherot, D. Lebrun, Corinne Berat, A. Cordier, Alain Lecacheux, F. Montanet, C. Riviere, T. Garcon, Richard Dallier, J. Lamblin, A. Bellétoile, P. Stassi, D. Ardouin, Laboratoire SUBATECH Nantes (SUBATECH), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), ESEO-GSII (GSII), ESEO-Tech, Université Bretagne Loire (UBL)-Université Bretagne Loire (UBL), Unité Scientifique de la Station de Nançay (USN), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO), Laboratoire d'astrophysique de l'observatoire de Besançon (UMR 6091) (LAOB), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Franche-Comté (UFC), Université Bourgogne Franche-Comté [COMUE] (UBFC)-Université Bourgogne Franche-Comté [COMUE] (UBFC), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), CODALEMA, Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Bretagne Loire (UBL)-École supérieure d'électronique de l'ouest [Angers] (ESEO)-Université Bretagne Loire (UBL)-École supérieure d'électronique de l'ouest [Angers] (ESEO), Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Subjects: 96.40.-z, Physics::Instrumentation and Detectors, 95.85.Ry, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, Astrophysics, 01 natural sciences, Asymmetry, Particle detector, Ultra-High-Energy Cosmic Rays, Extensive Air showers, Observatory, 0103 physical sciences, Radio detection, 010306 general physics, media_common, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, 010308 nuclear & particles physics, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, Air shower, Earth's magnetic field, 95.55.Jz, High Energy Physics::Experiment, Astrophysics - High Energy Astrophysical Phenomena, Radio wave
Abstract: The new setup of the CODALEMA experiment installed at the Radio Observatory in Nancay, France, is described. It includes broadband active dipole antennas and an extended and upgraded particle detector array. The latter gives access to the air shower energy, allowing us to compute the efficiency of the radio array as a function of energy. We also observe a large asymmetry in counting rates between showers coming from the North and the South in spite of the symmetry of the detector. The observed asymmetry can be interpreted as a signature of the geomagnetic origin of the air shower radio emission. A simple linear dependence of the electric field with respect to vxB is used which reproduces the angular dependencies of the number of radio events and their electric polarity., Comment: 9 pages, 15 figures, 1 table
Published: 2010
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34. ALICE Technical Design Report on Forward Detectors : FMD, T0 and V0

Author: Cortese, P., Dellacasa, G., Ramello, L., Sitta, M., Ahmad, N., Ahmad, S., Ahmad, T., Bari, W., Irfan, M., Zafar, M., Belogianni, A., Ganoti, P., Petridis, A., Roukoutakis, F., Spyropoulou-Stassinaki, M., Vassiliou, M., Bruno, G. E., Caselle, M., Di Bari, D., Elia, D., Fini, R. A., Ghidini, B., Lenti, V., Manzari, V., Nappi, E., Navach, F., Pastore, C., Paticchio, V., Posa, F., Santoro, R., Sgura, I., Corsi, F., Venuto, D., Fratino, U., Marzocca, C., Xiaojian Li, Liu, Z., Lu, S., Lu, Z., Meng, Q., Sa, B., Yuan, J., Zhou, J., Zhou, S., Alme, J., Bablok, S., Klovning, A., Nystr, J., Pommeresche, B., Richter, M., Röhrich, D., Ullal, K., Yang, H., Helstrup, H., Hetl, K., Roed, K., Choudhury, R. K., Dubey, A. K., Mahapatra, D. P., Mishra, D., Phatak, S. C., Sahoo, R., Evans, D., Jones, G. T., Jovanovic, P., Jusko, A., Kinson, J. B., Lietava, R., Villalobos Baillie, O., Alici, A., Antinori, S., Antonioli, P., Arcelli, S., Bari, G., Basile, M., Bellagamba, L., Boscherini, D., Bruni, A., Bruni, G., Cara Romeo, G., Cifarelli, L., Cindolo, F., Corradi, M., Falchieri, D., Gabrielli, A., Gandolfi, E., Giusti, P., Hatzifotiadou, D., Laurenti, G., Luvisetto, M. L., Margotti, A., Masetti, M., Nania, R., Noferini, F., Palmonari, F., Pesci, A., Polini, A., Sartorelli, G., Scapparone, E., Scioli, G., Vacca, G. P., Valenti, G., Venturi, G., Zampolli, C., Zichichi, A., Cerny, V., Janik, R., Lucan, L., Pikna, M., Pisut, J., Pisutova, N., Sitar, B., Strmen, P., Szarka, I., Zagiba, M., Aiftimiei, C., Catanescu, V., Duma, M., Legrand, C. I., Moisa, D., Eric Denes, Fodor, Z., Kiss, T., Palla, G., Zimanyi, J., Atanassov, I., Basciu, S., Cicalo, C., Falco, A., Floris, M., Masoni, A., Mura, D., Puddu, G., Serci, S., Siddi, E., Usai, G., Badala, A., Barbera, R., Lo Re, G., Palmeri, A., Pappalardo, G. S., Pulvirenti, A., Riggi, F., Anelli, G., Augustin, I., Augustinus, A., Baechler, J., Belikov, J. A., Betev, L., Boccardi, A., Brun, R., Burns, M., Buncic, P., Cali, I., Campagnolo, R., Campbell, M., Carena, F., Carena, W., Carminati, F., Carrer, N., Chapel, S., Cheshkov, C., Chochula, P., Christianssen, P., Christakoglou, P., Colla, A., Conrad, J., Correia Belbute, B. F., Davenport, M., Cataldo, G., Groot, J., Di Mauro, A., Divia, R., Engster, C., Evrard, S., Fabjan, C. W., Formenti, F., Fuchs, U., Gallas-Torreira, A., Garcia Lopez, A., Gheata, A., Gheata, M., Gonzalez-Gutierrez, C., Grosso, R., Gruwe, M., A Gustafsson, H., Hoedelmoser, H., Hristov, P., Ivanov, M., Jacobs, P., Jirden, L., Junique, A., Kapusta, S., Kickinger, W., Klempt, W., Kluge, A., Kuhr, T., Leistam, L., Lo, J. P., Lopez Noriega, M., Lourenco, C., Makhlyueva, I., C Marin, J., Martinengo, P., Meunier-Picard, D., Meoni, M., Morel, M., Morsch, A., Mota, B., Muller, H., Musa, L., Nilsson, P., Nouais, D., Osmic, F., Perini, D., Peters, A., Pinto Morais, V., Popescu, S., Rademakers, F., P Revol, J., Riedler, P., Riegler, W., Safark, K., Saiz, P., Schossmaier, K., Schukraft, J., Schutz, Y., Silva Loureiro, P. A., Soos, C., Stefanini, G., Swoboda, D., Tadel, M., Taureg, H., Tavlet, M., Tissot-Daguette, P., Torcato Matos, C., Vande Vyvre, P., P Vanuxem, J., Aggarwal, M. M., Bhati, A. K., Kumar, A., Sharma, M., Sood, G., Baldit, A., Barret, V., Bastid, N., Blanchard, G., Castor, J., Crochet, P., Daudon, F., Devaux, A., Dupieux, P., Force, P., Forestier, B., Fabien Guérin, Guernane, R., Insa, C., François Jouve, Lecoq, J., Manso, F., Rosnet, P., Royer, L., Saturnini, P., Savinel, G., Stoicea, G., Yermia, F., Humanic, T. J., Kotov, I. V., Lisa, M., Nilsen, B. S., Truesdale, D., Johnson, D., Bearden, I., Boggild, H., Christensen, C. H., Gaardhoje, J. J., Gulbrandsen, K., Nielsen, B. S., Renault, G., Bartke, J., Gadysz-Dziadus, E., Kornas, E., Kowalski, M., Rybicki, A., Wroblewski, A., Andronic, A., Antonczyk, D., Badura, E., Bailhache, R., Berdermann, E., Braun-Munzinger, P., Busch, O., Ciobanu, M., Foka, P., Frankenfeld, U., Garabatos, C., Gutbrod, H., Lippmann, C., Malzacher, P., Marin, A., Miskowiec, D., Radomski, S., Schmidt, H. R., Schwarz, K., Sedykh, S., Simon, R. S., Soyk, D., Stelzer, H., Tziledakis, G., Vranic, D., Wiechula, J., Bonnes, U., Kraus, I., Oeschler, H., Berger, J., Billmeier, A., Blume, C., Dietel, T., Flierl, D., Gazdzicki, M., Kolleger, T., Lange, S., Loizides, C., Renfordt, R., Stock, R., Ströbele, H., Ya. Berdnikov, Khanzadeev, A., Miftakhov, N., Nikouline, V., Poliakov, V., Rostchine, E., Samsonov, V., Tarasenkova, O., Tarakanov, V., Zhalov, M., Lopez Torres, E., Abrahantes Quintana, A., Diaz Valdes, R., Angelov, V., Guteisch, M., Lindenstruth, V., Panse, R., Reichling, C., Schneider, R., Steinbeck, T., Tilsner, H., Wiebalck, A., Adler, C., Bielcikova, J., Emschermann, D., Glässel, P., Herrmann, N., Th. Lehmann, Ludolphs, W., Mahmoud, T., Milosevic, J., Oyama, K., Petrovici, M., Rusanov, I., Schicker, R., Soltveit, H. C., Stachel, J., Stockmeier, M., Vulpescu, B., Windelb, B., Yurevich, S., Sugitate, T., Bhardwaj, S., Raniwala, R., Raniwala, S., Badyal, S. K., Bhasin, A., Anupam Gupta, Gupta, V. K., Mahajan, S., Mangotra, L. K., Potukuchi, B. V. K. S., Sambyal, S. S., Akichine, P. G., Areev, V. A., Ts. Baatar, Batiounia, B. V., Chepurnov, V. F., Chernenko, S. A., Dodokhov, V. K., Fateev, O. V., Fedunov, A. G., Haiduc, M., Hasegan, D., Kadychevsky, V. G., Kharadze, G., Khurelbaatar, B., Koshurnikov, E. K., Lioubochits, V. L., Lobanov, V. I., Malinina, L. V., Minaev, Y. I., Nioradze, M., Nomokonov, P. V., Panebrattsev, Y. A., Penev, V. N., Pismennaya, V. G., Pocheptsov, T. A., Roufanov, I., Shabratova, G. S., Shestakov, V., Shklovskaya, A. I., Sorin, A. S., Suleimanov, M. K., Tevzadze, Y., Togoo, R., Vodopianov, A. S., Yurevich, V. I., Zanevsky, Y. V., Zaporojets, S. A., Zinchenko, A. I., Aysto, J., Bondila, M., Lyapin, V., Oinonen, M., Malkiewicz, T., Ruuskanen, V., Seppanen, H., Trzaska, W., Yamaletkinov, S., Jung, H. T., Jung, W., W Kim, D., Kim, H. N., Kim, J. S., Lee, K. S., C Lee, S., Blank, T., Gemmeke, H., Bochek, G. L., Dovbnya, A. N., Kulibaba, V. I., Maslov, N. I., Naumov, S. V., Ovchinnik, V. D., Potin, S. M., Starodubtsev, A. F., Borshchov, V. N., Chykalov, O., Kaurova, L., Kiprich, S. K., Klymova, L., Listratenko, O. M., Mykhaylova, N., Protsenko, M., Reznik, O., Starkov, V. E., Kadenko, I., Martynov, Y., Molodtsov, S., Sokolov, O., Sinyukov, Y., Zinovjev, G., Bhattacharya, P., Bose, S., Majumdar, N., Mukhopadhyay, S., Sanyal, A., Sarkar, S., Sen, P., Sen, S. K., Sinha, B. C., Sinha, T., Ahammed, Z., Bhaskar, P., Chattopadhyay, S., Das, D., Das, S., Dutta Majumdar, M. R., Ganti, M. S., Ghosh, P., Mohanty, B., Nayak, T. K., Netrakanti, P. K., Pal, S., Singaraju, R. N., Singhal, V., Sinha, B., Trivedi, M. D., Viyogi, Y. P., Hartung, G., Krawutschke, T., Ban, J., Bombara, M., Dirner, A., Fedor, S., Hnatic, M., Kralik, I., Kravcakova, A., Krivan, F., Krivda, M., Martinska, G., Pastircak, B., Sandor, L., Jakub Urban, Vrlakova, J., Cinausero, M., Fioretto, E., Prete, G., Ricci, R. A., Vannucci, L., Branco, P., Carvalho, R., Seixas, J., Vilela Mendes, R., Oskarsson, A., Osterman, L., Otterlund, I., Stenlund, E. A., Cheynis, B., Ducroux, L., Y Grossiord, J., Guichard, A., Philippe Pillot, Rapp, B., Tieulent, R., Alfaro Molina, J. R., Ayala, A., Belmont Moreno, E., Contreras, J. G., Cuautle, E., Olivo, J. C. D., Dominguez, I., Flores, A., Herrera Corral, G., Leon Monzon, I., Linares, M., Martinez Castro, J., Martinez, M. I., Martinez Davalos, A., Menchaca-Rocha, A., Montano Zetina, L. M., Nellen, L., Paic, G., Del Pino, J., Reyes, P., Sandoval, A., Solano, J., Vargas, M. A., Zepeda, A., Feshcenko, V. A., Golubeva, M. B., Gorlychev, V. G., Guber, F. F., Karavichev, O. V., Karavicheva, T. L., Karpechev, E. V., Kurepin, A. B., Maevskaya, A. I., Marin, V. V., Pshenichnov, I. A., Razin, V. I., Rechetin, A. I., Shileev, K. A., Topilskaia, N. S., Akindinov, A. N., Golovine, V., Kaidalov, A. B., Kats, M. M., Kiselev, I. T., Kisselev, S. M., Lioublev, E., Martemianov, M., Martemiyanov, A. N., Polozov, P. A., Serov, V. S., Smirnitski, A. V., Tchoumakov, M. M., Vetlitski, I. A., Volochine, K. G., Vorobiev, L. S., Zagreev, B. V., Aleksandrov, D., Antonenko, V., Beliaev, S., Fokine, S., Ippolitov, M., Karadjev, K., Lebedev, V., Manko, V. I., Moukhanova, T., Nianine, A., Nikolaev, S., Nikouline, S., Patarakine, O., Peressounko, D., Sibiriak, I., Tsvetkov, A., Vasiliev, A., Vinogradov, A., Volkov, M., Yushmanov, I., Grigoriev, V. A., Kaplin, V. A., Loginov, V. A., Nandi, B. K., Varma, R., Chandratre, V., Kataria, V., Cédric Baumann, Bucher, D., Glasow, R., Gottschlag, H., Grose-Oetringhaus, J. F., Heine, N., Klein-Bosing, C., Reygers, K., Santo, R., Verhoeven, W., Wessels, J., Wilk, A., Laurent Aphecetche, Barbet, J. M., Conesa-Balbastre, G., Conesa-Del-Valle, Z., Jean-Pierre Cussonneau, Delagrange, H., Dialinas, M., Finck, C., Erazmus, B., Marie Germain, Kabana, S., Lefevre, F., Luquin, L., Lilian Martin, Gines Martinez Garcia, Roy, C., Tournaire, A., Frolov, A. R., Pestov, I. N., Awes, T., Cherney, M., Bimbot, L., Chambert, V., Charpy, A., Comets, M. P., Courtat, P., Sebastien DROUET, Edelbruck, P., Espagnon, B., Hrivnacova, I., Kunne, R., Le Bornec, Y., Mac Cormick, M., Jean Peyré, Pouthas, J., Rousseau, S., Suire, C., Willis, N., Bravina, L., Løvhoiden, G., Skaali, B., Tveter, T. S., Vik, T., Antinori, F., Dainese, A., Dima, R., Fabris, D., Faivre, J., Lunardon, M., Morando, M., Moretto, S., Pepato, A., Quercigh, E., Scarlassara, F., Segato, G., Turrisi, R., Viesti, G., Choi, J., Beitlerova, A., Mares, J., Polak, K., Zavada, P., Petracek, V., Pachr, M., Skoda, L., Yu Bogolyubsky, M., Khaoustov, G. V., Kharlov, I. V., Minaev, N. G., Petrov, V. S., Polichtchouk, B. V., Sadovsky, S. A., Senko, V. A., Soloviev, A. S., Stolpovsky, P. V., Victorov, V. A., Fernandez Tellez, A., Gamez Flores, E., Lopez, R., Tejeda, G., Vergara, S., Adamova, D., Kouchpil, S., Kouchpil, V., Kugler, A., Sumbera, M., Wagner, V., Di Liberto, S., Mazzoni, M. A., Meddi, F., Urciuoli, G. M., Cleymans, J., Vaux, G., Fearick, R. W., Szostak, A., Vilakazi, Z. Z., Anfreville, M., Baldisseri, A., Becker, Bern W., Borel, H., L Charvet, J., Combet, M., Gosset, J., Hardy, P., Herlant, S., Orsini, F., Penichot, Y., Pereira, H., Salasca, S., Staley, F. M., Usseglio, M., Caro, A., Guarnaccia, C., Gruttola, D., Pasquale, S., Di Bartolomeo, A., Fusco Girard, M., Grella, G., Guida, M., Romano, G., Sellitto, S., Silvestri, R., Virgili, T., Basmanov, V., Budnikov, D., Demanov, V., Ianowski, V., Ilkaev, R., Ilkaeva, L., Ivanov, A., Khlebnikov, A., Kouryakin, A., Nazarenko, S., Pavlov, V., Philchagin, S., Punin, V., Poutevskoi, S., Selin, I., Vinogradov, I., Zhelezov, S., Zhitnik, A., Gotovac, S., Mudnic, E., Vidak, L., Braun, M. A., Feolov, G. A., Igolkin, S. N., Kolojvari, A. A., Kondratiev, V. P., Otyugova, P. A., Stolyarov, O. I., Toulina, T. A., Tsimbal, F. A., Valiev, F. F., Vechernin, V. V., Vinogradov, L. I., Baudot, J., Bonnet, D., Coffin, J. P., Hippolyte, B., Kuhn, C., Lutz, J. R., Vernet, R., Hamagaki, H., Ozawa, K., Bonvicini, V., Borysov, O., Bosisio, L., Bregant, M., Camerini, P., Contin, G., Faleschini, F., Fragiacomo, E., Grion, N., Margagliotti, G., Piano, S., Rachevskaya, I., Rachevski, A., Rui, R., Vacchi, A., Alessandro, B., Arnaldi, R., Guillaume Batigne, Beole, S., Bruna, E., Cerello, P., Chiavassa, E., Coli, S., Crescio, E., Marco, N., Ferretti, A., Gagliardi, M., Gallio, M., Gaudichet, L., Gemme, R., Giraudo, G., Giubellino, P., Idzik, M., Martoiu, S., Marzari Chiesa, A., Masera, M., Mazza, G., Mereu, P., Monteno, M., Musso, A., Oppedisano, C., Piccotti, A., Poggio, F., Prino, F., Riccati, L., Rivetti, A., Scomparin, E., Tosello, F., Toscano, L., Travaglia, G., Vercellin, E., Werbrouck, A., Wheadon, R., Miake, Y., Esumi, S., Botje, M., Buskop, J. J. F., Haas, A. P., Kamermans, R., Kuijer, P. G., Nooren, G., Oskamp, C. J., Th. Peitzmann, Simili, E., Snellings, R., Sokolov, A. N., Den Brink, A., Eijndhoven, N., Enyo, H., Fujiwara, K., Kano, H., Onishi, H., Deloff, A., Dobrowolski, T., Karpio, K., Kozlowski, M., Malinowski, H., Redlich, K., Siemiarczuk, T., Stefanek, G., Tykarski, L., Wilk, G., Chajecki, Z., Gos, H., Janik, M., Jedynak, M., Kisiel, A., Pawlak, T. J., Peryt, W. S., Pluta, J., Skowronski, P., Slodkowski, M., Szuba, P., Traczyk, T., Conner, E. S., Keidel, R., Cai, X., Wang, X. R., Wu, T., Yang, H. Y., Yin, Z. B., Zhou, D. C., Cao, X., Li, Q., Atayan, M., Grigoryan, A., Grigoryan, S., Gulkanyan, H., Harutyunyan, A., Hayrapetyan, A., Kakoyan, V., Poghosyan, M., Sargsyan, G., Anticic, T., Kadija, K., Susa, T., Laboratoire de Physique Corpusculaire - Clermont-Ferrand (LPC), Université Blaise Pascal - Clermont-Ferrand 2 (UBP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire de Lyon (IPNL), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), ALICE, Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches Subatomiques (IReS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Cancéropôle du Grand Est-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), and Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)
Subjects: [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]
Abstract: ALICE PHASE EI SEP ACC S2I
Published: 2005

35. ALICE Technical Design Report of the Computing

Author: Cortese, P., Dellacasa, G., Ramello, L., Sitta, M., Ahmad, N., Ahmad, S., Ahmad, T., Bari, W., Irfan, M., Zafar, M., Belogianni, A., Ganoti, P., Petridis, A., Roukoutakis, F., Spyropoulou-Stassinaki, M., Vassiliou, M., Bruno, G. E., Caselle, M., Di Bari, D., Elia, D., Fini, R. A., Ghidini, B., Lenti, V., Manzari, V., Nappi, E., Navach, F., Pastore, C., Paticchio, V., Posa, F., Santoro, R., Sgura, I., Corsi, F., Venuto, D., Fratino, U., Marzocca, C., Xiaojian Li, Liu, Z., Lu, S., Lu, Z., Meng, Q., Sa, B., Yuan, J., Zhou, J., Zhou, S., Alme, J., Bablok, S., Klovning, A., Nystr, J., Pommeresche, B., Richter, M., Röhrich, D., Ullal, K., Yang, H., Helstrup, H., Hetl, K., Roed, K., Choudhury, R. K., Dubey, A. K., Mahapatra, D. P., Mishra, D., Phatak, S. C., Sahoo, R., Evans, D., Jones, G. T., Jovanovic, P., Jusko, A., Kinson, J. B., Lietava, R., Villalobos Baillie, O., Alici, A., Antinori, S., Antonioli, P., Arcelli, S., Bari, G., Basile, M., Bellagamba, L., Boscherini, D., Bruni, A., Bruni, G., Cara Romeo, G., Cifarelli, L., Cindolo, F., Corradi, M., Falchieri, D., Gabrielli, A., Gandolfi, E., Giusti, P., Hatzifotiadou, D., Laurenti, G., Luvisetto, M. L., Margotti, A., Masetti, M., Nania, R., Noferini, F., Palmonari, F., Pesci, A., Polini, A., Sartorelli, G., Scapparone, E., Scioli, G., Vacca, G. P., Valenti, G., Venturi, G., Zampolli, C., Zichichi, A., Cerny, V., Janik, R., Lucan, L., Pikna, M., Pisut, J., Pisutova, N., Sitar, B., Strmen, P., Szarka, I., Zagiba, M., Aiftimiei, C., Catanescu, V., Duma, M., Legrand, C. I., Moisa, D., Eric Denes, Fodor, Z., Kiss, T., Palla, G., Zimanyi, J., Atanassov, I., Basciu, S., Cicalo, C., Falco, A., Floris, M., Masoni, A., Mura, D., Puddu, G., Serci, S., Siddi, E., Usai, G., Badala, A., Barbera, R., Lo Re, G., Palmeri, A., Pappalardo, G. S., Pulvirenti, A., Riggi, F., Anelli, G., Augustin, I., Augustinus, A., Baechler, J., Belikov, J. A., Betev, L., Boccardi, A., Brun, R., Burns, M., Buncic, P., Cali, I., Campagnolo, R., Campbell, M., Carena, F., Carena, W., Carminati, F., Carrer, N., Chapel, S., Cheshkov, C., Chochula, P., Christianssen, P., Christakoglou, P., Colla, A., Conrad, J., Correia Belbute, B. F., Davenport, M., Cataldo, G., Groot, J., Di Mauro, A., Divia, R., Engster, C., Evrard, S., Fabjan, C. W., Formenti, F., Fuchs, U., Gallas-Torreira, A., Garcia Lopez, A., Gheata, A., Gheata, M., Gonzalez-Gutierrez, C., Grosso, R., Gruwe, M., A Gustafsson, H., Hoedelmoser, H., Hristov, P., Ivanov, M., Jacobs, P., Jirden, L., Junique, A., Kapusta, S., Kickinger, W., Klempt, W., Kluge, A., Kuhr, T., Leistam, L., Lo, J. P., Lopez Noriega, M., Lourenco, C., Makhlyueva, I., C Marin, J., Martinengo, P., Meunier-Picard, D., Meoni, M., Morel, M., Morsch, A., Mota, B., Muller, H., Musa, L., Nilsson, P., Nouais, D., Osmic, F., Perini, D., Peters, A., Pinto Morais, V., Popescu, S., Rademakers, F., P Revol, J., Riedler, P., Riegler, W., Safark, K., Saiz, P., Schossmaier, K., Schukraft, J., Schutz, Y., Silva Loureiro, P. A., Soos, C., Stefanini, G., Swoboda, D., Tadel, M., Taureg, H., Tavlet, M., Tissot-Daguette, P., Torcato Matos, C., Vande Vyvre, P., P Vanuxem, J., Aggarwal, M. M., Bhati, A. K., Kumar, A., Sharma, M., Sood, G., Baldit, A., Barret, V., Bastid, N., Blanchard, G., Castor, J., Crochet, P., Daudon, F., Devaux, A., Dupieux, P., Force, P., Forestier, B., Fabien Guérin, Guernane, R., Insa, C., François Jouve, Lecoq, J., Manso, F., Rosnet, P., Royer, L., Saturnini, P., Savinel, G., Stoicea, G., Yermia, F., Humanic, T. J., Kotov, I. V., Lisa, M., Nilsen, B. S., Truesdale, D., Johnson, D., Bearden, I., Boggild, H., Christensen, C. H., Gaardhoje, J. J., Gulbrandsen, K., Nielsen, B. S., Renault, G., Bartke, J., Gadysz-Dziadus, E., Kornas, E., Kowalski, M., Rybicki, A., Wroblewski, A., Andronic, A., Antonczyk, D., Badura, E., Bailhache, R., Berdermann, E., Braun-Munzinger, P., Busch, O., Ciobanu, M., Foka, P., Frankenfeld, U., Garabatos, C., Gutbrod, H., Lippmann, C., Malzacher, P., Marin, A., Miskowiec, D., Radomski, S., Schmidt, H. R., Schwarz, K., Sedykh, S., Simon, R. S., Soyk, D., Stelzer, H., Tziledakis, G., Vranic, D., Wiechula, J., Bonnes, U., Kraus, I., Oeschler, H., Berger, J., Billmeier, A., Blume, C., Dietel, T., Flierl, D., Gazdzicki, M., Kolleger, T., Lange, S., Loizides, C., Renfordt, R., Stock, R., Ströbele, H., Ya. Berdnikov, Khanzadeev, A., Miftakhov, N., Nikouline, V., Poliakov, V., Rostchine, E., Samsonov, V., Tarasenkova, O., Tarakanov, V., Zhalov, M., Lopez Torres, E., Abrahantes Quintana, A., Diaz Valdes, R., Angelov, V., Guteisch, M., Lindenstruth, V., Panse, R., Reichling, C., Schneider, R., Steinbeck, T., Tilsner, H., Wiebalck, A., Adler, C., Bielcikova, J., Emschermann, D., Glässel, P., Herrmann, N., Th. Lehmann, Ludolphs, W., Mahmoud, T., Milosevic, J., Oyama, K., Petrovici, M., Rusanov, I., Schicker, R., Soltveit, H. C., Stachel, J., Stockmeier, M., Vulpescu, B., Windelb, B., Yurevich, S., Sugitate, T., Bhardwaj, S., Raniwala, R., Raniwala, S., Badyal, S. K., Bhasin, A., Anupam Gupta, Gupta, V. K., Mahajan, S., Mangotra, L. K., Potukuchi, B. V. K. S., Sambyal, S. S., Akichine, P. G., Areev, V. A., Ts. Baatar, Batiounia, B. V., Chepurnov, V. F., Chernenko, S. A., Dodokhov, V. K., Fateev, O. V., Fedunov, A. G., Haiduc, M., Hasegan, D., Kadychevsky, V. G., Kharadze, G., Khurelbaatar, B., Koshurnikov, E. K., Lioubochits, V. L., Lobanov, V. I., Malinina, L. V., Minaev, Y. I., Nioradze, M., Nomokonov, P. V., Panebrattsev, Y. A., Penev, V. N., Pismennaya, V. G., Pocheptsov, T. A., Roufanov, I., Shabratova, G. S., Shestakov, V., Shklovskaya, A. I., Sorin, A. S., Suleimanov, M. K., Tevzadze, Y., Togoo, R., Vodopianov, A. S., Yurevich, V. I., Zanevsky, Y. V., Zaporojets, S. A., Zinchenko, A. I., Aysto, J., Bondila, M., Lyapin, V., Oinonen, M., Malkiewicz, T., Ruuskanen, V., Seppanen, H., Trzaska, W., Yamaletkinov, S., Jung, H. T., Jung, W., W Kim, D., Kim, H. N., Kim, J. S., Lee, K. S., C Lee, S., Blank, T., Gemmeke, H., Bochek, G. L., Dovbnya, A. N., Kulibaba, V. I., Maslov, N. I., Naumov, S. V., Ovchinnik, V. D., Potin, S. M., Starodubtsev, A. F., Borshchov, V. N., Chykalov, O., Kaurova, L., Kiprich, S. K., Klymova, L., Listratenko, O. M., Mykhaylova, N., Protsenko, M., Reznik, O., Starkov, V. E., Kadenko, I., Martynov, Y., Molodtsov, S., Sokolov, O., Sinyukov, Y., Zinovjev, G., Bhattacharya, P., Bose, S., Majumdar, N., Mukhopadhyay, S., Sanyal, A., Sarkar, S., Sen, P., Sen, S. K., Sinha, B. C., Sinha, T., Ahammed, Z., Bhaskar, P., Chattopadhyay, S., Das, D., Das, S., Dutta Majumdar, M. R., Ganti, M. S., Ghosh, P., Mohanty, B., Nayak, T. K., Netrakanti, P. K., Pal, S., Singaraju, R. N., Singhal, V., Sinha, B., Trivedi, M. D., Viyogi, Y. P., Hartung, G., Krawutschke, T., Ban, J., Bombara, M., Dirner, A., Fedor, S., Hnatic, M., Kralik, I., Kravcakova, A., Krivan, F., Krivda, M., Martinska, G., Pastircak, B., Sandor, L., Jakub Urban, Vrlakova, J., Cinausero, M., Fioretto, E., Prete, G., Ricci, R. A., Vannucci, L., Branco, P., Carvalho, R., Seixas, J., Vilela Mendes, R., Oskarsson, A., Osterman, L., Otterlund, I., Stenlund, E. A., Cheynis, B., Ducroux, L., Y Grossiord, J., Guichard, A., Philippe Pillot, Rapp, B., Tieulent, R., Alfaro Molina, J. 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Z., Anfreville, M., Baldisseri, A., Becker, Bern W., Borel, H., L Charvet, J., Combet, M., Gosset, J., Hardy, P., Herlant, S., Orsini, F., Penichot, Y., Pereira, H., Salasca, S., Staley, F. M., Usseglio, M., Caro, A., Guarnaccia, C., Gruttola, D., Pasquale, S., Di Bartolomeo, A., Fusco Girard, M., Grella, G., Guida, M., Romano, G., Sellitto, S., Silvestri, R., Virgili, T., Basmanov, V., Budnikov, D., Demanov, V., Ianowski, V., Ilkaev, R., Ilkaeva, L., Ivanov, A., Khlebnikov, A., Kouryakin, A., Nazarenko, S., Pavlov, V., Philchagin, S., Punin, V., Poutevskoi, S., Selin, I., Vinogradov, I., Zhelezov, S., Zhitnik, A., Gotovac, S., Mudnic, E., Vidak, L., Braun, M. A., Feolov, G. A., Igolkin, S. N., Kolojvari, A. A., Kondratiev, V. P., Otyugova, P. A., Stolyarov, O. I., Toulina, T. A., Tsimbal, F. A., Valiev, F. F., Vechernin, V. V., Vinogradov, L. I., Baudot, J., Bonnet, D., Coffin, J. P., Hippolyte, B., Kuhn, C., Lutz, J. 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Subjects: [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]
Abstract: ALICE, EI PHASE SEP
Published: 2005

36. ATLAS calorimeter performance

Author: Airapetian, A., Grabsky, V., Hakopian, H., Vartapetian, A., Fares, F., Moorhead, G. F., Sevior, M. E., Taylor, G. N., Tovey, S. N., Alexiev, D., Donnelly, I. J., Varvell, K. E., Williams, M. L., Hashemi-Nezhad, R., Peak, L., Saavedra, A., Ulrichs, J., Girtler, P., Kiener, C., Kneringer, E., Kuhn, D., Rudolph, G., Abdinov, O. B., Aliev, F. M., Khalilzade, F. T., Mekhdiev, R. R., Rzaev, H. J., Usubov, Z. U., Baturitsky, M. A., Bogush, A. A., Demchenko, A. I., Gazizov, A. Z., Gilevsky, V. V., Golubev, V. S., Levchuk, M. I., Satsunkevich, I. S., Shevtsov, V. V., Caloba, L. P., Galvez-Durand, F., Maidantchik, C. L., Marroquin, F., Seixas, J. M., Thome, Z. D., Da Silva, N. C., Dietzsch, O., Leite, M. A. L., Sakanoue, M. H., Takagui, E. M., Zandona, F., Armstrong, W. W., Burris, W., Gingrich, D. M., Hewlett, J. C., Holm, L., Mullin, S., Pinfold, J. L., Schaapman, J., Soukup, J., Wampler, L., Axen, D., Mayer, J. K., Orr, R. S., Armitage, J., Dixit, M., Dubeau, J., Estabrooks, P., Losty, M., Neuheimer, E., Neill, M. O., Oakham, G., Azuelos, G., Ben El Fassi, A., Depommier, P., Leon-Florian, E., Leroy, C., Lorazo, B., P Martin, J., Marullo, F., Pascal Roy, Savard, P., Bailey, D. C., Bhadra, S., Martin, J. F., Sinervo, P. K., Stairs, G. G., Trischuk, W., Astbury, A., Birney, P., Hodges, T., Langstaff, R., Oram, C., Roberts, B., Rosvick, M., Wellisch, H. P., Bishop, S., Fincke-Keeler, M., Honma, A., Keeler, R., Lefebvre, M., Neil, D. O., Poffenberger, P., Robertson, L., Roney, M., Sobie, R., Akesson, T., Anghinolfi, F., Bachy, G., Barberio, E., Benincasa, G., Bergsma, F., Bjorset, L., Blocki, J., Bloess, D., Bock, R., Bogaerts, J., Brawn, I., Burckhart, H. J., Butin, F., Campbell, M., Chesi, E., Chevalley, J. L., Christiansen, J., Cobal, M., Dabrowski, W., Dauvergne, J. P., Acqua, A., Eric Denes, Dittus, F., Dobinson, R., Drakoulakos, D., Dufey, J. P., Eerola, P., Efthymiopoulos, I., Ellis, N., Fabjan, C. W., Farthouat, P., Flegel, W., Francis, D., Froidevaux, D., Gebart, R., Gianotti, F., Gildemeister, O., Hatch, M., Haug, F., Hauviller, C., Heeley, R., Heijne, E., Henriques, A., Hoffmann, H. F., Hortnagl, C., Jarp, S., Jarron, P., Jenni, P., Jones, R., Kantardjian, G., Kaplon, J., Klempt, W., Klyuchnikova, T., Knobloch, J., Koski, K., Kotz, U., Lacasta, C., Langhans, W., Lasseur, C., Lehraus, I., Lemeilleur, F., Lichard, P., Liebhart, M., Linde, F., Lofstedt, B., Madsen, N., Mapelli, L., Marchioro, A., Martin, B., Maugin, J. M., Mclaren, R. A., Meier, D., Michelotto, M., Mornacchi, G., Myers, D., Nessi, M., Nicquevert, B., Onions, C., Patel, A., Poggioli, L., Poppleton, A., Posch, C., Poulard, G., Price, M., Riedler, P., Riegler, W., Roe, S., Rohrbach, F., Rosso, E., Rudge, A., Ryzhov, V., Schaller, M., Schmid, P., Schmitt, M., Schuler, G., Snoeys, W., Spegel, M., Spiwoks, R., Stavrianakou, M., Stavropoulos, G., Tartarelli, F., Ben Taylor, Ten Kate, H., Treichel, M., Tsesmelis, E., Bij, H., Vasey, F., Boehn-Bucholz, R., Voss, R., Vreeswijk, M., Vuillemin, V., Weilhammer, P., Wendler, H., Werner, P., Witzeling, W., Wotschack, J., Bohm, J., Hrivnac, J., Lednicky, R., Lokajicek, M., Nemecek, S., Sicho, P., Simak, V., Stastny, J., Stedron, M., Vanickova, M., Vrba, V., Davidek, T., Dolejsi, J., Dolezal, Z., Kucera, M., Leitner, R., Soustruznik, K., Suk, M., Tas, P., Trka, Z., Valkar, S., Wilhelm, I., Zdrazil, M., Jakubek, J., Kubasta, J., Macha, I., Ota, J., Pospisil, S., Sinor, M., Sopko, B., Tomiak, Z., Dam, M., Hansen, J. D., Hansen, J. R., Hansen, P., Rensch, B., Jalas, P., Schulman, T., Aubert, B., Colas, J., Eynard, G., Jezequel, S., Linossier, O., Massol, N., Minard, M. N., Nicoleau, S., Perrodo, P., Sauvage, G., Wingerter, I., Zitoun, R., Zolnierowski, Y., Ziad Ajaltouni, Badaud, F., Bouhemaid, N., Brette, P., Brossard, M., Chadelas, R., Chevaleyre, J. C., Crouau, M., Daudon, F., Dugne, J. J., Michel, B., Gerard Montarou, S Muanza, G., Pallin, D., Plothow-Besch, H., Poirot, S., Reinmuth, G., Says, L. P., Vazeille, F., Andrieux, M. L., Ballon, J., Collot, J., Daniel Dzahini, Guerre Chaley, B., Hostachy, J. Y., Laborie, G., Martin, P., Pouxe, J., Rabier, C., Rey-Campagnolle, M., Rossetto, O., Saintignon, P., Stassi, P., Wielers, M., Basa, S., Blanquart, L., Bonzom, V., Calzas, A., Chekhtman, A., Clemens, J. C., Cohen-Solal, M., Cousinou, M. C., Dargent, P., Delpierre, P., Dinkespiler, B., Duval, P. 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R., Payne, B. T., Perera, V. J. O., Phillips, P. W., Pilling, A., Quinton, S. P. H., Saunders, B. J., Seller, P., Shah, T. P., Tappern, G. J., Tyndel, M., White, D. J., Wickens, F. J., Booth, C. N., Buttar, C. M., Cartwright, S. L., Combley, F. H., Lehto, M. H., Sellin, P. J., Spooner, N. J. C., Thompson, L. F., Alam, M. S., Athar, S. B., Mahmood, A., Ovunc, S., Severini, H., Timm, S., Wappler, F., Zhichao, L., Berger, E. L., Blair, R., Dawson, J., Guarino, V., Hill, N., May, E. N., Nodulman, L. J., Price, L. E., Proudfoot, J., Schlereth, J. L., Stanek, R., Wagner, R. G., Wicklund, A. B., Cheu, E., Johns, K., Loch, P., Rutherfoord, J., Savin, A., Shaver, L., Shupe, M., Steinberg, J., Tompkins, D., K. De, Gallas, E., Li, J., Sawyer, L., Stephens, R., White, A., Barnett, M., Bintinger, D., Ciocio, A., Dahl, O., Einsweiler, K., Ely, R., Gilchriese, M., Haber, C., Hinchliffe, I., Holland, S., Joshi, A., Kipnis, I., Kleinfelder, S., Milgrome, O., Nygren, D., Palaio, N., Pengg, F., Shapiro, M., Siegrist, J., Spieler, H., Trilling, G., Hazen, E., Shank, J., Simmons, E., Whitaker, J. S., Zhou, B., Behrends, S., Bensinger, J. R., Blocker, C., Cunningham, J., Kirsch, L. E., Lamoureux, J., Wellenstein, H., Citterio, M., Cullen, J., Gibbard, B., Gordeev, A., Gordon, H., Graf, N., Grachev, V., Kandasamy, A., Kotcher, J., Lissauer, D., Ma, H., Makowiecki, D., Murtagh, M. J., Connor, P. O., Paige, F., Polychronakos, V., Protopopescu, S., Radeka, V., Rahm, D. C., Rajagopalan, S., Rescia, S., Smith, G., Sondericker, J., Stephani, D., Stumer, I., Takai, H., Chernyatin, V., Yu, B., Anderson, K., Blucher, E., Evans, H., Glenzinski, D., Merritt, F., Oreglia, M., Pilcher, J., Pod, E., Sanders, H., Shochet, M., Turcot, A., Cartiglia, N., Cunitz, H., Dodd, J., Gara, A., Leltchouk, M., Parsons, J., Seman, M., Shaevitz, M., Sippach, W., Willis, W., Fortney, L. R., Goshaw, A. T., Lee, A. M., Oh, S. H., Robertson, R. J., Wang, C. H., Wesson, D., Baker, K., Feldman, G. J., Franklin, M. E. B., Huth, J., Oliver, J., Hanson, G., Zhenyu Li, Luehring, F., Ogren, H., Rust, D. R., Lankford, A. J., Hackett, C., Pier, S., Schernau, M., Stoker, D., Haridas, P., Osborne, L. S., Paradiso, J. A., Pless, I. A., Taylor, F. E., Wadsworth, B. F., Abolins, M., Brock, R., Bromberg, C., Edmunds, D., Yu. Ermolin, Gross, S., Huston, J., Laurens, P., Linnemann, J., Miller, R., Owen, D., Pope, B. 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M., Reinhall, P., Rothberg, J., Wasserbaech, S., Zhao, T., Fasching, D., Gonzalez, S., Jared, R. C., Pan, Y. B., Scott, I. J., Walsh, J., Wu, S. L., Yamartino, J. M., Zobernig, G., Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Corpusculaire - Clermont-Ferrand (LPC), Université Blaise Pascal - Clermont-Ferrand 2 (UBP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), ATLAS, and Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)
Subjects: [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
Published: 1996

37. ATLAS computing technical proposal

Author: Airapetian, A., Grabsky, V., Hakopian, H., Vartapetian, A., Fares, F., Moorhead, G. F., Sevior, M. E., Taylor, G. N., Tovey, S. N., Alexiev, D., Donnelly, I. J., Varvell, K. E., Williams, M. L., Hashemi-Nezhad, R., Peak, L., Saavedra, A., Ulrichs, J., Girtler, P., Kiener, C., Kneringer, E., Kuhn, D., Rudolph, G., Abdinov, O. B., Aliev, F. M., Khalilzade, F. T., Mekhdiev, R. R., Rzaev, H. J., Usubov, Z. U., Baturitsky, M. A., Bogush, A. A., Demchenko, A. I., Gazizov, A. Z., Gilevsky, V. V., Golubev, V. S., Levchuk, M. I., Satsunkevich, I. S., Shevtsov, V. V., Caloba, L. P., Galvez-Durand, F., Maidantchik, C. L., Marroquin, F., Seixas, J. M., Thome, Z. D., Da Silva, N. C., Dietzsch, O., Leite, M. A. L., Sakanoue, M. H., Takagui, E. M., Zandona, F., Armstrong, W. W., Burris, W., Gingrich, D. M., Hewlett, J. C., Holm, L., Mullin, S., Pinfold, J. L., Schaapman, J., Soukup, J., Wampler, L., Axen, D., Mayer, J. K., Orr, R. S., Armitage, J., Dixit, M., Dubeau, J., Estabrooks, P., Losty, M., Neuheimer, E., Neill, M. O., Oakham, G., Azuelos, G., Ben El Fassi, A., Depommier, P., Leon-Florian, E., Leroy, C., Lorazo, B., P Martin, J., Marullo, F., Pascal Roy, Savard, P., Bailey, D. C., Bhadra, S., Martin, J. F., Sinervo, P. K., Stairs, G. G., Trischuk, W., Astbury, A., Birney, P., Hodges, T., Langstaff, R., Oram, C., Roberts, B., Rosvick, M., Wellisch, H. P., Bishop, S., Fincke-Keeler, M., Honma, A., Keeler, R., Lefebvre, M., Neil, D. O., Poffenberger, P., Robertson, L., Roney, M., Sobie, R., Akesson, T., Anghinolfi, F., Bachy, G., Barberio, E., Benincasa, G., Bergsma, F., Bjorset, L., Blocki, J., Bloess, D., Bock, R., Bogaerts, J., Brawn, I., Burckhart, H. J., Butin, F., Campbell, M., Chesi, E., Chevalley, J. L., Christiansen, J., Cobal, M., Dabrowski, W., Dauvergne, J. P., Acqua, A., Eric Denes, Dittus, F., Dobinson, R., Drakoulakos, D., Dufey, J. P., Eerola, P., Efthymiopoulos, I., Ellis, N., Fabjan, C. W., Farthouat, P., Flegel, W., Francis, D., Froidevaux, D., Gebart, R., Gianotti, F., Gildemeister, O., Hatch, M., Haug, F., Hauviller, C., Heeley, R., Heijne, E., Henriques, A., Hoffmann, H. F., Hortnagl, C., Jarp, S., Jarron, P., Jenni, P., Jones, R., Kantardjian, G., Kaplon, J., Klempt, W., Klyuchnikova, T., Knobloch, J., Koski, K., Kotz, U., Lacasta, C., Langhans, W., Lasseur, C., Lehraus, I., Lemeilleur, F., Lichard, P., Liebhart, M., Linde, F., Lofstedt, B., Madsen, N., Mapelli, L., Marchioro, A., Martin, B., Maugin, J. M., Mclaren, R. A., Meier, D., Michelotto, M., Mornacchi, G., Myers, D., Nessi, M., Nicquevert, B., Onions, C., Patel, A., Poggioli, L., Poppleton, A., Posch, C., Poulard, G., Price, M., Riedler, P., Riegler, W., Roe, S., Rohrbach, F., Rosso, E., Rudge, A., Ryzhov, V., Schaller, M., Schmid, P., Schmitt, M., Schuler, G., Snoeys, W., Spegel, M., Spiwoks, R., Stavrianakou, M., Stavropoulos, G., Tartarelli, F., Ben Taylor, Ten Kate, H., Treichel, M., Tsesmelis, E., Bij, H., Vasey, F., Boehn-Bucholz, R., Voss, R., Vreeswijk, M., Vuillemin, V., Weilhammer, P., Wendler, H., Werner, P., Witzeling, W., Wotschack, J., Bohm, J., Hrivnac, J., Lednicky, R., Lokajicek, M., Nemecek, S., Sicho, P., Simak, V., Stastny, J., Stedron, M., Vanickova, M., Vrba, V., Davidek, T., Dolejsi, J., Dolezal, Z., Kucera, M., Leitner, R., Soustruznik, K., Suk, M., Tas, P., Trka, Z., Valkar, S., Wilhelm, I., Zdrazil, M., Jakubek, J., Kubasta, J., Macha, I., Ota, J., Pospisil, S., Sinor, M., Sopko, B., Tomiak, Z., Dam, M., Hansen, J. D., Hansen, J. R., Hansen, P., Rensch, B., Jalas, P., Schulman, T., Aubert, B., Colas, J., Eynard, G., Jezequel, S., Linossier, O., Massol, N., Minard, M. N., Nicoleau, S., Perrodo, P., Sauvage, G., Wingerter, I., Zitoun, R., Zolnierowski, Y., Ziad Ajaltouni, Badaud, F., Bouhemaid, N., Brette, P., Brossard, M., Chadelas, R., Chevaleyre, J. C., Crouau, M., Daudon, F., Dugne, J. J., Michel, B., Gerard Montarou, S Muanza, G., Pallin, D., Plothow-Besch, H., Poirot, S., Reinmuth, G., Says, L. P., Vazeille, F., Andrieux, M. L., Ballon, J., Collot, J., Daniel Dzahini, Guerre Chaley, B., Hostachy, J. Y., Laborie, G., Martin, P., Pouxe, J., Rabier, C., Rey-Campagnolle, M., Rossetto, O., Saintignon, P., Stassi, P., Wielers, M., Basa, S., Blanquart, L., Bonzom, V., Calzas, A., Chekhtman, A., Clemens, J. C., Cohen-Solal, M., Cousinou, M. C., Dargent, P., Delpierre, P., Dinkespiler, B., Duval, P. Y., Etienne, F., Fallou, A., Fassnacht, P., Ferrato, D., Fouchez, D., Gally, Y., Grigorev, E., Habrard, M. C., Hallewell, G., Le Suu, A., Lilian Martin, Mekkaoui, A., Monnier, E., Mouthuy, T., Nacasch, R., Nagy, E., Olivetto, C., Pouit, L., Qian, Z., Raymond, M., Rondot, C., Rozanov, A., Sauvage, D., Tisserant, S., Touchard, F., Vacavant, L., Ardelean, J., Arnault, C., Auge, E., Barrand, G., Belot, G., Bouchel, M., Boucrot, J., Breton, D., Chollet, C., Coulon, J. P., christophe de La Taille, Delebecque, P., Ducorps, A., Fayard, L., Fournier, D., Gonzales, J., Grivaz, J. F., Hrisoho, A., Iconomidou-Fayard, L., Imbert, P., Jacquier, Y., Jean, P., Lavigne, B., Mace, G., Martin-Chassard, G., Merkel, B., Nikolic, I., Noppe, J. M., Parrour, G., Petroff, P., Puzo, P., Richer, J. P., Schaffer, A. C., Seguin-Moreau, N., Serin, L., Tisserand, V., Togat, V., Unal, G., Vales, F., Veillet, J. J., Vernay, E., Alexanian, H., Baubillier, M., Bezamat, J., Billoir, P., Blouzon, F., Canton, B., David, J., Genat, J. F., Imbault, D., Le Dortz, O., Nayman, P., Rossel, F., Savoy-Navarro, A., Schwemling, P., Belorgey, J., Bernard, R., Berriaud, C., Berthier, R., Borgeaud, P., Bourdinaud, M., Bystricky, J., Calvet, D., Chalifour, M., Chevalier, L., Cloue, O., Dael, A., Delagnes, E., Desages, F., Desportes, H., Ernwein, J., Gachelin, O., Gallet, B., Giacometti, J., Girolamo, P., Gosset, L., Guyot, C., Hansl-Kozanecka, T., Heitzmann, J., Hubbard, J. R., Huet, M., Kozanecki, W., Laporte, J. F., Le Du, P., Lesmond, C., Lottin, J. P., Lugiez, F., Mandzhavidze, I., Mansoulie, B., Mayri, C., Molinie, F., Mur, M., Pabot, Y., Pailler, P., Pascual, J., Pelle, J., Perrin, P., Pinabiau, M., Renardy, J. F., Schuller, J. P., Schune, P., Schwindling, J., Simion, S., Smizanska, M., Taguet, J. P., Teiger, J., Thooris, B., Tirler, R., Hille, H., Veenhof, R., Veyssiere, C., Virchaux, M., Walter, C., Chikovani, L., Gabuniya, L., Gogiberidze, G., Gogoladze, G., Grigalashvili, T., Khorguashvili, Z., Kipiani, K., Koshtoev, V., Sopromadze, D., Topchishvili, L., Tvalashvili, O., Chiladze, B., Dzhobava, T., Khelashvili, A., Zh. Khubua, Liparteliani, A., Metreveli, Z., Mosidze, M., Salukvadze, R., Desch, K., Fischer, P., Geich-Gimbel, C., Hilger, E., Meuser, S., Ockenfels, W., Raith, B., Wermes, N., Becker, C., Fuss, J., Gossling, C., Lisowski, B., Luthaus, P., Wunstorf, R., Bar, T., Jie Chen, Ebling, D. G., Goppert, R., Herten, G., Irsigler, R., Kollefrath, M., Kolpin, R., Landgraf, U., Lauxtermann, S., Ludwig, J., Mohr, W., Paschhoff, V., Rehmann, V., Rolker, B., Runge, K., Schafer, F., Scherberger, G., Schmid, T., Webel, M., Weber, C., Geweniger, C., Hanke, P., Kluge, E. E., Mass, A., Putzer, A., Tittel, K., Wunsch, M., Doersing, V., Erhard, W., Kammel, P., Reinsch, A., Buchholz, P., Hoelldorfer, F., Jakobs, K., Kleinknecht, K., Kopke, L., Marschalkowski, E., Merle, K., Othegraven, R., Renk, B., Schafer, U., Schue, Y., Walkowiak, W., Hoegl, H., Kugel, A., Ludvig, J., Manner, R., Noffz, K. H., Ruehl, S., Zoz, R., Deile, M., Dubbert, J., Faessler, M. A., Hessey, N. P., Sammer, T., Staude, A., Trefzger, T., Ackermann, K., Aderholz, M., Andricek, L., Blum, W., Bratzler, U., Brettel, H., Dietl, H., Dulny, B., Dydak, F., Fent, J., Gruhn, C., Hauff, D., Koffeman, E., Kroha, H., Lutz, G., Manz, A., Moser, H. G., Oberlack, H., Ostapchuk, A., Richter, R., Richter, R. H., Schacht, P., Schael, S., Stenzel, H., Striegel, D., Tribanek, W., Gillessen, G., Holder, M., Kreutz, A., Becks, K. H., Braun, H., Drees, J., Glitza, K. W., Hamacher, K., Kersten, S., Lenzen, G., Linder, C., Middelkamp, P., Wahlen, H., Dris, M., Filippas, A., Fokitis, E., Gazis, E., Katsoufis, E., Maltezos, S., Papadopoulou, T., Giokaris, N., Ioannou, P., Kourkoumelis, C., Papadopoulos, I., Tatsis, S., Tzanakos, G. S., Bouzakis, C., Chardalas, M., Chouridou, S., Dedoussis, S., Gavris, G., Lagouri, T., Liolios, A., Paschalias, P., Petridou, C., Sampsonidis, D., Sergiadis, G., Zamani, M., Dado, S., Goldberg, J., Lupu, N., Abramowicz, H., Alexander, G., Bella, G., Benary, O., Dagan, S., Grunhaus, J., Oren, Y., Breskin, A., Chechik, R., Duchovni, E., Eisenberg, Y., Gross, E., Hass, M., Karshon, U., Lellouch, D., Levinson, L., Mikenberg, G., Revel, D., Arneodo, M., Ayad, R., Capua, M., La Rotonda, L., Liguori, D., Schioppa, M., Susinno, G., Valdata-Nappi, M., Bilokon, H., Chiarella, V., Curatolo, M., Esposito, B., Ferrer, M. L., Maccarrone, G., Pace, E., Pepe-Altarelli, M., Spitalieri, M., Zuffranieri, F., Barberis, D., Bozzo, M., Caso, C., Dameri, M., Darbo, G., Gagliardi, G., Gemme, C., Morettini, P., Musico, P., Olcese, M., Osculati, B., Parodi, F., Pozzo, A., Ridolfi, G., Rossi, L., Sette, G., Cesaroni, F., Creti, P., Gorini, E., Grancagnolo, F., Palamara, O., Panareo, M., Petrera, S., Primavera, M., Battistoni, G., Bellini, G., Bonivento, W., Camin, D., Cavalli, D., Costa, G., Angelo, P. D., Fedyakin, N. N., Anthony Ferrari, Cozzi, L., Labanca, N., Mandelli, L., Mazzanti, M., Menasce, D., Milazzo, L., Moroni, L., Pedrini, D., Perasso, L., Perini, L., Resconi, S., Sala, P., Sala, S., Di Corato, M., Aloisio, A., Alviggi, M. G., Cevenini, F., Chiefari, G., Asmundis, R., Drago, E., Merola, L., Napolitano, M., Patricelli, S., Cambiaghi, M., Caselotti, G., Conta, C., Ferrari, R., Fraternali, M., Lanza, A., Livan, M., Polesello, G., Rimoldi, A., Bellettini, G., Bosi, F., Cavasinni, V., Cologna, S., Costanzo, D., Santo, A., Pretet. Del, Di Girolamo, B., Flaminio, V., Lami, S., Latino, G., Mazzoni, E., Paoletti, R., Raffaelli, F., Renzoni, G., Rizzi, D., Bagnaia, P., Bini, C., Caloi, R., Cavallari, A., Ciapetti, G., Zorzi, G., Falciano, S., Gauzzi, P., Gentile, S., Lacava, F., Luminari, L., Nisati, A., Oberson, P., Petrolo, E., Pontecorvo, L., Zanello, L., Camarri, P., Cardarelli, R., Di Ciaccio, A., Santonico, R., Bacci, C., Ceradini, F., Orestano, D., Pastore, F., Cauz, D., Auria, S. D., Angelis, A., Pauletta, G., Santi, L., Scuri, F., Waldner, F., Del Papa, C., Kawaguti, M., Tanaka, S., Asai, M., Iwata, Y., Ohsugi, T., Amako, K., Arai, Y., Fujii, H., Ikeno, M., Iwasaki, H., Kanzaki, J., Kohriki, T., Kondo, T., Manabe, A., Morita, Y., Nomachi, M., Ohska, T. K., Sasaki, O., Sasaki, T., Terada, S., Unno, Y., Watase, Y., Yamamoto, A., Yasu, Y., Kawagoe, K., Nozaki, M., Takeda, H., Takashima, R., Nagamatsu, M., Yoshida, H., Takeshita, T., Hasegawa, Y., Imori, M., Kawamoto, T., Kobayashi, T., Hamatsu, R., Emura, T., Boos, E., Pokrovsky, N., Zhautykov, B., Chakir, H., Cherkaoui, R., Hoummada, A., Saidi, H., Sayouty, E., Bakker, F. E., Bobbink, G. J., Bos, K., Boterenbrood, H., Buis, E. J., Dankers, R. J., Daum, C., Groenstege, H., Hartjes, F., Hendriks, P., Heubers, W., Kaan, B., Kieft, G. N. M., Kluit, R., Massaro, G. G. G., Meddeler, G., Metselaar, J., Rewiersma, P. A. M., Schuijlenburg, H., Spelt, J., Vermeulen, J. C., Werneke, P., Woudstra, M., Eijk, B., Graaf, H., Bergman, R., Brouwer, C., Crijns, F. J. G. H., Dijkema, J. A., Kittel, W., Klok, P. F., Konig, A. C., Metzger, W. J., Pols, C. L. A., Schotanus, D. J., Visser, E. J., Wijnen, T. A. M., Eigen, G., Frodesen, A. G., Klovning, A., Stugu, B., Bugge, L., Buran, T., Kristiansen, H., Nygard, E., Stapnes, S., Gadomski, S., Godlewski, J., Hajduk, Z., Kisielewski, B., Korcyl, K., Malecki, P., Moszczynski, A., Olszowska, J., Richter-Was, E., Sobala, A., Grybos, P., Idzik, M., Jagielski, S., Jelen, K., Kisielewska, D., Kowalski, T., Lisbon, E., Amorim, A., Carvalho, J., Casarejos, E., David, M., Gomes, A., Gomes, J., Maio, A., Maneira, M., Martins, J. P., Onofre, A., Pinhao, J., Santos, J., Silva, J., Varandas, M., Wolters, H., Arsenescu, R., Boldea, V., Caprini, I., Caprini, M., Constantin, F., Constantinescu, S., Dita, P., Dita, S., Legrand, I. C., Maniu, G., Micu, L., Niculescu, M., Pantea, D., Popeneciu, G., Serban, T., Artamonov, A., Epstein, V., Gorbunov, P., Gurin, R., Zhemanov, V., Khovansky, V., Kuchenkov, A., Kruchinin, S., Maslennikov, A., Ryabinin, M., Shatalov, P., Tsukerman, I., Zaitsev, V., Zeldovich, S., Akimov, A., Baranov, S. P., Belov, M., Blagov, M., Gavrilenko, I., Komar, A., Konovalov, S., Kopytin, M., Muravev, S., Popov, L., Shikanian, A., Shmeleva, A., Snesarev, A., Speransky, M., Sulin, V., Tikhomirov, V., Vasileva, L., Yakimenko, M., Bondarenko, V., Dolgoshein, B., Konstantinov, A., Nevsky, P., Romanyuk, A., Semenov, S., Smirnov, S., Sosnovtsev, V., Bashindzhagian, G. L., Basiladze, S. G., Chudakov, E. A., Erasov, A. B., Ya. Grishkevich, Karmanov, D. E., Kramarenko, V. A., Larichev, A. N., Melikhov, D. I., Merkin, M. M., Nikitin, N. V., Rizatdinova, F. K., Selikov, A. V., Yu Sivoklokov, S., Smirnova, L. N., Yu Zhukov, V., Zverev, E. G., Batrakov, A., Chilingarov, A., Fedotov, M., Gaponenko, I., Klimenko, S., Kollegov, M., Kozlov, V., Kuper, E., Yu. Merzlyakov, Panin, V., Shamov, A., Telnov, V., Yu. Tikhonov, Yu. Velikzhanin, Amelin, D. V., Ammosov, V. V., Antipov, Yu M., Batarin, V., Yu Bogolyubsky, M., Borisov, A. A., Borisov, E., Bozhko, N. I., Bryzgalov, V. V., Chekulaev, S. V., Denisov, S. P., Yu Dushkin, A., Fakhrutdinov, R., Fenyuk, A. B., Gapienko, V. A., Gilitsky, Yu V., Goryachev, V., Gouz, Yu P., Karyukhin, A. N., Khokhlov, Yu A., Kirsanov, M. M., Klyukhin, V., Kozhin, A. S., Kononov, A. I., Konstantinov, V., Kopikov, S. V., Korotkov, V. A., Kostrikov, M. E., Kostyukhin, V. V., Kravtsov, V. I., Kulemzin, A., Kurchaninov, L. L., Lapin, V. V., Levitsky, M. L., Los, S., Maksimov, V., Myagkov, A. G., Mikhailin, V. N., Minaenko, A. A., Moiseev, A. M., Onuchin, V. A., Pleskach, A. V., Salomatin, Yu I., Senko, V. A., Shein, I., Soldatov, A. P., Solodkov, A. A., Solovyanov, O. V., Starchenko, E. A., Yu. Sviridov, Sytnik, V. V., Chmil, V., Chuntonov, A., Tikhonov, V. V., Yu. Tsyupa, Usenko, E., Vorobev, A. P., Vovenko, A. S., Zaets, V. G., Zaitsev, A. M., Zimin, S., Zmushko, V., Fedin, O., Filimonov, V., Gavrilov, G., Ivochkin, V., Khomutnikov, V., Kolos, S., Krivshich, A., Lochak, I., Maleev, V., Nadtochy, A., Patrichev, S., Prokofev, D., Yu. Ryabov, Shchegelsky, V., Solovev, I., Spiridenkov, E., Zalite, A., Aleksandrov, I., Alekseev, G., Alikov, B., Anosov, V., Astvatsaturov, A., Azhgirei, L., Bannikov, A., Baranov, S. A., Boyko, I., Yu. Budagov, Chelkov, G., Cheplakov, A., Chirikov-Zorin, I., Chlachidze, G., Dodonov, V., Feshchenko, A., Flyagin, V., Glagolev, V., Golikov, V., Golubykh, S., Yu. Gornushkin, Ignatenko, M., Zhuravlev, N., Kakurin, S., Kalinichenko, V., Kazarinov, M., Kazymov, A., Kekelidze, V., Khasanov, A., Khomenko, B., Khovansky, N., Kotov, V., Kovtun, V., Krumshtein, Z., Kukhtin, V., Yu. Kulchitsky, Kuznetsov, O., Ladygin, E., Lazarev, A., Lebedev, A., Lyablin, M., Yu. Lomakin, Malyshev, V. L., Malyukov, S., Yu. Merekov, Merzlyakov, S., Minashvili, I., Nikolenko, M., Nozdrin, A., Obudovsky, V., Olshevsky, A., Peshekhonov, V., Pisarev, I., Podkladkin, S., Pose, R., Pukhov, O., Romanov, V., Rumyantsev, V., Rusakovich, N., Ryabchenko, K., Salihagic, D., Samoilov, V., Savin, I., Shchelchkov, A., Yu. Sedykh, Semenov, A., Senchishin, V., Shabalin, D., Shalyugin, A., Shigaev, V., Shilov, Y., Sisakian, A., Snyatkov, V., Yu. Sorokina, Tkachev, L., Tokmenin, V., Topilin, N., Tskhadadze, E., Yu. Usov, Vertogradov, L., Vinogradov, V., Vorozhtsov, S., Yamburenko, V., Yarygin, G., Yu. Yatsunenko, Zhuravlev, V., Ban, J., Bruncko, D., Chochula, P., Dubnickova, A. Z., Ferencei, J., Jusko, A., Kladiva, E., Kubinec, P., Kurca, T., Masarik, J., Povinec, P., Rosinsky, P., Stanicek, J., Stavina, P., Strizenec, P., Sykora, I., Tokar, S., Vanko, J., Cindro, V., Filipcic, A., Kramberger, G., Mikuz, M., Tadel, M., Zontar, D., Blanchot, G., Bosman, M., Bravo, S., Cavalli-Sforza, M., Chmeissani, M., Crespo, J. M., Delfino, M., Fernandez, E., Grauges, E., Yu. Ivanyushenkov, Juste, A., Martinez, M., Miralles, L., Pacheco, A., Park, I. C., Perlas, J. A., Ruiz, H., Vichou, I., Barreiro, F., Del Peso, J., Hervas, L., Labarga, L., Albiol, F., Ballester, F., Benlloch, J. M., Bernabeu, J., Cases, R., Castillo, M. V., Ferrer, A., Fuster, J., Garcia, C., Gonzalez, V., Gil, I., Lopez, J. M., Romance, J. B., Salt, J., Sanchez, J., Sanchis, E., Sanchis, M. A., Sebastia, A., Zuniga, J., Almehed, S., Carling, H., Danielsson, H., Egede, U., Hedberg, V., Jarlskog, G., Lorstad, B., Lundberg, B., Mjornmark, U., Soderberg, M., Carlson, P., Clement, C., Lund-Jensen, B., Pearce, M., Soderqvist, J., Vanyashin, A., Agnvall, S., Berglund, S., Bohm, C., Engstrom, M., Fristedt, A., Hellman, S., Holmgren, S. O., Johansson, E., Jon-And, K., Sellden, B., Silverstein, S., Tardell, S., Yamdagni, N., Zhao, X., Bingefors, N., Botner, O., Brenner, R., Bystrom, O., Ekelof, T., Gustafsson, L., Hallgren, A., Kullander, S., Staaf, P., Beringer, J., Borer, K., Hess, M., Lehmann, G., Mommsen, R., Pal, T., Pretzl, K., Bonino, R., Clark, A. G., Couyoumtzelis, C., Demierre, P., Kambara, H., Kowalewski, R., La Marra, D., Leger, A., Perrin, E., Vuaridel, B., Wu, X., Arik, E., Birol, I., Cicek, Z., Cuhadar, T., Gun, S., Hacinliyan, A., Mailov, A., Nurdan, K., Perdahci, Z., Turk, I., Unel, G., Charlton, D. G., Dowell, J. D., Garvey, J., Hillier, S. J., Homer, R. J., Jovanovic, P., Kenyon, I. R., Mcmahon, T. J., Neale, S. W. O., Rees, D. L., Staley, R. J., Watkins, P. M., Watson, A. T., Watson, N. K., Wilson, J. A., Batley, J. R., Carter, J. R., Drage, L., Goodrick, M. J., Hill, J. C., Munday, D. J., Parker, M. A., Robinson, D., Wyllie, K. H., Boyle, O., Candlin, D. J., Candlin, E. R. S., Knowles, I. G., Playfer, S. M., Doyle, A. T., Flavell, A. J., Lynch, J. G., Martin, D. J., Shea, V. O., Raine, C., Saxon, D. H., Skillicorn, I. O., Smith, K. M., Brodbeck, T. J., Henderson, R. C. W., Hughes, G. H., Komorowski, T., Ratoff, P. N., Sloan, T., Allport, P. P., Booth, P. S. L., Carroll, L. J., Cooke, P. A., Greenall, A., Houlden, M. A., Jackson, J. N., Jones, T. J., King, B. T., Moreton, A., Richardson, J. D., Smith, N. A., Sutcliffe, P., Turner, P. R., Beck, G. A., Carter, A. A., Eisenhandler, E. F., Kyberd, P., Landon, M., Lloyd, S. L., Martin, A. J., Pentney, J. M., Pritchard, T. W., Graham. Thompson, Blair, G. A., George, S., Green, B. J., Medcalf, T., Strong, J. A., Bignall, P., Clarke, P., Cranfield, R., Crone, G., Esten, M., Jones, T., Lane, J., Sherwood, P., Duerdoth, I. P., Dunne, P. W., Finnegan, P. F., Foster, J. M., Freestone, J., Gilbert, S. D., Hughes-Jones, R. E., Ibbotson, M., Kolya, S. D., Loebinger, F. K., Marshall, R., Mercer, D., Snow, S., Thompson, R. J., Bibby, J. H., Buira-Clark, D., Fox-Murphy, A., Grewal, A., Harris, F. J., Hawes, B. M., Hill, J., Holmes, A., Howell, D., Hunt, S. J., Kundu, N., Lloyd, J., Loken, J. G., Nickerson, R. B., Reichold, A., Renton, P. B., Segar, A. M., Wastie, R. L., Weidberg, A. R., Apsimon, R. J., Baines, J. T., Baynham, D. E., Botterill, D. R., Campbell, D. A., Clifft, R. W., Edwards, J. P., Edwards, M., English, R. L., Fisher, S. M., Gee, C. N. P., Gibson, M. D., Gillman, A. R., Hart, J. C., Hatley, R. W., Haywood, S. J., Hill, D. L., Madani, S., Mccubbin, N. A., Mcphail, D. J., Middleton, R. P., Morrissey, M. C., Murray, W. J., Nichols, A., Norton, P. R., Payne, B. T., Perera, V. J. O., Phillips, P. W., Pilling, A., Quinton, S. P. H., Saunders, B. J., Seller, P., Shah, T. P., Tappern, G. J., Tyndel, M., White, D. J., Wickens, F. J., Booth, C. N., Buttar, C. M., Cartwright, S. L., Combley, F. H., Lehto, M. H., Sellin, P. J., Spooner, N. J. C., Thompson, L. F., Alam, M. S., Athar, S. B., Mahmood, A., Ovunc, S., Severini, H., Timm, S., Wappler, F., Zhichao, L., Berger, E. L., Blair, R., Dawson, J., Guarino, V., Hill, N., May, E. N., Nodulman, L. J., Price, L. E., Proudfoot, J., Schlereth, J. L., Stanek, R., Wagner, R. G., Wicklund, A. B., Cheu, E., Johns, K., Loch, P., Rutherfoord, J., Savin, A., Shaver, L., Shupe, M., Steinberg, J., Tompkins, D., K. De, Gallas, E., Li, J., Sawyer, L., Stephens, R., White, A., Barnett, M., Bintinger, D., Ciocio, A., Dahl, O., Einsweiler, K., Ely, R., Gilchriese, M., Haber, C., Hinchliffe, I., Holland, S., Joshi, A., Kipnis, I., Kleinfelder, S., Milgrome, O., Nygren, D., Palaio, N., Pengg, F., Shapiro, M., Siegrist, J., Spieler, H., Trilling, G., Hazen, E., Shank, J., Simmons, E., Whitaker, J. S., Zhou, B., Behrends, S., Bensinger, J. R., Blocker, C., Cunningham, J., Kirsch, L. E., Lamoureux, J., Wellenstein, H., Citterio, M., Cullen, J., Gibbard, B., Gordeev, A., Gordon, H., Graf, N., Grachev, V., Kandasamy, A., Kotcher, J., Lissauer, D., Ma, H., Makowiecki, D., Murtagh, M. J., Connor, P. O., Paige, F., Polychronakos, V., Protopopescu, S., Radeka, V., Rahm, D. C., Rajagopalan, S., Rescia, S., Smith, G., Sondericker, J., Stephani, D., Stumer, I., Takai, H., Chernyatin, V., Yu, B., Anderson, K., Blucher, E., Evans, H., Glenzinski, D., Merritt, F., Oreglia, M., Pilcher, J., Pod, E., Sanders, H., Shochet, M., Turcot, A., Cartiglia, N., Cunitz, H., Dodd, J., Gara, A., Leltchouk, M., Parsons, J., Seman, M., Shaevitz, M., Sippach, W., Willis, W., Fortney, L. R., Goshaw, A. T., Lee, A. M., Oh, S. H., Robertson, R. J., Wang, C. H., Wesson, D., Baker, K., Feldman, G. J., Franklin, M. E. B., Huth, J., Oliver, J., Hanson, G., Zhenyu Li, Luehring, F., Ogren, H., Rust, D. R., Lankford, A. J., Hackett, C., Pier, S., Schernau, M., Stoker, D., Haridas, P., Osborne, L. S., Paradiso, J. A., Pless, I. A., Taylor, F. E., Wadsworth, B. F., Abolins, M., Brock, R., Bromberg, C., Edmunds, D., Yu. Ermolin, Gross, S., Huston, J., Laurens, P., Linnemann, J., Miller, R., Owen, D., Pope, B. G., Richards, R., Weerts, H., Gold, M., Gorfine, G., Matthews, J., Seidel, S., Khandaker, M., Mcfarlane, K., Punjabi, V., Salgado, C. W., Fortner, M., Sirotenko, V. I., Gutierrez, P., Mcmahon, T., Nemati, B., Skubic, P., Snow, J., Strauss, M., Dressnandt, N., Keener, P., Newcomer, F. M., Berg, R., Williams, H. H., Cleland, W. E., Clemen, M., Bazizi, K., England, D., Ferbel, T., Ginther, G., Glebov, V., Haelen, T., Lobkowicz, F., Slattery, P., Zielinski, M., Dorfan, D., Dubbs, T., Grillo, A., Heusch, C., Kashigin, S., Litke, A., Popelvine, P., Sadrozinski, H. F. W., Seiden, A., Spencer, E., Coan, T. E., Skwarnicki, T., Stroynowski, R., Teplitz, V., Mann, A., Milburn, R., Napier, A., Katrina Sliwa, Downing, R. W., Errede, D., Errede, S., Haney, M. J., Simaitis, V. J., Thaler, J., Burnett, T. H., Chaloupka, V., Cook, V., Daly, C., Davisson, R., Forbush, D., Guldenmann, H., Lubatti, H. J., Mockett, P. M., Reinhall, P., Rothberg, J., Wasserbaech, S., Zhao, T., Fasching, D., Gonzalez, S., Jared, R. C., Pan, Y. B., Scott, I. J., Walsh, J., Wu, S. L., Yamartino, J. M., Zobernig, G., Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Corpusculaire - Clermont-Ferrand (LPC), Université Blaise Pascal - Clermont-Ferrand 2 (UBP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), ATLAS, and Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)
Subjects: [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
Published: 1996

38. Light-particle correlations in heavy-ion reactions at ganil

Author: Erazmus, B., Lebrun, C., Lednicky, R., Ghisalberti, C., Lilian Martin, Nouais, D., Pluta, J., Ardouin, D., Jean-Pierre Cussonneau, Eudes, P., Guilbault, F., Pascal Lautridou, Rahmani, A., Reposeur, T., Daniel Roy, Sezac, L., Carjan, N., Quebert, J., Siemssen, R., Lewitowicz, M., Mittig, W., Roussel-Chomaz, P., Abdelouahad Chbihi, Galin, J., Guerreau, D., Morjean, M., Peghaire, A., Aguer, P., Burzynski, W., Peryt, W., Dabrowski, H., Stefanski, P., Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Grand Accélérateur National d'Ions Lourds (GANIL), Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse (CSNSM), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Lorgeril, Jocelyne, Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Subjects: [PHYS.NEXP] Physics [physics]/Nuclear Experiment [nucl-ex], [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], Nuclear Physics
Published: 1994

39. Neutrinos et rayons cosmiques chargés

Author: Coyle, P., Richard Dallier, Derome, L., Ghia, P., Kouchner, A., Rosier-Lees, S., antoine letessier selvon, Lilian Martin, Parizot, E., Schüssler, F., Stolarczyk, T., Suomijarvi, T., Corentin Vallée, Montanet, F., Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), and Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)
Subjects: [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
Abstract: Groupe de Travail G5 : Univers haute énergie, ondes gravitationnelles, tests de la gravitation

40. ATLAS: technical proposal for a general-purpose p p experiment at the large hadron collider at CERN

Author: Armstrong, W. W., Burris, W., Gingrich, D. M., Green, P., Greeniaus, L. G., Hewlett, J. C., Holm, L., Mcdonald, J. W., Mullin, S., Olsen, W. C., Pinfold, J. L., Rodning, N., Schaapman, J., Soukup, J., Boos, E., Pokrovsky, N., Zhautykov, B., Bakker, E., Bobbink, G. J., Bos, K., Boterenbrood, H., Dankers, R. J., Daum, C., Waard, A., Groenstege, H., Hartjes, F., Heubers, W., Kieft, G. N. M., Kluit, R., Linde, F., Massaro, G. G. G., Metselaar, J., Rewiersma, P. A. M., Schuijlenburg, H., Tolsma, H., Udo, F., Den Berg, F. D., Graaf, H., Eijk, B., Vermeulen, J. C., Werneke, P., Wilhelm, R., Aubert, B., Bazan, A., Beaugiraud, B., Boniface, J., Colas, J., Christian Girard, Jezequel, S., Lecoq, J., Le Flour, T., Linossier, O., Moynot, M., Nicoleau, S., Riccadonna, X., Sauvage, G., Thion, J., Wingerter-Seez, I., Zitoun, R., Zolnierowski, Y., Berger, E. L., Blair, R., Dawson, J., Fuess, T. A., Guarino, V., Hill, N., Magill, S. R., May, E. N., Nodulman, L. J., Price, L. E., Proudfoot, J., Stanek, R., Underwood, D. G., Wagner, R. G., Wicklund, A. B., Forden, G. E., Johns, K., Loch, P., Rutherfoord, J., Savin, A., Shaver, L., Shupe, M., Steinberg, J., K. De, Gallas, E., Li, J., Sawyer, L., Stephens, R., White, A., Dris, M., Filippas, A., Fokitis, E., Gazis, E., Katsoufis, E., Maltezos, S., Papadopoulou, T., Tzanakos, G. S., Abdinov, O. B., Aliev, F. M., Aliev, R. M., Khalilzade, F. T., Mekhdiev, R. R., Rzaev, H. J., Usubov, Z. U., Blanchot, G., Bosman, M., Cavalli-Sforza, M., Chmeissani, M., Crespo, J. M., Delfino, M., Efthymiopoulos, I., Fernandez, E., Garrido, L., Yu. Ivanyushenkov, Juste, A., Martinez, M., Miralles, L., Orteu, S., Padilla, C., Perlas, J. A., Pacheco, A., Riu, I., Ronceux, B., Sanchez, F., Teubert, F., Bintinger, D., Ciocio, A., Collins, T., Dahl, O., Einsweiler, K., Gilchriese, M., Haber, C., Holland, S., Kipnis, I., Lee, R., Milgrome, O., Millaud, J., Nygren, D., Shapiro, M., Siegrist, J., Spieler, H., Trilling, G., Wright, M., Beringer, J., Borer, K., Hess, M., Pal, T., Pretzl, K., Carney, R. E., Charlton, D. G., Dowell, J. D., Garvey, J., Homer, R. J., Jovanovic, P., Kenyon, I. R., Mcmahon, T. J., Neale, S. W. O., Rees, D. L., Staley, R. J., Watkins, P. M., Watson, A. T., Wilson, J. A., Fischer, P., Geich-Gimbel, C., Hilger, E., Stahl, A., Wermes, N., Hazen, E., Marin, A., Rohlf, J., Shank, J., Simmons, E., Varner, G., Whitaker, J. S., Worstell, W., Zhou, B., Behrends, S., Bensinger, J. R., Blocker, C., Cunningham, J., Kirsch, L. E., Lamoureux, J., Wellenstein, H., Chochula, P., Hlinka, V., Janik, R., Kubinec, P., Lichard, P., Luchan, L., Masarik, J., Pikna, M., Povinec, P., Sitar, B., Strmen, P., Szarka, J., Tokar, S., Gibbard, B., Gordeev, A., Gordon, H., Graf, N., Grachev, V., Kandasamy, A., Kotcher, J., Lissauer, D., Ma, H., Makowiecki, D., Mccorkle, S., Murtagh, M. J., Connor, P. O., Paige, F., Polychronakos, V., Protopopescu, S., Radeka, V., Rahm, D. C., Rescia, S., Smith, G., Sondericker, J., Stephani, D., Stumer, I., Takai, H., Chernyatin, V., Yu, B., Arsenescu, R., Blaj, C., Boldea, V., Caprini, I., Caprini, M., Constantin, F., Constantinescu, S., Corcotoi, I., Dita, S., Dita, P., Legrand, I. C., Micu, L., Batley, J. R., Carter, J. R., Goodrick, M. J., Hill, J. C., Munday, D. J., Parker, M. A., Robinson, D., Wyllie, K. H., Armitage, J., Dixit, M., Dubeau, J., Estabrooks, P., Losty, M., Neuheimer, E., Oakham, G., Neill, M. O., Anghinolfi, F., Bee, C., Bergsma, F., Blum, W., Bock, R., Burckhart, H. J., Campbell, M., Chevalley, J. L., Dauvergne, J. P., Acqua, A., Drakoulakos, D., Dufey, J. P., Eerola, P., Ellis, N., Fabjan, C. W., Farthouat, P., Flegel, W., Franz, A., Froidevaux, D., Fuchs, W., Funk, W., Gerwig, H., Gianotti, F., Gildemeister, O., Goret, B., Hatch, M., Haug, F., Hauviller, C., Heijne, E., Henriques, A., Hoffmann, H. F., Jarron, P., Jenni, P., Jones, R., Kantardjian, G., Klempt, W., Knobloch, J., Krischer, W., Langhans, W., Lasseur, C., Lehraus, I., Lofstedt, B., Mapelli, L., Marchioro, A., Mclaren, R. A., Mornacchi, G., Nessi, M., Onions, C., Poggioli, L., Poppleton, A., Poulard, G., Price, M., Richter-Was, E., Roe, S., Rohrbach, F., Rosso, E., Schmid, P., Schuh, S., Snoeys, W., Ben Taylor, Trischuk, E., Tsesmelis, E., Vasey, F., Viehhauser, G., Voss, R., Vuillemin, V., Weilhammer, P., Wendler, H., Witzeling, W., Wotschack, J., Anderson, K., Armstrong, R., Blucher, E., Evans, H., Merritt, F., Pilcher, J., Sanders, H., Turcot, A., Wagner, D., Ziad Ajaltouni, Badaud, F., Bouhemaid, N., Brette, P., Brossard, M., Chadelas, R., Chevaleyre, J. C., Crouau, M., Daudon, F., Dugne, J. J., Michel, B., Gerard Montarou, S Muanza, G., Pallin, D., Plothow-Besch, H., Poirot, S., Reinmuth, G., Says, L. P., Vazeille, F., Cartiglia, N., Cunitz, H., Dodd, J., Gara, A., Leltchouk, M., Parsons, J., Seman, M., Shaevitz, M., Sippach, W., Willis, W., Damgaard, G., Hansen, J. B., Hansen, J. D., Hansen, J. R., Hansen, P., Kjaer, N. J., Moller, R., Nielsen, B. S., Arneodo, M., La Rotonda, L., Liguori, D., Schioppa, M., Susinno, G., Valdata-Nappi, M., Blocki, J., Czermak, A., Gadomski, S., Godlewski, J., Hajduk, Z., Iwanski, W., Kaplon, J., Korcyl, K., Malecki, P., Olszowska, J., Sobala, A., Dabrowski, W., Grybos, P., Idzik, M., Jagielski, S., Jelen, K., Kisielewska, D., Kowalski, T., Rulikowska-Zarebska, E., Andrle, J., Fuss, J., Gossling, C., Lisowski, B., Rolf, A., Spiwoks, R., Stavropoulos, G., Wunstorf, R., Aleksandrov, I., Alekseev, G., Anosov, V., Astvatsaturov, A., Azhgirei, L., Bannikov, A., Baranov, S. A., Borisov, O., Boyko, I., Yu. Budagov, Bychkov, V., Chelkov, G., Cheplakov, A., Chirikov-Zorin, I., Chlachidze, G., Dodonov, V., Feshchenko, A., Flyagin, V., Glagolev, V., Yu. Gornushkin, Ignatenko, M., Kazarinov, M., Kekelidze, V., Khovansky, N., Kodes, P., Kotov, V., Kovtun, V., Krivokhizhin, V., Krumshtein, Z., Kukhtin, V., Yu. Kulchitsky, Ladygin, E., Lebedev, A., Liba, I., Yu. Lomakin, Malyshev, V. L., Malyukov, S., Minashvili, I., Nikolenko, M., Nozdrin, A., Obudovsky, V., Olshevsky, A., Pantea, D., Peshekhonov, V., Pose, R., Pukhov, O., Romanov, V., Rumyantsev, V., Rusakovich, N., Salihagic, D., Savin, I., Yu. Sedykh, Senchishin, V., Semenov, A., Sisakian, A., Shchelchkov, A., Snyatkov, V., Tkachev, L., Topilin, N., Tokmenin, V., Vertogradov, L., Vorozhtsov, S., Yarygin, G., Fortney, L. R., Goshaw, A. T., Lee, A. M., Oh, S. H., Robertson, R. J., Wang, C. H., Wesson, D., Candlin, D. J., Peach, K. J., Capannesi, G., Colocci, M., Giorgetti, E., Nuti, M., Palchetti, L., Pelfer, P. G., Rosada, A., Sedda, A. F., Sottini, S., Trigari, S., Ventura, G., Vinattieri, A., Bilokon, H., Chiarella, V., Curatolo, M., Esposito, B., Maccarrone, G., Pepe-Altarelli, M., Jie Chen, Ebling, D. G., Geppert, R., Goppert, R., Herten, G., Irsigler, R., Kolpin, R., Landgraf, U., Lauxtermann, S., Ludwig, J., Mohr, W., Runge, K., Schafer, F., Scherberger, G., Schmid, T., Webel, M., Weber, C., Kawaguti, M., Tanaka, S., Bonino, R., Clark, A. G., Couyoumtzelis, C., Kambara, H., La Marra, D., Leger, A., Perrin, E., Richeux, J. P., Wu, X., Barberis, D., Bozzo, M., Caso, C., Dameri, M., Darbo, G., Gemme, C., Morettini, P., Musico, P., Osculati, B., Parodi, F., Ridolfi, G., Rossi, L., Sette, G., Auria, S. D., Doyle, A. T., Flavell, A. J., Lynch, J. G., Martin, D. J., Shea, V. O., Raine, C., Saxon, D. H., Skillicorn, I. O., Smith, K. M., Stavrianakou, M., Collot, J., Christophorou, G., Saintignon, P., Daniel Dzahini, Hostachy, J. Y., Laborie, G., Martin, P., Rey-Campagnolle, M., Rossetto, O., Dado, S., Goldberg, J., Lupu, N., Feick, H., Fretwurst, E., Lindstrom, G., Schulz, T., Feldman, G. J., Franklin, M. E. B., Huth, J., Oliver, J., Kenney, C. J., Parker, S. I., Geweniger, C., Hanke, P., Kluge, E. E., Putzer, A., Rensch, B., Tittel, K., Wunsch, M., Jalas, P., Schulman, T., Asai, M., Iwata, Y., Ohsugi, T., Hanson, G., Zhenyu Li, Luehring, F., Ogren, H., Rust, D. R., Girtler, P., Hortnagl, C., Kneringer, E., Kuhn, D., Rudolph, G., Lankford, A. J., Pier, S., Schmid, B., Stoker, D., Arik, E., Birol, I., Cicek, Z., Cuhadar, T., Mailov, A., Nurdan, K., Ziya Nazım Perdahçı, Unel, G., Doersing, V., Erhard, W., Kammel, P., Reinsch, A., Amako, K., Arai, Y., Fujii, H., Ikeno, M., Iwasaki, H., Kanzaki, J., Kohriki, T., Kondo, T., Manabe, A., Morita, Y., Nomachi, M., Ohska, T. K., Sasaki, O., Terada, S., Unno, Y., Watase, Y., Yamamoto, A., Yasu, Y., Kawagoe, K., Nozaki, M., Takeda, H., Ban, J., Bruncko, D., Ferencei, J., Jusko, A., Kladiva, E., Kurca, T., Strizenec, P., Takashima, R., Brodbeck, T. J., Hughes, G. H., Komorowski, T., Henderson, R. C. W., Ratoff, P. N., Sloan, T., Cesaroni, F., Creti, P., Gorini, E., Grancagnolo, F., Palamara, O., Panareo, M., Petrera, S., Primavera, M., Amorim, A., Barreira, G., Carvalho, J., David, M., Gomes, A., Gomes, J., Gomes, P., Mota, M., Maio, A., Maneira, M., Onofre, A., Pinhao, J., Wolters, H., Allport, P. P., Biagi, S. F., Booth, P. S. L., Bowcock, T. J. V., Carroll, L. J., Cooke, P. A., Houlden, M. A., Forbes, K., Greenall, A., Jackson, J. N., Jones, T. J., King, B. T., Mcmahon, S. J., Moreton, A., Richardson, J. D., Smith, N. A., Sutcliffe, P., Turner, P. R., Tzamarias, S. E., Wormald, M., Beck, G. A., Carter, A. A., Eisenhandler, E. F., Kyberd, P., Landon, M., Lloyd, S. L., Martin, A. J., Pentney, J. M., Pritchard, T. W., Graham. Thompson, Blair, G. A., Green, B. J., Medcalf, T., Mir, L. M., Strong, J. A., Bignall, P., Clarke, P., Cranfield, R., Crone, G., Esten, M., Jones, T., Lane, J., Sherwood, P., Akesson, T., Almehed, S., Carling, H., Danielsson, H., Egede, U., Hedberg, V., Ivarsson, J., Jarlskog, G., Lorstad, B., Lundberg, B., Mjornmark, U., Thulesius, M., Barreiro, F., Hervas, L., Labarga, L., Del Peso, J., Buchholz, P., Kopke, L., Kleinknecht, K., Merle, K., Renk, B., Duerdoth, I. P., Dunne, P. W., Finnegan, P. F., Foster, J. M., Freestone, J., Gilbert, S. D., Hughes-Jones, R. E., Ibbotson, M., Kolya, S. D., Loebinger, F. K., Lumb, N., Marshall, R., Snow, S., Mercer, D., Thompson, R. J., Kugel, A., Ludvig, J., Manner, R., Noffz, K. H., Zoz, R., Basa, S., Blanquart, L., Bonzom, V., Calzas, A., Chekhtman, A., Clemens, J. C., Cohen-Solal, M., Cousinou, M. C., Dargent, P., Delpierre, P., Dinkespiler, B., Duval, P. Y., Etienne, F., Fallou, A., Fassnacht, P., Ferrato, D., Fouchez, D., Gally, Y., Grigorev, E., Habrard, M. C., Hallewell, G., Le Suu, A., Lilian Martin, Mekkaoui, A., Monnier, E., Mouthuy, T., Nacasch, R., Nagy, E., Olivetto, C., Pouit, L., Qian, Z., Raymond, M., Rondot, C., Rozanov, A., Sauvage, D., Tisserant, S., Touchard, F., Vacavant, L., Haridas, P., Osborne, L. S., Paradiso, J. A., Pless, I. A., Taylor, F. E., Wadsworth, B. F., Fares, F., Gorfine, G., Moorhead, G. F., Sevior, M. E., Taylor, G. N., Tovey, S. N., Abolins, M., Brock, R., Bromberg, C., Edmunds, D., Gross, S., Huston, J., Linnemann, J., Miller, R., Owen, D., Pope, B. G., Richards, R., Weerts, H., Battistoni, G., Bellini, G., Camin, D., Cavalli, D., Costa, G., Cozzi, L., Di Corato, M., Avella, A. D., Fedyakin, N. N., Anthony Ferrari, Inzani, P., Mandelli, L., Mazzanti, M., Menasce, D., Moroni, L., Pedrini, D., Perasso, L., Perini, L., Ragusa, F., Sala, P., Sala, S., Tartarelli, F., Bogush, A. A., Dazhneko, A. V., Satsunkevich, I. S., Sergeenko, M. N., Zyazyulya, F. E., Azuelos, G., Beaudoin, G., Castillo, A., Cote, J. C., Depommier, P., Florian, E. L., Leroy, C., Lorazo, B., P Martin, J., Pascal Roy, Savard, P., Tafirout, R., Trigger, I., Zacek, V., Artamonov, A., Epstein, V., Gorbunov, P., Gurin, R., Zhemanov, V., Khovansky, V., Kruchinin, S., Kuchenkov, A., Maslennikov, A., Ryabinin, M., Shatalov, P., Tsukerman, I., Zaitsev, V., Zeldovich, S., Baranov, S. P., Belov, M., Gavrilenko, I., Komar, A., Konovalov, S., Kopytin, M., Muravev, S., Popov, L., Shmeleva, A., Shikanian, A., Snesarev, A., Sulin, V., Tikhomirov, V., Vasileva, L., Yakimenko, M., Bondarenko, V., Dolgoshein, B., Grigorev, V., Kondratev, O., Konstantinov, A., Nevsky, P., Pavlenko, S., Romanyuk, A., Semenov, S., Smirnov, S., Sosnovtsev, V., Bashindzhagian, G. L., Basiladze, S. G., Chudakov, E. A., Karmanov, D. E., Kuleshov, A. V., Kramarenko, V. A., Larichev, A. N., Melikhov, D. I., Merkin, M. M., Rizatdinova, F. K., Selikov, A. V., Yu Sivoklokov, S., Smirnova, L. N., Yu Zhukov, V., Zverev, E. G., Deile, M., Faessler, M. A., Hessey, N. P., Staude, A., Aderholz, M., Brettel, H., Breuker, H., Cesura, G., Dietl, H., Dulny, B., Dydak, F., Fent, J., Gruhn, C., Hauff, D., Jakobs, K., Kiesling, C., Kroha, H., Lutz, G., Manz, A., Moser, H. G., Oberlack, H., Ostapchuk, A., Richter, R. H., Richter, R., Schacht, P., Schael, S., Schmucker, H., Tribanek, W., Aloisio, A., Alviggi, M. G., Cevenini, F., Chiefari, G., Asmundis, R., Drago, E., Merola, L., Napolitano, M., Patricelli, S., Yoshida, H., Bergman, R., Brouwer, C., Crijns, F. J. G. H., Dijkema, J. A., Kittel, W., Klok, P. F., Konig, A. C., Metzger, W. J., Pols, C. L. A., Schotanus, D. J., Visser, E. J., Wijnen, T. A. M., Sirotenko, V. I., Batrakov, A., Chilingarov, A., Fedotov, M., Gaponenko, I., Klimenko, S., Kollegov, M., Kozlov, V., Kuper, E., Malyshev, V. M., Yu. Merzlyakov, Panin, V., Shamov, A., Telnov, V., Yu. Tikhonov, Yu. Velikzhanin, Ardelean, J., Arnault, C., Auge, E., Barrand, G., Bouchel, M., Breton, D., Chase, R. L., Chollet, C., Coulon, J. P., La Taille, C., Delebecque, P., Ducorps, A., Fayard, L., Fournier, D., Grivaz, J. F., Hrisoho, A., Iconomidou-Fayard, L., Jean, P., Lavigne, B., Martin, G., Merkel, B., Noppe, J. M., Parrour, G., Petroff, P., Richer, J. P., Schaffer, A. C., Seguin-Moreau, N., Serin, L., Tisserand, V., Unal, G., Veillet, J. J., Vernay, E., Vichou, I., Bugge, L., Buran, T., Kristiansen, H., Nygard, E., Stapnes, S., Bibby, J. H., Brooks, C. B., Harris, F. J., Howell, D., Fox-Murphy, A., Grewal, A., Hawes, B. M., Hawkings, R. J., Holmes, A., Hunt, S. J., Kundu, N., Loken, J. G., Nickerson, R. B., Reichold, A., Renton, P. B., Segar, A. M., Wastie, R. L., Alexanian, H., Baubillier, M., Bezamat, J., Billoir, P., Blouzon, F., Canton, B., David, J., Genat, J. F., Imbault, D., Le Dortz, O., Nayman, P., Rossel, F., Savoy-Navarro, A., Schwemling, P., Ambrosini, G., Cambiaghi, M., Cattaneo, P., Conta, C., Ferrari, R., Fraternali, M., Fumagalli, G., Introzzi, G. L., Lanza, A., Livan, M., Orestano, D., Pastore, F., Pennacchio, E., Polesello, G., Rimoldi, A., Vercesi, V., Dressnandt, N., Keener, P., Newcomer, F. M., Berg, R., Williams, H. H., Angelini, C., Autiero, D., Bellettini, G., Bosi, F., Cavasinni, V., Cobal, M., Santo, A., Pretet. Del, Di Girolamo, B., Flaminio, V., Lami, S., Lazzeroni, C., Raffaelli, M., Renzoni, G., Cleland, W. E., Clemen, M., Bohm, J., Gabor, P., Hrivnac, J., Lednicky, R., Lokajicek, M., Nemecek, S., Sicho, P., Simak, V., Smizanska, M., Stastny, J., Stedron, M., Vanickova, M., Vrba, V., Davidek, T., Dolejsi, J., Dolezal, Z., Kucera, M., Leitner, R., Suk, M., Tas, P., Trka, Z., Valkar, S., Wilhelm, I., Jakubek, J., Kubasta, J., Macha, I., Ota, J., Pospisil, S., Sopko, B., Amelin, D. V., Ammosov, V. V., Yu Bogolyubsky, M., Borisov, A. A., Bozhko, N. I., Bryzgalov, V. V., Chekulaev, S. V., Chernichenko, S. K., Chuntonov, A., Chmil, V., Denisov, S. P., Yu Dushkin, A., Gapienko, V. A., Gilitsky, Yu V., Goryachev, V., Karyukhin, A. N., Khmelnikov, V. A., Khokhlov, Yu A., Kirsanov, M. M., Kiryunin, A. A., Klyukhin, V., Kopikov, S. V., Kostrikov, M. E., Kononov, A. I., Korotkov, V. A., Kozhin, A. S., Kravtsov, V. I., Kurchaninov, L. L., Lapin, V. V., Levitsky, M. L., Mikhailin, V. N., Moiseev, A. M., Minaenko, A. A., Myagkov, A. G., Onuchin, V. A., Pleskach, A. V., Popov, A. I., Protopopov, Yu M., Ryabchikov, D. I., Salomatin, Yu I., Semenov, P. A., Shein, I., Soldatov, A. P., Solodkov, A. A., Solovyanov, O. V., Smol, A., Starchenko, E. A., Surkov, A. N., Sytnik, V. V., Tikhonov, V. V., Yu. Tsyupa, Vorobev, A. P., Vovenko, A. S., Zaets, V. G., Zaitsev, A. M., Zmushko, V., Caloba, L. P., Maidantchik, C. L., Marroquin, F., Mesquita, A., Seixas, J. M., Thome, Z. D., Broer, W., Ferbel, T., Ginther, G., Glebov, V., Haelen, T., Lobkowicz, F., Mansour, J., Slattery, P., Zielinski, M., Cox, P. T., Giokaris, N., Khazins, D., Alfino, M., Bagnaia, P., Camarri, P., Ciapetti, G., Falciano, S., Gentile, S., Lacava, F., Nisati, A., Petrolo, E., Pontecorvo, L., Veneziano, S., Verzocchi, M., Zanello, L., Cardarelli, R., Di Ciaccio, A., Santonico, R., Bacci, C., Ceradini, F., Apsey, R. Q., Apsimon, R. J., Baines, J. T., Baynham, D. E., Botterill, D. R., Carr, F. S., Clifft, R. W., Coombs, R. C., Cragg, D. A., Cunliffe, N. H., Dowdell, J. G., Edgecock, T. R., Edwards, J. P., Edwards, M., English, R. L., Evans, E., Fisher, S. M., Gee, C. N. P., Gibson, M. D., Gillman, A. R., Gorbold, J. R., Greenhalgh, R. J. S., Hart, J. C., Hatley, R. W., Haywood, S. J., Hiddleston, J., Hill, D. L., Holtom, E., Jones, L. L., Leake, J. L., Mccubbin, N. A., Mcphail, D. J., Middleton, R. P., Morrissey, M. C., Murray, P., Murray, W. J., Nichols, A., Norton, P. R., Payne, B. T., Perera, V. J. O., Phillips, P. W., Saunders, B. J., Seller, P., Shah, T. P., Shankar, K., Tappern, G. J., Tyndel, M., Walters, C. R., White, D. J., Wickens, F. J., Baze, J. M., Bernard, R., Bourdinaud, M., Brisson, J. C., Bystricky, J., Calvet, D., Chevalier, L., Cloue, O., Convert, P., Cure, C., Dael, A., Delagnes, E., Desportes, H., Djidi, K., Duthil, R., Trogoff, J., Ernwein, J., Fourches, N., Gachelin, O., Giovannoni, P., Gosset, L., Guyot, C., Hansl-Kozanecka, T., Heitzmann, J., Hubbard, J. R., Huet, M., Joudon, A., Kozanecki, W., Lamare, P., Laporte, J. F., Lavocat, P., Lesmond, C., Lottin, J. P., Le Du, P., Mandzhavidze, I., Mansoulie, B., Meyer, J. P., Mur, M., Pabot, Y., Pascual, J., Patoux, A., Renardy, J. F., Schuller, J. P., Schune, P., Schwindling, J., Taguet, J. P., Teiger, J., Thooris, B., Vedrine, P., Veyssiere, C., Virchaux, M., Walter, C., Dewitt, J., Dorfan, D., Grillo, A., Litke, A., Sadrozinski, H., Seiden, A., Spencer, E., Booth, C. N., Buttar, C. M., Cartwright, S. L., Combley, F. H., Lehto, M. H., Sellin, P. J., Spooner, N. J. C., Thompson, L. F., Takeshita, T., Gillessen, G., Holder, M., Kreutz, A., Coan, T. E., Skwarnicki, T., Stroynowski, R., Teplitz, V., Agnvall, S., Berglund, S., Bohm, C., Engstrom, M., Hellman, S., Holmgren, S. O., Johansson, E., Jon-And, K., Sellden, B., Tardell, S., Yamdagni, N., Zhao, X., Agehed, K., Carlson, P., Eek, L. O., Eide, A., Hultberg, S., Lindblad, T., Lindsey, C., Lund-Jensen, B., Minerskjold, M., Soderqvist, J., Vanyashin, A., Sukhorukov, A. V., Konyakhin, I. A., Fedin, O., Ivochkin, V., Nadtochy, A., Yu. Ryabov, Shchegelsky, V., Smirnov, A. I., Spiridenkov, E., Alexiev, D., Donnelly, I. J., Varvell, K. E., Williams, M. L., Chikovani, L., Gabuniya, L., Gogiberidze, G., Gogoladze, G., Grigalashvili, T., Khorguashvili, Z., Kipiani, K., Koshtoev, V., Sopromadze, D., Topchishvili, L., Tskhadadze, E., Tvalashvili, O., Chiladze, B., Khelashvili, A., Zh. Khubua, Liparteliani, A., Salukvadze, R., Abramowicz, H., Alexander, G., Bella, G., Benary, O., Dagan, S., Levy, A., Oren, Y., Chouridou, S., Eleftheriadis, C., Liolios, A., Petridou, C., Sampsonidis, D., Nakagawa, Y., Yamagata, T., Imori, M., Kawamoto, T., Kobayashi, T., Mashimo, T., Fukunaga, C., Hamatsu, R., Emura, T., Bhadra, S., Martin, J. F., Mayer, J. K., Orr, R. S., Sinervo, P. K., Stairs, G. G., Astbury, A., Birney, P., Hodges, T., Langstaff, R., Oram, C., Roberts, B., Mann, A., Milburn, R., Napier, A., Katrina Sliwa, Arvidson, A., Bingefors, N., Brenner, R., Botner, O., Bystrom, O., Ekelof, T., Gustafsson, L., Hallgren, A., Kullander, S., Downing, R. W., Errede, D., Errede, S., Haney, M. J., Simaitis, V. J., Thaler, J., Albiol, F., Benlloch, J. M., Cases, R., Ferrer, A., Fuster, J., Garcia, C., Honore, P. F., Salt, J., Sanchis, E., Sanchis, M. A., Sebastia, A., Valls, J. A., Velasco, J., Axen, D., Howard, R., Beer, G., Fincke-Keeler, M., Keeler, R., Lefebvre, M., Poffenberger, P., Robertson, L., Robertson, S., Sobie, R., White, J., Burnett, T. H., Chaloupka, V., Cook, V., Daly, C., Davisson, R., Dennis, B., Forbush, D., Feng, Z. Y., Franklin, J., Lubatti, H. J., Mockett, P. M., Reinhall, P., Rothberg, J., Toevs, F., Wasserbaech, S., Zhao, T., Barberio, E., Breskin, A., Chechik, R., Duchovni, E., Eisenberg, Y., Gross, E., Hass, M., Karshon, U., Lellouch, D., Levinson, L., Mikenberg, G., Revel, D., Gonzalez, S., Jared, R. C., Pan, Y. B., Saadi, Y., Schmitt, M., Scott, I. J., Wu, S. L., Yamartino, J. M., Zobernig, G., Becks, K. H., Drees, J., Garg, M., Glitza, K. W., Hamacher, K., Kersten, S., Lenzen, G., Middelkamp, P., Uberschar, S., Wahlen, H., Hakopian, H., Grabsky, V., Vartapetian, A., Mnatsakanian, E., Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Corpusculaire - Clermont-Ferrand (LPC), Université Blaise Pascal - Clermont-Ferrand 2 (UBP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), ATLAS, and Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)
Subjects: [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]

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