AugerPrime surface detector electronics

The Pierre Auger Collaboration, Adila Abdul Halim,Pedro Abreu, M. Aglietta, I. Allekotte,Kévin Almeida Cheminant, A. Almela,Roberto Aloisio, J. Álvarez-Muñiz,J. Ammerman Yebra,Gioacchino Alex Anastasi,Luis A. Anchordoqui, Belén Andrada, S. Andringa, Anukriti, C. Aramo, Paulo Ricardo Araújo Ferreira,Enrico Arnone, Juan Carlos Arteaga Velázquez, P. Assis, G. Ávila, E. Avocone,Alina Mihaela Badescu, A. Bakalova,Felicia Barbato, Adriel Bartz Mocellin, J. A. Bellido, C. Bérat, M. Bertaina,Gopal Bhatta,Marta Bianciotto,Peter L. Biermann, Virginia Binet, Kathrin Bismark,Teresa Bister, J. Biteau,Jiří Blažek, C. Bleve, J. Blümer,M. Bohã̌cov́a, D. Boncioli,C. Bonifazi,Luan Bonneau Arbeletche, N. Borodai, Jeffrey Brack, P. Gabriel Brichetto Orchera,Florian Lukas Briechle, A. Bueno, S. Buitink,Mario Buscemi, A. Bwembya,Max Büsken, K. S. Caballero-Mora, S. Cabana-Freire, L. Caccianiga, R. Caruso,A. Castellina, F. Catalani,G. Cataldi, L. Cazón,Marcos Cerda, A. Cermenati, J. Chinellato, J. Chudoba, L. Chytka, R. W. Clay,A. C. Cobos Cerutti, R. Colalillo,Alan Coleman, M. R. Coluccia, R. Conceição,Antonio Condorelli, G. Consolati, M. Conte, F. Convenga, Diego Correia dos Santos, P. J. Costa, C. E. Covault, M. Cristinziani, Carlo Salvattore Cruz Sanchez, S. Dasso, K. Daumiller, B. R. Dawson, R. M. de Almeida,Joaquín de Jesús,Sijbrand J. de Jong, J. R. T. de Mello Neto,I. De Mitri,Jaime de Oliveira, D. Franco,F. de Palma,Vítor de Souza, B. P. de Souza de Errico,Emanuele De Vito,A. Del Popolo,O. Deligny, N. Denner, Luca Deval,Armando di Matteo, M. Dobre, C. Dobrigkeit,Juan Carlos D’Olivo, Luis Miguel Domingues Mendes, J. C. dos Anjos,Rita Cassia dos Anjos, Jan Ebr, Fiona H. Ellwanger, Mohamed Emam, R. Engel,Italo Epicoco, M. Erdmann, A. Etchegoyen, Carmelo Evoli,H. Falcke,John Farmer, Glennys R. Farrar, A. C. Fauth, N. Fazzini,Fridtjof Feldbusch,Francesco Fenu, Alexandra Fernandes, B. Fick, J. M. Figueira, A. Filip̧cǐc, T. Fitoussi, Benjamin Flaggs, Tomáš Fodran, Toshihiro Fujii,Alan Fuster, C. Galea, Claudio Galelli,Beatriz García, Chloé Gaudu, H. Gemmeke, F. Gesualdi, A. Gherghel-Lascu, P. L. Ghia, U. Giaccari,Jonas Glombitza,Fabian Gobbi, Fernando Gollan, G. Golup,Juan Pablo Gongora, Juan Manuel González, N. González, Isabel Goos, A. Gorgi, M. Gottowik, T. D. Grubb, F. Guarino, G. P. Guedes,Eleonora Guido, M. Gómez Berisso, Primo F. Gómez Vitale,Dariusz Góra,Steffen Hahn, P. Hamal,Matías Rolf Hampel, Patricia María Hansen, D. Harari, Violet M. Harvey, A. Haungs, T. Hebbeker, C. Hojvat, P. Horváth, M. Hrabovský, T. Huege, J. R. Hörandel, A. Insolia, P. G. Isar,Petr Janeček, Jeffrey A. Johnsen,Jakub Jurýšek,Karl-Heinz Kampert, B. Keilhauer, Abha Khakurdikar, Varada Varma Kizakke Covilakam, H. O. Klages, M. Kleifges, Felix Knapp, Norbert Kunka,Bruno L. Lago, Niklas Langner,M. A. Leigui de Oliveira, Yago Lema-Capeans, A. Letessier‐Selvon, I. Lhenry-Yvon, L. Lopes,Lu Lu, Quentin Luce,Jon Paul Lundquist, Allan Machado Payeras, M. Majercakova,Dušan Mandát,Bradley C. Manning, P. Mantsch, S. Marafico, F. M. Mariani, A. G. Mariazzi, I. C. Mariş, G. Marsella, D. Martello, Sara Martinelli, M. A. Martins, O. Martínez Bravo, H. J. Mathes, J. Matthews, G. Matthiae, E. Mayotte, Sonja Mayotte, P. O. Mazur, G. Medina‐Tanco, J. Meinert, D. Melo,Alexander Menshikov, Carmen Merx,Stanislav Michal, M. I. Micheletti, L. Miramonti,Silvia Mollerach, F. Montanet, Leonel Morejón, C. Morello, Katharine Mulrey, R. Mussa,Wilson M. Namasaka, Shubham Negi,Lukas Nellen, Khoa Dang Nguyen, Gabriela Nicora,Marcus Niechciol, D. Nitz, D. Nosek,Vladimír Novotný, L. Nožka, A. A. Nucita, L. A. Núñez, C. Oliveira, M. Palatka, J. Pallotta,Subhasis Panja, G. Parente, T. Paulsen, J. Pawlowsky, M. Pech, R. Pelayo, L. A. S. Pereira, Edyvânia Emily Pereira Martins, Johnnier Perez Armand, L. Perrone, S. Petrera, C. Petrucci, T. Pierog, M. Pimenta, M. Platino,Bjarni Pont, Mart Pothast, Mohsen Pourmohammad Shahvar, P. Privitera, M. Prouza, A. Puyleart, Carmina Pérez Bertolli, Jan Pękala, S. Querchfeld, J. Rautenberg, D. Ravignani, J. V. Reginatto Akim,Maximilian Reininghaus, J. R̆ídký,Felix Riehn, M. Risse,Vincenzo Rizi, W. Rodrigues de Carvalho, Ezequiel Rodríguez, Juan Rojo,Matías J. Roncoroni, Simone Rossoni,Markus Roth, Esteban Roulet, A. C. Rovero, Philip Ruehl, A. Sǎftoiu, M. Saharan, F. Salamida, H. Salazar, G. Salina,J. D. Sanabria Gómez, Eva Santos, Edivaldo Moura Santos, F. Sarazin, R. Sarmento, R. Sato,Pierpaolo Savina, V. Scherini, H. Schieler, Martin Schimassek, Michael Schimp, D. Schmidt,Olaf Scholten, H. Schoorlemmer, Petr Schovánek,Frank G. Schröder,Josina Schulte, Tobias Schulz, C. Schäfer, S. J. Sciutto, Marina Scornavacche, A. Segreto, S. Sehgal, S. U. Shivashankara,Guenter Sigl, Gaia Silli, O. Sima, F. Simon, R. Smau, P. Sommers, Jorge F. Soriano, R. Squartini, Maximilian Stadelmaier, S. Stanič, J. Stasielak, P. Stassi, M. Straub, S. Strähnz, T. Suomijärvi, A. D. Supanitsky, Zuzana Svozilikova, Z. Szadkowski, F. Sánchez, F. Tairli, A. Tapia,Carla Taricco, C. Timmermans, Olena Tkachenko, Petr Tobiška, C. J. Todero Peixoto, B. Tomé,Zoé Torrès, A. Travaini, P. Trávničék, Caterina Trimarelli, M. Tueros, M. Unger, L. Vaclavek,Martin Vacula,J. F. Valdés Galicia, L. Valore, E. Varela, D. Veberič,Cynthia Ventura,Indira D. Vergara Quispe, V. Verzi, J. Vícha,Jacco Vink, Jilek Vlastimil, S. Vorobiov, Adriana Vásquez-Ramírez, C. Watanabe, Alan Watson, A. Weindl, L. Wiencke, H. Wilczyński, David Wittkowski, B. Wundheiler, Bin Yue, A. Yushkov, Orazio Zapparrata, E. Zas,D. Zavrtanik, M. Zavrtanik, R. Šmída

Journal of Instrumentation(2023)

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摘要
Operating since 2004, the Pierre Auger Observatory has led to major advances in our understanding of the ultra-high-energy cosmic rays. The latest findings have revealed new insights that led to the upgrade of the Observatory, with the primary goal of obtaining information on the primary mass of the most energetic cosmic rays on a shower-by-shower basis. In the framework of the upgrade, called AugerPrime, the 1660 water-Cherenkov detectors of the surface array are equipped with plastic scintillators and radio antennas, allowing us to enhance the composition sensitivity. To accommodate new detectors and to increase experimental capabilities, the electronics is also upgraded. This includes better timing with up-to-date GPS receivers, higher sampling frequency, increased dynamic range, and more powerful local processing of the data. In this paper, the design characteristics of the new electronics and the enhanced dynamic range will be described. The manufacturing and test processes will be outlined and the test results will be discussed. The calibration of the SD detector and various performance parameters obtained from the analysis of the first commissioning data will also be presented.
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augerprime surface detector electronics
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