Calibration and Performance of the Surface Scintillator Detector of the Pierre Auger Observatory

The Pierre Auger Observatory has led to significant advances in our understanding of ultra- high-energy cosmic rays. These new insights have driven a major upgrade of the Observatory, known as AugerPrime, through which the experiment has entered its Phase II, a new period of data collection. A key part of the upgrade is adding surface scintillator detectors (SSD) on top of the existing water-Cherenkov detectors (WCD). The main goal is to leverage their different responses to the electromagnetic and muonic shower components, enhancing the reconstruction of the primary cosmic-ray mass. In this contribution, we present the methods that involve analyzing peak and charge distributions of atmospheric muons for accurate calibration during extensive air-shower event reconstruction, along with the development of a rate-based algorithm for independent calibration. We also show the performance of the SSDs with Phase-II data, including PMT reliability and stability of key parameters, such as gain and signal-to-noise ratio.

Authors

Publication Details

Published
2025-09-23
DOI
https://doi.org/10.22323/1.501.0227
Primary Topic
Radiation Detection and Scintillator Technologies
Type
article
Field-Weighted Citation Impact
0.00

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Calibration and Performance of the Surface Scintillator Detector of the Pierre Auger Observatory

Belén Andrada, Zbigniew Szadkowski, Bruno L. Lago, Carla Taricco et al.
Radiation Detection and Scintillator Technologies
article

Calibration and Performance of the Surface Scintillator Detector of the Pierre Auger Observatory

Belén Andrada, Zbigniew Szadkowski, Bruno L. Lago, Carla Taricco, Giovanni Consolati, Juan Manuel Gonzalez, S. Petrera, T. Pierog, G. Sigl, Mateo Fernandez, T. Huege, Nicolas Leal, Carmina Pérez Bertolli, Carlo Salvattore Cruz Sanchez, Frank Schröder, Gustavo Medina‐Tanco, A. C. Fauth, Enrico Arnone, Enrique Varela, O. Schölten, Olena Tkachenko, Lorenzo Cazon, Pierpaolo Savina, Lukáš Vaclavek, B. R. Dawson, Laura Valore, A. Haungs, Dalibor Nosek, G. Parente, Paula Gina Isar, Janning Meinert, Emanuele De Vito, Dušan Mandát, Adila Abdul Halim, Gonzalo Rodriguez Fernandez, Jiří Blažek, Therese Paulsen, Adriel Bartz Mocellin, Berenika Čermáková, S. J. de Jong, V. Rizi, Armando di Matteo, Alexey Yushkov, K. Daumiller, A. Insolia, Lorenzo Caccianiga, Darko Veberič, María Isabel Micheletti, A. Segreto, L. Nellen, Felicia Barbato, Jan Pękala, Thomas Fitoussi, Khoa D. Nguyen, Katarína Simkova, R. Caruso, I. Allekotte, F. Sarazin, Luis A. Núñez, Chaitanya Priyadarshi, M. Cristinziani, E. Zas, Clara Keiko Oliveira Watanabe, Roberta Colalillo, L. Miramonti, F. Simon, F. Salamida, P. Trávnı́ček, Benjamin Flaggs, P. Hamal, G.P. Guedes, A. D. Supanitsky, Pedro J. Costa, Maximilian Straub, R. Mussa, Camilla Petrucci, Steffen Hahn, Federico Maria Mariani, Fiona H. Ellwanger, J. Vícha, Jaime Álvarez-Muñiz, C. Hojvat, Denise Boncioli, L. Chytka, Martin Vacula, Miguel A. Martins, F. Guarino, Glennys R. Farrar, M. Erdmann, Jarosław Stasielak, Shima Ujjani Shivashankara, C. E. Covault, Tobias Schulz, M. Palatka, I. De Mitri, Antoine Letessier-Selvon, K. S. Caballero‐Mora, Antonio Franco, Bjarni Pont, Simone Rossoni, S. Buitink, Petr Tobiška, Juan Ammerman Yebra, Violet M. Harvey, Achille Nucita, Hermann-Josef Mathes, P. Mantsch, Lawrence Wiencke, Rukije Uzeiroska, Nicolás Martín González, Silvia Mollerach, Toshihiro Fujii, Nicolas San Martin, Zuzana Svozilikova, M. Pech, Maximilian Stadelmaier, P. Assis, F. Montanet, Mohit Saharan, T. Hebbeker, M. Mallamaci, Alena Bakalová, Peter L. Biermann, Jan Ebr, Anthony Bwembya, J. A. Chinellato, S. Andringa, Jorge Caraça-Valente, Krzysztof Pytel, R. Conceição, C. Bonifazi, Shefali Negi, Jon Paul Lundquist, Edyvânia Emily Pereira Martins, Fridtjof Feldbusch, Josina Schulte, S. Vorobiov, Ezequiel Rodriguez, Alexander Novikov, Varada Varma Kizakke Covilakam, Emanuele Avocone, J. Biteau, H.O. Klages, H. Wilczyński, Antonio Ambrosone, Pranav Sampathkumar, M. Aglietta, Patricia María Hansen, A. Gorgi, F. de Palma, V. de Souza, Esteban Roulet, S. Dasso, Leo Östman, Fabio Convenga, B. Tomé, J. Matthews, Fernando Catalani, Adrian Sedoski, Radomir Šmída, Eva Santos, Joaquín de Jesús, Milton Freitas, M. Pimenta, Carmelo Evoli, Jose A. Bellido, Kathrin Bismark, Adrián Rovero, D. Góra, J. Řídký, B. Keilhauer, Stef Verpoest, Antonino Del Popolo, Katharine Mulrey, Diego Correia dos Santos, Mario Buscemi, Wilson M. Namasaka, Vincent Pelgrims, Chloé Gaudu, Yago Lema-Capeans, Carmen Merx, Mohsen Pourmohammad Shahvar, Lukas Gülzow, Nikolas Denner, Simon Strähnz, Sergio Cabana-Freire, Alessandro Cermenati, Beatriz de Errico, João Vítor Reginatto Akim, Fedor Tairli, Alex Reuzki, Tim Fehler, Eric William Mayotte, M. Unger, J. Chudoba, Andreas Weindl, Markus Roth, A. De Roeck, Brian Wundheiler, Gioacchino Alex Anastasi, Indira D. Vergara Quispe, José Ochoa, Teresa Bister, Tiina Suomijärvi, Marko Zavrtanik, Alan Watson, K.‐H. Kampert, Jose Sanabria Gomez, B. Garćıa, Marcus Niechciol, Leonel Morejón, J. Brack, Igor Vaiman, Ralph Engel, Juan Carlos D'Olivo, Juan Pallotta, Alejandro Almela, Andrej Filipčič, Humberto Ibarguen Salazar, Rita Cassia dos Anjos, Analisa Mariazzi, Norbert Kunka, Luca Deval, Peter Mazur, Marvin Gottowik, Stanislav Michal, Johannes Blümer, Jelena Köhler, Danilo Zavrtanik, Fernando Gollan, Luis Miguel Domingues Mendes, Edivaldo Moura Santos, Isabelle Lhenry-Yvon, Federico Andrés Sánchez, Qader Dorosti, Italo Epicoco, Alberto Etchegoyen, Charles Timmermans, Paul Filip, Antonio Bueno, Carlos J. Todero Peixoto, Luan Bonneau Arbeletche, Michael Prouza, Harm Schoorlemmer, Mariano Gómez Berisso, Roger W Clay, Felix Riehn, Margita Kubátová, Melanie Weitz, Primo F. Gómez Vitale, Rogerio M. de Almeida, Corinne Berat, Martina Boháčová, David Schmidt, Niklas Langner, R. Sarmento, Pavel Horváth, G. Marsella, Nataliia Borodai, Cristina Galea, Kévin Almeida Cheminant, Martin Schimassek, Jose F. Valdés Galicia, H. Schieler, Sergio J Sciutto, Jorge Rubén Rodriguez Rojo, Markus Risse, Daniele Martello, Adriana Vásquez-Ramírez, Florian Lukas Briechle, Samo Stanič, Marcelo Augusto Leigui de Oliveira, Ioana Codrina Maris, Giorgio Matthiae, Marcos Cerda, Valerio Verzi, Piera Luisa Ghia, P. Gabriel Brichetto Orchera, Gaetano Salina, Ruben Squartini, Gabriela Nicora, Agustín Cobos Cerutti, Manuel Platino, Michael Schimp, Antonella Castellina, Brian Fick, Dave Nitz, Alan Fuster, Vladimír Novotný, Lorenzo Perrone, Petr Janeček, Virginia Binet, Diego Ravignani, Rodrigo Pelayo, Marina Scornavacche, Alexander Menshikov, C. Dobrigkeit, P. Abreu, Jörg Hörandel, Juan Carlos Arteaga Velázquez, Ricardo Sato, Cainã Oliveira, Max Büsken, Luis A. Anchordoqui, Gualberto Avila, Marta Bianciotto, A. Săftoiu, L. Lopes, Patrick Stassi, Abha Khakurdikar, Sonja Mayotte, Fabian Gobbi, Baobiao Yue, Paolo Privitera, Lorenzo Apollonio, Carla Aramo, Srijan Sehgal, Miroslav Hrabovský, Joao dos Anjos, Roberto Aloisio, Mario E. Bertaina, Diego Melo, Shayoni Panja, Vlastimil Jílek, Matías Rolf Hampel, Veronika Vašíčková, Alexandra Fernandes, Ugo GIACCARI, J. Rautenberg, Viviana Scherini, Luiz Augusto Pereira, Sara Martinelli, Heino Falcke, Geraldina Golup, Matteo Conte, Jaime de Oliveira, Petr Schovanek, Libor Nožka, Jannis Pawlowsky, Olivier Deligny, Danelise de Oliveira Franco, Juan Manuel Figueira, Federico Campuzano, Frederik Krieger, Sven Querchfeld, Jacco Vink, Matthias Kleifges, Alex Tapia, Luciana Andrade Dourado, Tomáš Fodran, Matias Jorge Tueros, G. Cataldi, Megha Mogarkar, Jhansi Bhavani Vuta, Eric-Teunis de Boone, Mohamed Ismaiel, Karolina Syrokvas, Matteo Tambone, Pim van Dillen
article en

Abstract

The Pierre Auger Observatory has led to significant advances in our understanding of ultra- high-energy cosmic rays. These new insights have driven a major upgrade of the Observatory, known as AugerPrime, through which the experiment has entered its Phase II, a new period of data collection. A key part of the upgrade is adding surface scintillator detectors (SSD) on top of the existing water-Cherenkov detectors (WCD). The main goal is to leverage their different responses to the electromagnetic and muonic shower components, enhancing the reconstruction of the primary cosmic-ray mass. In this contribution, we present the methods that involve analyzing peak and charge distributions of atmospheric muons for accurate calibration during extensive air-shower event reconstruction, along with the development of a rate-based algorithm for independent calibration. We also show the performance of the SSDs with Phase-II data, including PMT reliability and stability of key parameters, such as gain and signal-to-noise ratio.

Strong, European Commission, Deutsche Forschungsgemeinschaft, Agence Nationale de la Recherche, Fundação de Amparo à Pesquisa do Estado de São Paulo, Ministerstvo Školství, Mládeže a Tělovýchovy, Grantová Agentura České Republiky, Bundesministerium für Bildung und Forschung, Fonds De La Recherche Scientifique - FNRS, Consejo Nacional de Investigaciones Científicas y Técnicas, Fonds Wetenschappelijk Onderzoek, Conselho Nacional de Desenvolvimento Científico e Tecnológico, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Centre National de la Recherche Scientifique, Financiadora de Estudos e Projetos, Ministério da Ciência, Tecnologia, Inovações e Comunicações, Vlaamse regering, Helmholtz Alliance for Astroparticle Physics, Agencia Nacional de Promoción Científica y Tecnológica, Institut National de Physique Nucléaire et de Physique des Particules
Openalex Percentile: Top 67%
Radiation Detection and Scintillator Technologies
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.