Inference of the Mass Composition of Cosmic Rays with Energies from 10^{18.5} to 10^{20} eV Using the Pierre Auger Observatory and Deep Learning.
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- 10.1103/physrevlett.134.021001
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- 2025 Jan 17
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@article{allodium:10.1103/physrevlett.134.021001,
title = {Inference of the Mass Composition of Cosmic Rays with Energies from 10\textasciicircum{}\{18.5\} to 10\textasciicircum{}\{20\} eV Using the Pierre Auger Observatory and Deep Learning.},
author = {Abdul Halim A and Abreu P and Aglietta M and Allekotte I and Almeida Cheminant K and Almela A and Aloisio R and Alvarez-Muñiz J and Ammerman Yebra J and Anastasi GA and Anchordoqui L and Andrada B and Andrade Dourado L and Andringa S and Apollonio L and Aramo C and Araújo Ferreira PR and Arnone E and Arteaga Velázquez JC and Assis P and Avila G and Avocone E and Bakalova A and Barbato F and Bartz Mocellin A and Berat C and Bertaina ME and Bhatta G and Bianciotto M and Biermann PL and Binet V and Bismark K and Bister T and Biteau J and Blazek J and Bleve C and Blümer J and Boháčová M and Boncioli D and Bonifazi C and Bonneau Arbeletche L and Borodai N and Brack J and Brichetto Orchera PG and Briechle FL and Bueno A and Buitink S and Buscemi M and Büsken M and Bwembya A and Caballero-Mora KS and Cabana-Freire S and Caccianiga L and Campuzano F and Caruso R and Castellina A and Catalani F and Cataldi G and Cazon L and Cerda M and Čermáková B and Cermenati A and Chinellato JA and Chudoba J and Chytka L and Clay RW and Cobos Cerutti AC and Colalillo R and Coluccia MR and Conceição R and Condorelli A and Consolati G and Conte M and Convenga F and Correia Dos Santos D and Costa PJ and Covault CE and Cristinziani M and Cruz Sanchez CS and Dasso S and Daumiller K and Dawson BR and de Almeida RM and de Errico B and de Jesús J and de Jong SJ and de Mello Neto JRT and De Mitri I and de Oliveira J and de Oliveira Franco D and de Palma F and de Souza V and De Vito E and Del Popolo A and Deligny O and Denner N and Deval L and di Matteo A and do JA and Dobre M and Dobrigkeit C and D'Olivo JC and Domingues Mendes LM and Dorosti Q and Dos Anjos JC and Dos Anjos RC and Ebr J and Ellwanger F and Emam M and Engel R and Epicoco I and Erdmann M and Etchegoyen A and Evoli C and Falcke H and Farrar G and Fauth AC and Fehler T and Feldbusch F and Fenu F and Fernandes A and Fick B and Figueira JM and Filip P and Filipčič A and Fitoussi T and Flaggs B and Fodran T and Fujii T and Fuster A and Galea C and García B and Gaudu C and Gherghel-Lascu A and Ghia PL and Giaccari U and Glombitza J and Gobbi F and Gollan F and Golup G and Gómez Berisso M and Gómez Vitale PF and Gongora JP and González JM and González N and Góra D and Gorgi A and Gottowik M and Guarino F and Guedes GP and Guido E and Gülzow L and Hahn S and Hamal P and Hampel MR and Hansen P and Harari D and Harvey VM and Haungs A and Hebbeker T and Hojvat C and Hörandel JR and Horvath P and Hrabovský M and Huege T and Insolia A and Isar PG and Janecek P and Jilek V and Johnsen JA and Jurysek J and Kampert KH and Keilhauer B and Khakurdikar A and Kizakke Covilakam VV and Klages HO and Kleifges M and Knapp F and Köhler J and Krieger F and Kunka N and Lago BL and Langner N and Leigui de Oliveira MA and Lema-Capeans Y and Letessier-Selvon A and Lhenry-Yvon I and Lopes L and Lu L and Luce Q and Lundquist JP and Machado Payeras A and Majercakova M and Mandat D and Manning BC and Mantsch P and Mariani FM and Mariazzi AG and Mariş IC and Marsella G and Martello D and Martinelli S and Martínez Bravo O and Martins MA and Mathes HJ and Matthews J and Matthiae G and Mayotte E and Mayotte S and Mazur PO and Medina-Tanco G and Meinert J and Melo D and Menshikov A and Merx C and Michal S and Micheletti MI and Miramonti L and Mollerach S and Montanet F and Morejon L and Mulrey K and Mussa R and Namasaka WM and Negi S and Nellen L and Nguyen K and Nicora G and Niechciol M and Nitz D and Nosek D and Novotny V and Nožka L and Nucita A and Núñez LA and Oliveira C and Palatka M and Pallotta J and Panja S and Parente G and Paulsen T and Pawlowsky J and Pech M and Pȩkala J and Pelayo R and Pelgrims V and Pereira LAS and Pereira Martins EE and Pérez Bertolli C and Perrone L and Petrera S and Petrucci C and Pierog T and Pimenta M and Platino M and Pont B and Pothast M and Pourmohammad Shahvar M and Privitera P and Prouza M and Querchfeld S and Rautenberg J and Ravignani D and Reginatto Akim JV and Reininghaus M and Reuzki A and Ridky J and Riehn F and Risse M and Rizi V and Rodrigues de Carvalho W and Rodriguez E and Rodriguez Rojo J and Roncoroni MJ and Rossoni S and Roth M and Roulet E and Rovero AC and Saftoiu A and Saharan M and Salamida F and Salazar H and Salina G and Sanabria Gomez JD and Sánchez F and Santos EM and Santos E and Sarazin F and Sarmento R and Sato R and Savina P and Schäfer CM and Scherini V and Schieler H and Schimassek M and Schimp M and Schmidt D and Scholten O and Schoorlemmer H and Schovánek P and Schröder FG and Schulte J and Schulz T and Sciutto SJ and Scornavacche M and Sedoski A and Segreto A and Sehgal S and Shivashankara SU and Sigl G and Simkova K and Simon F and Smau R and Šmída R and Sommers P and Squartini R and Stadelmaier M and Stanič S and Stasielak J and Stassi P and Strähnz S and Straub M and Suomijärvi T and Supanitsky AD and Svozilikova Z and Szadkowski Z and Tairli F and Tapia A and Taricco C and Timmermans C and Tkachenko O and Tobiska P and Todero Peixoto CJ and Tomé B and Torrès Z and Travaini A and Travnicek P and Tueros M and Unger M and Uzeiroska R and Vaclavek L and Vacula M and Valdés Galicia JF and Valore L and Varela E and Vašíčková V and Vásquez-Ramírez A and Veberič D and Vergara Quispe ID and Verzi V and Vicha J and Vink J and Vorobiov S and Watanabe C and Watson AA and Weindl A and Wiencke L and Wilczyński H and Wittkowski D and Wundheiler B and Yue B and Yushkov A and Zapparrata O and Zas E and Zavrtanik D and Zavrtanik M and Pierre Auger Collaboration},
year = {2025},
journal = {Physical review letters},
doi = {10.1103/physrevlett.134.021001},
url = {https://doi.org/10.1103/physrevlett.134.021001}
}RIS
TY - JOUR
TI - Inference of the Mass Composition of Cosmic Rays with Energies from 10^{18.5} to 10^{20} eV Using the Pierre Auger Observatory and Deep Learning.
AU - Abdul Halim A
AU - Abreu P
AU - Aglietta M
AU - Allekotte I
AU - Almeida Cheminant K
AU - Almela A
AU - Aloisio R
AU - Alvarez-Muñiz J
AU - Ammerman Yebra J
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AU - Mollerach S
AU - Montanet F
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AU - Palatka M
AU - Pallotta J
AU - Panja S
AU - Parente G
AU - Paulsen T
AU - Pawlowsky J
AU - Pech M
AU - Pȩkala J
AU - Pelayo R
AU - Pelgrims V
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AU - Pérez Bertolli C
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AU - Petrera S
AU - Petrucci C
AU - Pierog T
AU - Pimenta M
AU - Platino M
AU - Pont B
AU - Pothast M
AU - Pourmohammad Shahvar M
AU - Privitera P
AU - Prouza M
AU - Querchfeld S
AU - Rautenberg J
AU - Ravignani D
AU - Reginatto Akim JV
AU - Reininghaus M
AU - Reuzki A
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AU - Riehn F
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AU - Scherini V
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AU - Sedoski A
AU - Segreto A
AU - Sehgal S
AU - Shivashankara SU
AU - Sigl G
AU - Simkova K
AU - Simon F
AU - Smau R
AU - Šmída R
AU - Sommers P
AU - Squartini R
AU - Stadelmaier M
AU - Stanič S
AU - Stasielak J
AU - Stassi P
AU - Strähnz S
AU - Straub M
AU - Suomijärvi T
AU - Supanitsky AD
AU - Svozilikova Z
AU - Szadkowski Z
AU - Tairli F
AU - Tapia A
AU - Taricco C
AU - Timmermans C
AU - Tkachenko O
AU - Tobiska P
AU - Todero Peixoto CJ
AU - Tomé B
AU - Torrès Z
AU - Travaini A
AU - Travnicek P
AU - Tueros M
AU - Unger M
AU - Uzeiroska R
AU - Vaclavek L
AU - Vacula M
AU - Valdés Galicia JF
AU - Valore L
AU - Varela E
AU - Vašíčková V
AU - Vásquez-Ramírez A
AU - Veberič D
AU - Vergara Quispe ID
AU - Verzi V
AU - Vicha J
AU - Vink J
AU - Vorobiov S
AU - Watanabe C
AU - Watson AA
AU - Weindl A
AU - Wiencke L
AU - Wilczyński H
AU - Wittkowski D
AU - Wundheiler B
AU - Yue B
AU - Yushkov A
AU - Zapparrata O
AU - Zas E
AU - Zavrtanik D
AU - Zavrtanik M
AU - Pierre Auger Collaboration
PY - 2025
JO - Physical review letters
DO - 10.1103/physrevlett.134.021001
UR - https://doi.org/10.1103/physrevlett.134.021001
ER - APA
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- pubmed · retrieved 2026-09-25T19:00:34.982Z