Deep-learning based reconstruction of the shower maximum 𝑿max using the water-Cherenkov detectors of the Pierre Auger Observatory (2021)
- Authors:
- USP affiliated authors: CATALANI, FERNANDO - EEL ; SOUZA FILHO, LUIZ VITOR DE - IFSC ; SANTOS, EDIVALDO MOURA - IF ; PEIXOTO, CARLOS JOSÉ TODERO - EEL ; ARBELETCHE, LUAN BONNEAU - IFSC ; HUERTA, HUMBERTO MARTINEZ - IFSC ; LANG, RODRIGO GUEDES - IFSC ; ARMAND, JOHNNIER PÉREZ - IF ; CARVALHO JUNIOR, WASHINGTON RODRIGUES DE - IF
- Unidades: EEL; IFSC; IF
- DOI: 10.1088/1748-0221/16/07/P07019
- Subjects: FÍSICA DE ALTA ENERGIA; RAIOS CÓSMICOS
- Keywords: Data analysis; Pattern recognition; Cluster finding; Calibration and fitting methods; Large detector systems for particle and astroparticle physics; Particle identification methods
- Agências de fomento:
- Financiado pela Agencia Nacional de Promoción Científica y Tecnológica
- Financiado pelo Conicet, Argentina
- Financiado pelo CNPq
- Financiado pela FINEP
- Financiado pela FAPERJ
- Financiado pela FAPESP
- Financiado pelo MCTI
- Financiado pelo BMBF
- Financiado pela DFG
- Financiado pelo INAF
- Financiado pelo Conacyt, México
- Financiado pelo FEDER
- Language: Inglês
- Imprenta:
- Source:
- Título: Journal of Instrumentation
- ISSN: 1748-0221
- Volume/Número/Paginação/Ano: v. 16, n. 7, p. P07019-1-P07019-27, July 2021
- Status:
- Artigo aberto em periódico híbrido (Hybrid Open Access)
- Versão do Documento:
- Versão publicada (Published version)
- Acessar versão aberta:
-
ABNT
AAB, A. et al. Deep-learning based reconstruction of the shower maximum 𝑿max using the water-Cherenkov detectors of the Pierre Auger Observatory. Journal of Instrumentation, v. 16, n. 7, p. P07019-1-P07019-27, 2021Tradução . . Disponível em: https://doi.org/10.1088/1748-0221/16/07/P07019. Acesso em: 10 maio 2026. -
APA
Aab, A., Arbeletche, L. B., Catalani, F., Souza, V. de, Lang, R. G., Martínez-Huerta, H., et al. (2021). Deep-learning based reconstruction of the shower maximum 𝑿max using the water-Cherenkov detectors of the Pierre Auger Observatory. Journal of Instrumentation, 16( 7), P07019-1-P07019-27. doi:10.1088/1748-0221/16/07/P07019 -
NLM
Aab A, Arbeletche LB, Catalani F, Souza V de, Lang RG, Martínez-Huerta H, Armand JP, Carvalho Junior WR de, Santos EM, Peixoto CJT. Deep-learning based reconstruction of the shower maximum 𝑿max using the water-Cherenkov detectors of the Pierre Auger Observatory [Internet]. Journal of Instrumentation. 2021 ; 16( 7): P07019-1-P07019-27.[citado 2026 maio 10 ] Available from: https://doi.org/10.1088/1748-0221/16/07/P07019 -
Vancouver
Aab A, Arbeletche LB, Catalani F, Souza V de, Lang RG, Martínez-Huerta H, Armand JP, Carvalho Junior WR de, Santos EM, Peixoto CJT. Deep-learning based reconstruction of the shower maximum 𝑿max using the water-Cherenkov detectors of the Pierre Auger Observatory [Internet]. Journal of Instrumentation. 2021 ; 16( 7): P07019-1-P07019-27.[citado 2026 maio 10 ] Available from: https://doi.org/10.1088/1748-0221/16/07/P07019 - The energy spectrum of cosmic rays beyond the turn-down around 10' POT. 17' eV as measured with the surface detector of the Pierre Auger Observatory
- Search for magnetically-induced signatures in the arrival directions of ultra-high-energy cosmic rays measured at the Pierre Auger Observatory
- Studies on the response of a water-Cherenkov detector of the Pierre Auger Observatory to atmospheric muons using an RPC hodoscope
- Direct measurement of the muonic content of extensive air showers between 2 × 10^17 and 2 × 10^18 eV at the Pierre Auger Observatory
- Features of the energy spectrum of cosmic rays above 2.5 × 10^18 eV using the Pierre Auger Observatory
- A Search for ultra-high-energy neutrinos from TXS 0506+056 using the Pierre Auger Observatory
- Reconstruction of events recorded with the surface detector of the Pierre Auger Observatory
- Measurement of the cosmic-ray energy spectrum above 2.5 × 10 18 eV using the Pierre Auger Observatory
- The Pierre Auger Observatory and its upgrade
- Design, upgrade and characterization of the silicon photomultiplier front-end for the AMIGA detector at the Pierre Auger Observatory
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