Features of the energy spectrum of cosmic rays above 2.5 × 10^18 eV using the Pierre Auger Observatory (2020)
- 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: 10.1103/PhysRevLett.125.121106
- Subjects: RAIOS CÓSMICOS; FÍSICA DE ALTA ENERGIA; ASTROFÍSICA
- 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:
- Publisher place: College Park
- Date published: 2020
- Source:
- Título: Physical Review Letters
- ISSN: 0031-9007
- Volume/Número/Paginação/Ano: v. 125, n. 12, p. 121106-1-121106-10, Sept. 2020
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: hybrid
- Licença: cc-by
-
ABNT
AAB, A. et al. Features of the energy spectrum of cosmic rays above 2.5 × 10^18 eV using the Pierre Auger Observatory. Physical Review Letters, v. 125, n. 12, p. 121106-1-121106-10, 2020Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.125.121106. Acesso em: 04 ago. 2025. -
APA
Aab, A., Arbeletche, L. B., Catalani, F., Souza, V. de, Lang, R. G., Martínez-Huerta, H., et al. (2020). Features of the energy spectrum of cosmic rays above 2.5 × 10^18 eV using the Pierre Auger Observatory. Physical Review Letters, 125( 12), 121106-1-121106-10. doi:10.1103/PhysRevLett.125.121106 -
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. Features of the energy spectrum of cosmic rays above 2.5 × 10^18 eV using the Pierre Auger Observatory [Internet]. Physical Review Letters. 2020 ; 125( 12): 121106-1-121106-10.[citado 2025 ago. 04 ] Available from: https://doi.org/10.1103/PhysRevLett.125.121106 -
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. Features of the energy spectrum of cosmic rays above 2.5 × 10^18 eV using the Pierre Auger Observatory [Internet]. Physical Review Letters. 2020 ; 125( 12): 121106-1-121106-10.[citado 2025 ago. 04 ] Available from: https://doi.org/10.1103/PhysRevLett.125.121106 - 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
- Direct measurement of the muonic content of extensive air showers between 2 × 10^17 and 2 × 10^18 eV at the Pierre Auger Observatory
- Calibration of the underground muon detector of the Pierre Auger Observatory
- 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
- Measurement of the cosmic-ray energy spectrum above 2.5 × 10 18 eV using the Pierre Auger Observatory
- Extraction of the muon signals recorded with the surface detector of the Pierre Auger Observatory using recurrent neural networks
- Reconstruction of events recorded 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
- Design and implementation of the AMIGA embedded system for data acquisition
Informações sobre o DOI: 10.1103/PhysRevLett.125.121106 (Fonte: oaDOI API)
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