Measurement of the cosmic-ray energy spectrum above 2.5 × 10 18 eV using the Pierre Auger Observatory (2020)
- Authors:
- USP affiliated authors: CATALANI, FERNANDO - EEL ; PEIXOTO, CARLOS JOSÉ TODERO - EEL ; SANTOS, EDIVALDO MOURA - IF ; SOUZA FILHO, LUIZ VITOR DE - IFSC ; HUERTA, HUMBERTO MARTINEZ - IFSC ; LANG, RODRIGO GUEDES - IFSC ; ARMAND, JOHNNIER PÉREZ - IF ; CARVALHO JUNIOR, WASHINGTON RODRIGUES DE - IF ; ARBELETCHE, LUAN BONNEAU - IFSC
- Unidades: EEL; IF; IFSC
- DOI: 10.1103/PhysRevD.102.062005
- Subjects: RAIOS CÓSMICOS; ASTROFÍSICA; OBSERVATÓRIOS
- Agências de fomento:
- Language: Inglês
- Imprenta:
- Publisher place: College Park
- Date published: 2020
- Source:
- Título: Physical Review D
- ISSN: 2470-0010
- Volume/Número/Paginação/Ano: v. 102, n. 6, p. 062005-1-062005-27, Sept. 2020
- Este periódico é de acesso aberto
- Este artigo NÃO é de acesso aberto
-
ABNT
AAB, A. et al. Measurement of the cosmic-ray energy spectrum above 2.5 × 10 18 eV using the Pierre Auger Observatory. Physical Review D, v. 102, n. 6, p. 062005-1-062005-27, 2020Tradução . . Disponível em: https://doi.org/10.1103/PhysRevD.102.062005. Acesso em: 16 fev. 2026. -
APA
Aab, A., Armand, J. P., Carvalho Junior, W. R. de, Santos, E. M., Arbeletche, L. B., Peixoto, C. J. T., et al. (2020). Measurement of the cosmic-ray energy spectrum above 2.5 × 10 18 eV using the Pierre Auger Observatory. Physical Review D, 102( 6), 062005-1-062005-27. doi:10.1103/PhysRevD.102.062005 -
NLM
Aab A, Armand JP, Carvalho Junior WR de, Santos EM, Arbeletche LB, Peixoto CJT, Catalani F, Souza V de, Lang RG, Martínez-Huerta H. Measurement of the cosmic-ray energy spectrum above 2.5 × 10 18 eV using the Pierre Auger Observatory [Internet]. Physical Review D. 2020 ; 102( 6): 062005-1-062005-27.[citado 2026 fev. 16 ] Available from: https://doi.org/10.1103/PhysRevD.102.062005 -
Vancouver
Aab A, Armand JP, Carvalho Junior WR de, Santos EM, Arbeletche LB, Peixoto CJT, Catalani F, Souza V de, Lang RG, Martínez-Huerta H. Measurement of the cosmic-ray energy spectrum above 2.5 × 10 18 eV using the Pierre Auger Observatory [Internet]. Physical Review D. 2020 ; 102( 6): 062005-1-062005-27.[citado 2026 fev. 16 ] Available from: https://doi.org/10.1103/PhysRevD.102.062005 - Deep-learning based reconstruction of the shower maximum 𝑿max using the water-Cherenkov detectors of the Pierre Auger Observatory
- Extraction of the muon signals recorded with the surface detector of the Pierre Auger Observatory using recurrent neural networks
- The FRAM robotic telescope for atmospheric monitoring at the Pierre Auger Observatory
- Design and implementation of the AMIGA embedded system for data acquisition
- Calibration of the underground muon detector of the Pierre Auger Observatory
- Measurement of the fluctuations in the number of muons in extensive air Showers with 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
- Direct measurement of the muonic content of extensive air showers between 2 × 10^17 and 2 × 10^18 eV 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
- Search for magnetically-induced signatures in the arrival directions of ultra-high-energy cosmic rays measured at the Pierre Auger Observatory
Informações sobre o DOI: 10.1103/PhysRevD.102.062005 (Fonte: oaDOI API)
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