AugerPrime surface detector electronics: requirements, verification and performance (2025)
- Authors:
- USP affiliated authors: CATALANI, FERNANDO - EEL ; SOUZA FILHO, LUIZ VITOR DE - IFSC ; SANTOS, EDIVALDO MOURA - IF ; PEIXOTO, CARLOS JOSÉ TODERO - EEL ; OLIVEIRA, CAINÃ DE - IFSC
- Unidades: EEL; IFSC; IF
- DOI: 10.22323/1.501.0197
- Subjects: RAIOS CÓSMICOS; OBSERVATÓRIOS; ASTROFÍSICA
- Language: Inglês
- Imprenta:
- Source:
- Título: Proceedings of Science
- ISSN: 1824-8039
- Volume/Número/Paginação/Ano: v. 501, p. 197-1-197-7, Dec. 2025
- Conference titles: International Cosmic Ray Conference - ICRC
- Este periódico é de acesso aberto
- Este artigo NÃO é de acesso aberto
-
ABNT
BOHÁČOVÁ, Martina et al. AugerPrime surface detector electronics: requirements, verification and performance. Proceedings of Science. Trieste: Escola de Engenharia de Lorena, Universidade de São Paulo. Disponível em: https://doi.org/10.22323/1.501.0197. Acesso em: 13 fev. 2026. , 2025 -
APA
Boháčová, M., Catalani, F., Souza, V. de, Oliveira, C. de, Santos, E. M., & Peixoto, C. J. T. (2025). AugerPrime surface detector electronics: requirements, verification and performance. Proceedings of Science. Trieste: Escola de Engenharia de Lorena, Universidade de São Paulo. doi:10.22323/1.501.0197 -
NLM
Boháčová M, Catalani F, Souza V de, Oliveira C de, Santos EM, Peixoto CJT. AugerPrime surface detector electronics: requirements, verification and performance [Internet]. Proceedings of Science. 2025 ; 501 197-1-197-7.[citado 2026 fev. 13 ] Available from: https://doi.org/10.22323/1.501.0197 -
Vancouver
Boháčová M, Catalani F, Souza V de, Oliveira C de, Santos EM, Peixoto CJT. AugerPrime surface detector electronics: requirements, verification and performance [Internet]. Proceedings of Science. 2025 ; 501 197-1-197-7.[citado 2026 fev. 13 ] Available from: https://doi.org/10.22323/1.501.0197 - Search for a diffuse flux of photons with energies above tens of PeV at the Pierre Auger Observatory
- The Pierre Auger Observatory open data
- Scaler rates from the Pierre Auger Observatory: a new proxy of solar activity
- Search for photons above 1018 eV by simultaneously measuring the atmospheric depth and the muon content of air showers at the Pierre Auger Observatory
- The scintillator surface detector of the Pierre Auger observatory
- Large-scale cosmic-ray anisotropies with 19 yr of data from the Pierre Auger Observatory
- Measurement of the depth of maximum of air-shower profiles with energies between 10^18.5 and 10^20 eV using the surface detector of the Pierre Auger Observatory and deep learning
- 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
- Energy spectrum of ultrahigh-energy cosmic rays across declinations −90° to + 44.8° as measured at the Pierre Auger Observatory
- A search for photons with energies above 2×1017eV using hybrid data from the low-energy extensions of the Pierre Auger Observatory
Informações sobre o DOI: 10.22323/1.501.0197 (Fonte: oaDOI API)
Download do texto completo
| Tipo | Nome | Link | |
|---|---|---|---|
 |
PROD038099_3289210.pdf | Direct link |
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
