Auger@TA: a collaborative approach to cross-calibrating the world’s largest cosmic ray observatories (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: 10.22323/1.501.0182
- Subjects: RAIOS GAMA; ASTROFÍSICA
- Agências de fomento:
- Language: Inglês
- Imprenta:
- Source:
- Título: Proceedings of Science
- ISSN: 1824-8039
- Volume/Número/Paginação/Ano: v. 501, p. 182-1-182-15, Sept. 2025
- Conference titles: International Cosmic Ray Conference - ICRC
- Este periódico é de acesso aberto
- Este artigo NÃO é de acesso aberto
-
ABNT
MOCELLIN, Adriel Gustavo Bartz et al. Auger@TA: a collaborative approach to cross-calibrating the world’s largest cosmic ray observatories. Proceedings of Science. Trieste: Escola de Engenharia de Lorena, Universidade de São Paulo. Disponível em: https://doi.org/10.22323/1.501.0182. Acesso em: 21 jan. 2026. , 2025 -
APA
Mocellin, A. G. B., Catalani, F., Souza, V. de, Oliveira, C. de, Santos, E. M., & Peixoto, C. J. T. (2025). Auger@TA: a collaborative approach to cross-calibrating the world’s largest cosmic ray observatories. Proceedings of Science. Trieste: Escola de Engenharia de Lorena, Universidade de São Paulo. doi:10.22323/1.501.0182 -
NLM
Mocellin AGB, Catalani F, Souza V de, Oliveira C de, Santos EM, Peixoto CJT. Auger@TA: a collaborative approach to cross-calibrating the world’s largest cosmic ray observatories [Internet]. Proceedings of Science. 2025 ; 501 182-1-182-15.[citado 2026 jan. 21 ] Available from: https://doi.org/10.22323/1.501.0182 -
Vancouver
Mocellin AGB, Catalani F, Souza V de, Oliveira C de, Santos EM, Peixoto CJT. Auger@TA: a collaborative approach to cross-calibrating the world’s largest cosmic ray observatories [Internet]. Proceedings of Science. 2025 ; 501 182-1-182-15.[citado 2026 jan. 21 ] Available from: https://doi.org/10.22323/1.501.0182 - Reconstruction of the depth of the shower maximum of air showers with the SD-750 surface detector of the Pierre Auger Observatory using neural networks
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- 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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- Search for photons above 1018 eV by simultaneously measuring the atmospheric depth and the muon content of air showers at the Pierre Auger Observatory
- Search for a diffuse flux of photons with energies above tens of PeV at the Pierre Auger Observatory
- Scaler rates from the Pierre Auger Observatory: a new proxy of solar activity
Informações sobre o DOI: 10.22323/1.501.0182 (Fonte: oaDOI API)
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