Scaler rates from the Pierre Auger Observatory: a new proxy of solar activity (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: 10.3847/1538-4357/adccc3
- Subjects: RAIOS CÓSMICOS; FÍSICA DE ALTA ENERGIA; ASTROFÍSICA
- Agências de fomento:
- Language: Inglês
- Imprenta:
- Publisher place: Philadelphia
- Date published: 2025
- Source:
- Título: Astrophysical Journal
- ISSN: 1538-4357
- Volume/Número/Paginação/Ano: v. 987, n. 1, p. 41-1-41-13, July 2025
- Este periódico é de acesso aberto
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: gold
- Licença: cc-by
-
ABNT
HALIM, Adila Binti Abdul et al. Scaler rates from the Pierre Auger Observatory: a new proxy of solar activity. Astrophysical Journal, v. 987, n. 1, p. 41-1-41-13, 2025Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/adccc3. Acesso em: 26 dez. 2025. -
APA
Halim, A. B. A., Catalani, F., Souza, V. de, Oliveira, C. de, Santos, E. M., & Peixoto, C. J. T. (2025). Scaler rates from the Pierre Auger Observatory: a new proxy of solar activity. Astrophysical Journal, 987( 1), 41-1-41-13. doi:10.3847/1538-4357/adccc3 -
NLM
Halim ABA, Catalani F, Souza V de, Oliveira C de, Santos EM, Peixoto CJT. Scaler rates from the Pierre Auger Observatory: a new proxy of solar activity [Internet]. Astrophysical Journal. 2025 ; 987( 1): 41-1-41-13.[citado 2025 dez. 26 ] Available from: https://doi.org/10.3847/1538-4357/adccc3 -
Vancouver
Halim ABA, Catalani F, Souza V de, Oliveira C de, Santos EM, Peixoto CJT. Scaler rates from the Pierre Auger Observatory: a new proxy of solar activity [Internet]. Astrophysical Journal. 2025 ; 987( 1): 41-1-41-13.[citado 2025 dez. 26 ] Available from: https://doi.org/10.3847/1538-4357/adccc3 - The Pierre Auger Observatory open data
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- Large-scale cosmic-ray anisotropies with 19 yr of data from the Pierre Auger Observatory
- Auger@TA: a collaborative approach to cross-calibrating the world’s largest cosmic ray observatories
- 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
- 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
Informações sobre o DOI: 10.3847/1538-4357/adccc3 (Fonte: oaDOI API)
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