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 (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: 10.1103/PhysRevLett.134.021001
- Subjects: RAIOS CÓSMICOS; APRENDIZAGEM PROFUNDA; ASTROFÍSICA; OBSERVATÓRIOS
- Agências de fomento:
- Financiamento ANPCyT
- Financiamento Conicet, Argentina
- Financiamento ARC
- Financiamento FNRS, Bélgica
- Financiamento FWO
- Financiamento CNPq
- Financiamento FINEP
- Financiamento FAPERJ
- Financiamento FAPESP
- Financiamento MCTIC
- Financiamento CNRS
- Financiamento BMBF
- Financiamento DFG
- Financiamento Helmholtz-Gemeinschaft
- Financiamento INAF
- Financiamento Conacyt, Mexico
- Financiamento PAPIIT/UNAM
- Financiamento NWO
- Financiamento Ministry of Science and Higher Education, Poland
- Financiamento NCN
- Financiamento FEDER
- Financiamento UEFISCDI
- Financiamento ARRS
- Financiamento Consellería de Innovación e Industria/Xunta de Galicia, Santiago de Compostela, España
- Financiamento Junta de Andalucía, España
- Financiamento DOE
- Financiamento Grainger Foundation
- Financiamento Marie Curie International Research Staff Exchange Scheme Fellowship
- Language: Inglês
- Imprenta:
- Publisher place: College Park
- Date published: 2025
- Source:
- Título: Physical Review Letters
- ISSN: 0031-9007
- Volume/Número/Paginação/Ano: v. 134, n. 2, p. 021001-1-021001-10, Jan. 2025
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: hybrid
- Licença: cc-by
-
ABNT
HALIM, Adila Binti Abdul et al. 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. Physical Review Letters, v. 134, n. Ja 2025, p. 021001-1-021001-10, 2025Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.134.021001. Acesso em: 23 abr. 2025. -
APA
Halim, A. B. A., Catalani, F., Souza, V. de, Santos, E. M., Oliveira, C. de, & Peixoto, C. J. T. (2025). 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. Physical Review Letters, 134( Ja 2025), 021001-1-021001-10. doi:10.1103/PhysRevLett.134.021001 -
NLM
Halim ABA, Catalani F, Souza V de, Santos EM, Oliveira C de, Peixoto CJT. 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 [Internet]. Physical Review Letters. 2025 ; 134( Ja 2025): 021001-1-021001-10.[citado 2025 abr. 23 ] Available from: https://doi.org/10.1103/PhysRevLett.134.021001 -
Vancouver
Halim ABA, Catalani F, Souza V de, Santos EM, Oliveira C de, Peixoto CJT. 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 [Internet]. Physical Review Letters. 2025 ; 134( Ja 2025): 021001-1-021001-10.[citado 2025 abr. 23 ] Available from: https://doi.org/10.1103/PhysRevLett.134.021001 - Search for photons above 1018 eV by simultaneously measuring the atmospheric depth and the muon content of air showers at 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
- Large-scale cosmic-ray anisotropies with 19 yr of data from 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
- Radio measurements of the depth of air-shower maximum at the Pierre Auger Observatory
- Cosmological implications of photon-flux upper limits at ultrahigh energies in scenarios of Planckian-interacting massive particles for dark matter
- AugerPrime surface detector electronics
- Arrival directions of cosmic rays above 32 EeV from phase one of the Pierre Auger Observatory
- Search for ultra-high-energy photons from gravitational wave sources with the Pierre Auger Observatory
- A catalog of the highest-energy cosmic rays recorded during phase I of operation of the Pierre Auger Observatory
Informações sobre o DOI: 10.1103/PhysRevLett.134.021001 (Fonte: oaDOI API)
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