An indication of anisotropy in arrival directions of ultra-high-energy cosmic rays through comparison to the flux pattern of extragalactic gamma-ray sources (2018)
- Authors:
- USP affiliated authors: ALBUQUERQUE, IVONE FREIRE DA MOTA E - IF ; CATALANI, FERNANDO - EEL ; SOUZA FILHO, LUIZ VITOR DE - IFSC ; SANTOS, EDIVALDO MOURA - IF ; PEIXOTO, CARLOS JOSÉ TODERO - EEL
- Unidades: IF; EEL; IFSC
- DOI: 10.3847/2041-8213/aaa66d
- Subjects: RAIOS CÓSMICOS; ASTROFÍSICA; OBSERVATÓRIOS
- Keywords: Astroparticle physics; Cosmic rays; Galaxies: active; Galaxies: starburst; Methods: data analysis
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: Astrophysical Journal Letters
- ISSN: 2041-8205
- Volume/Número/Paginação/Ano: v. 853, n. 2, p. L29-1-L29-10, Feb. 2018
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: bronze
-
ABNT
AAB, A. et al. An indication of anisotropy in arrival directions of ultra-high-energy cosmic rays through comparison to the flux pattern of extragalactic gamma-ray sources. Astrophysical Journal Letters, v. 853, n. 2, p. L29-1-L29-10, 2018Tradução . . Disponível em: https://doi.org/10.3847/2041-8213/aaa66d. Acesso em: 19 abr. 2024. -
APA
Aab, A., Albuquerque, I. F. da M. e, Catalani, F., Souza, V. de, Kemmerich, N., Lang, R. G., et al. (2018). An indication of anisotropy in arrival directions of ultra-high-energy cosmic rays through comparison to the flux pattern of extragalactic gamma-ray sources. Astrophysical Journal Letters, 853( 2), L29-1-L29-10. doi:10.3847/2041-8213/aaa66d -
NLM
Aab A, Albuquerque IF da M e, Catalani F, Souza V de, Kemmerich N, Lang RG, Prado RR, Carvalho WR de, Santos EM, Peixoto CJT. An indication of anisotropy in arrival directions of ultra-high-energy cosmic rays through comparison to the flux pattern of extragalactic gamma-ray sources [Internet]. Astrophysical Journal Letters. 2018 ; 853( 2): L29-1-L29-10.[citado 2024 abr. 19 ] Available from: https://doi.org/10.3847/2041-8213/aaa66d -
Vancouver
Aab A, Albuquerque IF da M e, Catalani F, Souza V de, Kemmerich N, Lang RG, Prado RR, Carvalho WR de, Santos EM, Peixoto CJT. An indication of anisotropy in arrival directions of ultra-high-energy cosmic rays through comparison to the flux pattern of extragalactic gamma-ray sources [Internet]. Astrophysical Journal Letters. 2018 ; 853( 2): L29-1-L29-10.[citado 2024 abr. 19 ] Available from: https://doi.org/10.3847/2041-8213/aaa66d - Inferences on mass composition and tests of hadronic interactions from 0.3 to 100 EeV using the water-Cherenkov detectors of the Pierre Auger Observatory
- A new method to determine the energy scale for high-energy cosmic rays using radio measurements at the Pierre Auger Observatory
- Report of the Telescope Array - Pierre Auger Observatory working group on energy spectrum
- All-sky search for correlations in the arrival directions of astrophysical neutrino candidates and ultrahigh-energy cosmic rays
- Peculiar lightning-related events observed by the surface detector of the Pierre Auger Observatory
- The Pierre Auger Observatory Upgrade
- First results from the AugerPrime engineering array
- AugerPrime: the upgrade program of the Pierre Auger Observatory
- Dipolar anisotropy of cosmic rays above 8 EeV
- <Xmax> measurements and tests of hadronic models using the surface detector of the Pierre Auger Observatory
Informações sobre o DOI: 10.3847/2041-8213/aaa66d (Fonte: oaDOI API)
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