Filtros : " IFSC226" "Santos, Edivaldo Moura" Removidos: "Universidade Federal de São Carlos (UFSCar)" "Financiamento MINECO" Limpar

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  • Source: Physical Review D. Unidades: EEL, IFSC, IF

    Subjects: RAIOS CÓSMICOS, FLUORESCÊNCIA, ASTRONOMIA, ASTROFÍSICA

    Versão PublicadaAcesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      HALIM, Adila Binti Abdul et al. Radio measurements of the depth of air-shower maximum at the Pierre Auger Observatory. Physical Review D, v. 109, n. Ja 2024, p. 022002-1-022002-24, 2024Tradução . . Disponível em: https://doi.org/10.1103/PhysRevD.109.022002. Acesso em: 09 nov. 2024.
    • APA

      Halim, A. B. A., Catalani, F., Peixoto, C. J. T., Souza, V. de, Oliveira, C. de, Armand, J. P., & Santos, E. M. (2024). Radio measurements of the depth of air-shower maximum at the Pierre Auger Observatory. Physical Review D, 109( Ja 2024), 022002-1-022002-24. doi:10.1103/PhysRevD.109.022002
    • NLM

      Halim ABA, Catalani F, Peixoto CJT, Souza V de, Oliveira C de, Armand JP, Santos EM. Radio measurements of the depth of air-shower maximum at the Pierre Auger Observatory [Internet]. Physical Review D. 2024 ; 109( Ja 2024): 022002-1-022002-24.[citado 2024 nov. 09 ] Available from: https://doi.org/10.1103/PhysRevD.109.022002
    • Vancouver

      Halim ABA, Catalani F, Peixoto CJT, Souza V de, Oliveira C de, Armand JP, Santos EM. Radio measurements of the depth of air-shower maximum at the Pierre Auger Observatory [Internet]. Physical Review D. 2024 ; 109( Ja 2024): 022002-1-022002-24.[citado 2024 nov. 09 ] Available from: https://doi.org/10.1103/PhysRevD.109.022002
  • Source: Journal of Cosmology and Astroparticle Physics. Unidades: IFSC, IQ, IF, EEL

    Subjects: TELESCÓPIOS, OBSERVATÓRIOS, RAIOS CÓSMICOS, ASTROFÍSICA

    Versão PublicadaAcesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      HALIM, Adila Binti Abdul et al. Constraining models for the origin of ultra-high-energy cosmic rays with a novel combined analysis of arrival directions, spectrum, and composition data measured at the Pierre Auger Observatory. Journal of Cosmology and Astroparticle Physics, v. 2024, n. Ja 2024, p. 022-1-022-40, 2024Tradução . . Disponível em: http://dx.doi.org/10.1088/1475-7516/2024/01/022. Acesso em: 09 nov. 2024.
    • APA

      Halim, A. B. A., Catalani, F., Souza, V. de, Oliveira, C. de, Pérez Armand, J., Santos, E. M., & Peixoto, C. J. T. (2024). Constraining models for the origin of ultra-high-energy cosmic rays with a novel combined analysis of arrival directions, spectrum, and composition data measured at the Pierre Auger Observatory. Journal of Cosmology and Astroparticle Physics, 2024( Ja 2024), 022-1-022-40. doi:10.1088/1475-7516/2024/01/022
    • NLM

      Halim ABA, Catalani F, Souza V de, Oliveira C de, Pérez Armand J, Santos EM, Peixoto CJT. Constraining models for the origin of ultra-high-energy cosmic rays with a novel combined analysis of arrival directions, spectrum, and composition data measured at the Pierre Auger Observatory [Internet]. Journal of Cosmology and Astroparticle Physics. 2024 ; 2024( Ja 2024): 022-1-022-40.[citado 2024 nov. 09 ] Available from: http://dx.doi.org/10.1088/1475-7516/2024/01/022
    • Vancouver

      Halim ABA, Catalani F, Souza V de, Oliveira C de, Pérez Armand J, Santos EM, Peixoto CJT. Constraining models for the origin of ultra-high-energy cosmic rays with a novel combined analysis of arrival directions, spectrum, and composition data measured at the Pierre Auger Observatory [Internet]. Journal of Cosmology and Astroparticle Physics. 2024 ; 2024( Ja 2024): 022-1-022-40.[citado 2024 nov. 09 ] Available from: http://dx.doi.org/10.1088/1475-7516/2024/01/022

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