Source: Physical Review Letters. Unidades: EEL, IFSC, IF
Subjects: RAIOS CÓSMICOS, FÍSICA DE ALTA ENERGIA, ASTROFÍSICA
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AAB, A. et al. Features of the energy spectrum of cosmic rays above 2.5 × 10^18 eV using the Pierre Auger Observatory. Physical Review Letters, v. 125, n. 12, p. 121106-1-121106-10, 2020Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.125.121106. Acesso em: 19 set. 2024.APA
Aab, A., Arbeletche, L. B., Catalani, F., Souza, V. de, Lang, R. G., Martínez-Huerta, H., et al. (2020). Features of the energy spectrum of cosmic rays above 2.5 × 10^18 eV using the Pierre Auger Observatory. Physical Review Letters, 125( 12), 121106-1-121106-10. doi:10.1103/PhysRevLett.125.121106NLM
Aab A, Arbeletche LB, Catalani F, Souza V de, Lang RG, Martínez-Huerta H, Armand JP, Carvalho Junior WR de, Santos EM, Peixoto CJT. Features of the energy spectrum of cosmic rays above 2.5 × 10^18 eV using the Pierre Auger Observatory [Internet]. Physical Review Letters. 2020 ; 125( 12): 121106-1-121106-10.[citado 2024 set. 19 ] Available from: https://doi.org/10.1103/PhysRevLett.125.121106Vancouver
Aab A, Arbeletche LB, Catalani F, Souza V de, Lang RG, Martínez-Huerta H, Armand JP, Carvalho Junior WR de, Santos EM, Peixoto CJT. Features of the energy spectrum of cosmic rays above 2.5 × 10^18 eV using the Pierre Auger Observatory [Internet]. Physical Review Letters. 2020 ; 125( 12): 121106-1-121106-10.[citado 2024 set. 19 ] Available from: https://doi.org/10.1103/PhysRevLett.125.121106