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Artigo de periodico
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 (2024)
Halim, Adila Binti Abdul; Catalani, Fernando ; Souza, Vitor de ; Oliveira, Cainã de ; Pérez Armand, Johnnier; Santos, Edivaldo Moura ; Peixoto, Carlos Jose Todero
Fonte: Journal of Cosmology and Astroparticle Physics. Unidades: IFSC, EEL, IF
Assuntos: TELESCÓPIOS, OBSERVATÓRIOS, RAIOS CÓSMICOS, ASTROFÍSICA
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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: 06 nov. 2025.
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 2025 nov. 06 ] 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 2025 nov. 06 ] Available from: http://dx.doi.org/10.1088/1475-7516/2024/01/022
Artigo de periodico
Impact of the magnetic horizon on the interpretation of the Pierre Auger Observatory spectrum and composition data (2024)
Halim, Adila Binti Abdul; Catalani, Fernando ; Souza, Vitor de ; Oliveira, Cainã de ; Pérez Armand, Johnnier; Santos, Edivaldo Moura ; Peixoto, Carlos Jose Todero
Fonte: Journal of Cosmology and Astroparticle Physics. Unidades: EEL, IFSC, IF
Assuntos: TELESCÓPIOS, OBSERVATÓRIOS, RAIOS CÓSMICOS, ASTROFÍSICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
HALIM, Adila Binti Abdul et al. Impact of the magnetic horizon on the interpretation of the Pierre Auger Observatory spectrum and composition data. Journal of Cosmology and Astroparticle Physics, v. 2024, n. 7, p. 094-1-094-30, 2024Tradução . . Disponível em: https://doi.org/10.1088/1475-7516/2024/07/094. Acesso em: 06 nov. 2025.
APA
Halim, A. B. A., Catalani, F., Souza, V. de, Oliveira, C. de, Pérez Armand, J., Santos, E. M., & Peixoto, C. J. T. (2024). Impact of the magnetic horizon on the interpretation of the Pierre Auger Observatory spectrum and composition data. Journal of Cosmology and Astroparticle Physics, 2024( 7), 094-1-094-30. doi:10.1088/1475-7516/2024/07/094
NLM
Halim ABA, Catalani F, Souza V de, Oliveira C de, Pérez Armand J, Santos EM, Peixoto CJT. Impact of the magnetic horizon on the interpretation of the Pierre Auger Observatory spectrum and composition data [Internet]. Journal of Cosmology and Astroparticle Physics. 2024 ; 2024( 7): 094-1-094-30.[citado 2025 nov. 06 ] Available from: https://doi.org/10.1088/1475-7516/2024/07/094
Vancouver
Halim ABA, Catalani F, Souza V de, Oliveira C de, Pérez Armand J, Santos EM, Peixoto CJT. Impact of the magnetic horizon on the interpretation of the Pierre Auger Observatory spectrum and composition data [Internet]. Journal of Cosmology and Astroparticle Physics. 2024 ; 2024( 7): 094-1-094-30.[citado 2025 nov. 06 ] Available from: https://doi.org/10.1088/1475-7516/2024/07/094
Artigo de periodico
Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants (2023)
Acero, Fabio; Catalani, Fernando ; Dal Pino, Elisabete Maria de Gouveia ; Souza, Vitor de ; Gonçalves, Diego Antonio Falceta ; Silva, Rodrigo Nemmen da ; Pereira, Luiz Augusto Stuani; Viana, Aion
Fonte: Astroparticle Physics. Unidades: IFSC, EEL, IAG, EACH
Assuntos: RAIOS CÓSMICOS, RAIOS GAMA, ANÁLISE DE DADOS, SUPERNOVAS, TELESCÓPIOS, HÁDRONS, ASTROFÍSICA
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ABNT
ACERO, Fabio et al. Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants. Astroparticle Physics, v. 150, 2023Tradução . . Disponível em: https://doi.org/10.1016/j.astropartphys.2023.102850. Acesso em: 06 nov. 2025.
APA
Acero, F., Catalani, F., Dal Pino, E. M. de G., Souza, V. de, Gonçalves, D. A. F., Silva, R. N. da, et al. (2023). Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants. Astroparticle Physics, 150. doi:10.1016/j.astropartphys.2023.102850
NLM
Acero F, Catalani F, Dal Pino EM de G, Souza V de, Gonçalves DAF, Silva RN da, Pereira LAS, Viana A. Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants [Internet]. Astroparticle Physics. 2023 ; 150[citado 2025 nov. 06 ] Available from: https://doi.org/10.1016/j.astropartphys.2023.102850
Vancouver
Acero F, Catalani F, Dal Pino EM de G, Souza V de, Gonçalves DAF, Silva RN da, Pereira LAS, Viana A. Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants [Internet]. Astroparticle Physics. 2023 ; 150[citado 2025 nov. 06 ] Available from: https://doi.org/10.1016/j.astropartphys.2023.102850
Artigo de periodico
Galactic Center as an efficient source of cosmic rays (2020)
Anjos, Rita de Cássia dos ; Catalani, Fernando
Fonte: Physical review d. Unidade: EEL
Assuntos: RAIOS CÓSMICOS, COSMOLOGIA, GRAVIDADE, ASTROFÍSICA
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ABNT
ANJOS, Rita de Cássia dos e CATALANI, Fernando. Galactic Center as an efficient source of cosmic rays. Physical review d, n. , p. 123015-, 2020Tradução . . Disponível em: https://doi.org/10.1103/PhysRevD.101.123015. Acesso em: 06 nov. 2025.
APA
Anjos, R. de C. dos, & Catalani, F. (2020). Galactic Center as an efficient source of cosmic rays. Physical review d, ( ), 123015-. doi:10.1103/PhysRevD.101.123015
NLM
Anjos R de C dos, Catalani F. Galactic Center as an efficient source of cosmic rays [Internet]. Physical review d. 2020 ;( ): 123015-.[citado 2025 nov. 06 ] Available from: https://doi.org/10.1103/PhysRevD.101.123015
Vancouver
Anjos R de C dos, Catalani F. Galactic Center as an efficient source of cosmic rays [Internet]. Physical review d. 2020 ;( ): 123015-.[citado 2025 nov. 06 ] Available from: https://doi.org/10.1103/PhysRevD.101.123015

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