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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
Source: Journal of Cosmology and Astroparticle Physics. Unidades: IFSC, EEL, IF
Subjects: 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: 05 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. 05 ] 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. 05 ] 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
Source: Journal of Cosmology and Astroparticle Physics. Unidades: EEL, IFSC, IF
Subjects: 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: 05 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. 05 ] 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. 05 ] Available from: https://doi.org/10.1088/1475-7516/2024/07/094
Artigo de periodico
Sensitivity to sub-GeV dark matter from cosmic-ray scattering with very-high-energy gamma-ray observatories (2024)
Reis, Igor ; Moulin, Emmanuel ; Viana, Aion ; Gonçalves, Victor Paulo
Source: Journal of Cosmology and Astroparticle Physics. Unidade: IFSC
Subjects: RAIOS GAMA, MATÉRIA ESCURA, ASTROFÍSICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
REIS, Igor et al. Sensitivity to sub-GeV dark matter from cosmic-ray scattering with very-high-energy gamma-ray observatories. Journal of Cosmology and Astroparticle Physics, v. 2024, n. 7, p. 012-1-012-23, 2024Tradução . . Disponível em: https://doi.org/10.1088/1475-7516/2024/07/012. Acesso em: 05 nov. 2025.
APA
Reis, I., Moulin, E., Viana, A., & Gonçalves, V. P. (2024). Sensitivity to sub-GeV dark matter from cosmic-ray scattering with very-high-energy gamma-ray observatories. Journal of Cosmology and Astroparticle Physics, 2024( 7), 012-1-012-23. doi:10.1088/1475-7516/2024/07/012
NLM
Reis I, Moulin E, Viana A, Gonçalves VP. Sensitivity to sub-GeV dark matter from cosmic-ray scattering with very-high-energy gamma-ray observatories [Internet]. Journal of Cosmology and Astroparticle Physics. 2024 ; 2024( 7): 012-1-012-23.[citado 2025 nov. 05 ] Available from: https://doi.org/10.1088/1475-7516/2024/07/012
Vancouver
Reis I, Moulin E, Viana A, Gonçalves VP. Sensitivity to sub-GeV dark matter from cosmic-ray scattering with very-high-energy gamma-ray observatories [Internet]. Journal of Cosmology and Astroparticle Physics. 2024 ; 2024( 7): 012-1-012-23.[citado 2025 nov. 05 ] Available from: https://doi.org/10.1088/1475-7516/2024/07/012
Artigo de periodico
Uncertainties in measuring the dark matter signal from milky way satellites using Cherenkov telescopes (2023)
Kherlakian, Maria Carolina; Viana, Aion ; Souza, Vitor de
Source: Journal of Cosmology and Astroparticle Physics. Unidade: IFSC
Subjects: TELESCÓPIOS, GALÁXIAS, MATÉRIA ESCURA, RAIOS GAMA, ASTROFÍSICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
KHERLAKIAN, Maria Carolina e VIANA, Aion e SOUZA, Vitor de. Uncertainties in measuring the dark matter signal from milky way satellites using Cherenkov telescopes. Journal of Cosmology and Astroparticle Physics, v. 2023, p. 025-1-025-14, 2023Tradução . . Disponível em: https://doi.org/10.1088/1475-7516/2023/03/025. Acesso em: 05 nov. 2025.
APA
Kherlakian, M. C., Viana, A., & Souza, V. de. (2023). Uncertainties in measuring the dark matter signal from milky way satellites using Cherenkov telescopes. Journal of Cosmology and Astroparticle Physics, 2023, 025-1-025-14. doi:10.1088/1475-7516/2023/03/025
NLM
Kherlakian MC, Viana A, Souza V de. Uncertainties in measuring the dark matter signal from milky way satellites using Cherenkov telescopes [Internet]. Journal of Cosmology and Astroparticle Physics. 2023 ; 2023 025-1-025-14.[citado 2025 nov. 05 ] Available from: https://doi.org/10.1088/1475-7516/2023/03/025
Vancouver
Kherlakian MC, Viana A, Souza V de. Uncertainties in measuring the dark matter signal from milky way satellites using Cherenkov telescopes [Internet]. Journal of Cosmology and Astroparticle Physics. 2023 ; 2023 025-1-025-14.[citado 2025 nov. 05 ] Available from: https://doi.org/10.1088/1475-7516/2023/03/025

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