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Artigo de periodico
Ultrahigh-energy cosmic rays dipole and beyond (2021)
Lang, Rodrigo Guedes ; Taylor, Andrew M.; Souza, Vitor de
Source: Physical Review D. Unidade: IFSC
Subjects: RAIOS CÓSMICOS, ASTROFÍSICA
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ABNT
LANG, Rodrigo Guedes e TAYLOR, Andrew M. e SOUZA, Vitor de. Ultrahigh-energy cosmic rays dipole and beyond. Physical Review D, v. 103, n. 6, p. 063005-1-063005-12, 2021Tradução . . Disponível em: https://doi.org/10.1103/PhysRevD.103.063005. Acesso em: 15 nov. 2024.
APA
Lang, R. G., Taylor, A. M., & Souza, V. de. (2021). Ultrahigh-energy cosmic rays dipole and beyond. Physical Review D, 103( 6), 063005-1-063005-12. doi:10.1103/PhysRevD.103.063005
NLM
Lang RG, Taylor AM, Souza V de. Ultrahigh-energy cosmic rays dipole and beyond [Internet]. Physical Review D. 2021 ; 103( 6): 063005-1-063005-12.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1103/PhysRevD.103.063005
Vancouver
Lang RG, Taylor AM, Souza V de. Ultrahigh-energy cosmic rays dipole and beyond [Internet]. Physical Review D. 2021 ; 103( 6): 063005-1-063005-12.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1103/PhysRevD.103.063005
Artigo de periodico
Revisiting the distance to the nearest ultrahigh energy cosmic ray source: effects of extragalactic magnetic fields (2020)
Lang, Rodrigo Guedes ; Taylor, Andrew M.; Ahlers, Markus ; Souza, Vitor de
Source: Physical Review D. Unidade: IFSC
Subjects: FÍSICA DE PARTÍCULAS, RAIOS CÓSMICOS
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ABNT
LANG, Rodrigo Guedes et al. Revisiting the distance to the nearest ultrahigh energy cosmic ray source: effects of extragalactic magnetic fields. Physical Review D, v. 102, n. 6, p. 063012-01-063012-11, 2020Tradução . . Disponível em: https://doi.org/10.1103/PhysRevD.102.063012. Acesso em: 15 nov. 2024.
APA
Lang, R. G., Taylor, A. M., Ahlers, M., & Souza, V. de. (2020). Revisiting the distance to the nearest ultrahigh energy cosmic ray source: effects of extragalactic magnetic fields. Physical Review D, 102( 6), 063012-01-063012-11. doi:10.1103/PhysRevD.102.063012
NLM
Lang RG, Taylor AM, Ahlers M, Souza V de. Revisiting the distance to the nearest ultrahigh energy cosmic ray source: effects of extragalactic magnetic fields [Internet]. Physical Review D. 2020 ; 102( 6): 063012-01-063012-11.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1103/PhysRevD.102.063012
Vancouver
Lang RG, Taylor AM, Ahlers M, Souza V de. Revisiting the distance to the nearest ultrahigh energy cosmic ray source: effects of extragalactic magnetic fields [Internet]. Physical Review D. 2020 ; 102( 6): 063012-01-063012-11.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1103/PhysRevD.102.063012
Artigo de periodico
Measurement of the cosmic-ray energy spectrum above 2.5 × 10 18 eV using the Pierre Auger Observatory (2020)
Aab, A.; Armand, Johnnier Pérez; Carvalho Junior, Washington Rodrigues de; Santos, Edivaldo Moura ; Arbeletche, Luan Bonneau; Peixoto, Carlos Jose Todero ; Catalani, Fernando; Souza, Vitor de ; Lang, Rodrigo Guedes ; Martínez-Huerta, Humberto
Source: Physical Review D. Unidades: EEL, IF, IFSC
Subjects: RAIOS CÓSMICOS, ASTROFÍSICA, OBSERVATÓRIOS
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ABNT
AAB, A. et al. Measurement of the cosmic-ray energy spectrum above 2.5 × 10 18 eV using the Pierre Auger Observatory. Physical Review D, v. 102, n. 6, p. 062005-1-062005-27, 2020Tradução . . Disponível em: https://doi.org/10.1103/PhysRevD.102.062005. Acesso em: 15 nov. 2024.
APA
Aab, A., Armand, J. P., Carvalho Junior, W. R. de, Santos, E. M., Arbeletche, L. B., Peixoto, C. J. T., et al. (2020). Measurement of the cosmic-ray energy spectrum above 2.5 × 10 18 eV using the Pierre Auger Observatory. Physical Review D, 102( 6), 062005-1-062005-27. doi:10.1103/PhysRevD.102.062005
NLM
Aab A, Armand JP, Carvalho Junior WR de, Santos EM, Arbeletche LB, Peixoto CJT, Catalani F, Souza V de, Lang RG, Martínez-Huerta H. Measurement of the cosmic-ray energy spectrum above 2.5 × 10 18 eV using the Pierre Auger Observatory [Internet]. Physical Review D. 2020 ; 102( 6): 062005-1-062005-27.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1103/PhysRevD.102.062005
Vancouver
Aab A, Armand JP, Carvalho Junior WR de, Santos EM, Arbeletche LB, Peixoto CJT, Catalani F, Souza V de, Lang RG, Martínez-Huerta H. Measurement of the cosmic-ray energy spectrum above 2.5 × 10 18 eV using the Pierre Auger Observatory [Internet]. Physical Review D. 2020 ; 102( 6): 062005-1-062005-27.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1103/PhysRevD.102.062005
Artigo de periodico
Dark Energy Survey Year 1 results: Methodology and projections for joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions (2019)
Baxter, E J; Lima, Marcos Vinicius Borges Teixeira
Source: Physical Review D. Unidade: IF
Subjects: COSMOLOGIA, MATÉRIA ESCURA
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ABNT
BAXTER, E J e LIMA, Marcos Vinicius Borges Teixeira. Dark Energy Survey Year 1 results: Methodology and projections for joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions. Physical Review D, v. 99, p. 023508/1-023508/22, 2019Tradução . . Disponível em: https://doi.org/10.1103/PhysRevD.99.023508. Acesso em: 15 nov. 2024.
APA
Baxter, E. J., & Lima, M. V. B. T. (2019). Dark Energy Survey Year 1 results: Methodology and projections for joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions. Physical Review D, 99, 023508/1-023508/22. doi:10.1103/PhysRevD.99.023508
NLM
Baxter EJ, Lima MVBT. Dark Energy Survey Year 1 results: Methodology and projections for joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions [Internet]. Physical Review D. 2019 ; 99 023508/1-023508/22.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1103/PhysRevD.99.023508
Vancouver
Baxter EJ, Lima MVBT. Dark Energy Survey Year 1 results: Methodology and projections for joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions [Internet]. Physical Review D. 2019 ; 99 023508/1-023508/22.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1103/PhysRevD.99.023508
Artigo de periodico
Dark Energy Survey Year 1 Results: Tomographic cross-correlations between Dark Energy Survey galaxies and CMB lensing from South Pole Telescope + Planck (2019)
Omori, Y; Lima, Marcos Vinicius Borges Teixeira
Source: Physical Review D. Unidade: IF
Subjects: COSMOLOGIA, GALÁXIAS
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ABNT
OMORI, Y e LIMA, Marcos Vinicius Borges Teixeira. Dark Energy Survey Year 1 Results: Tomographic cross-correlations between Dark Energy Survey galaxies and CMB lensing from South Pole Telescope + Planck. Physical Review D, v. 100, p. 043501/1-043501/18, 2019Tradução . . Disponível em: https://doi.org/10.1103/PhysRevD.100.043501. Acesso em: 15 nov. 2024.
APA
Omori, Y., & Lima, M. V. B. T. (2019). Dark Energy Survey Year 1 Results: Tomographic cross-correlations between Dark Energy Survey galaxies and CMB lensing from South Pole Telescope + Planck. Physical Review D, 100, 043501/1-043501/18. doi:10.1103/PhysRevD.100.043501
NLM
Omori Y, Lima MVBT. Dark Energy Survey Year 1 Results: Tomographic cross-correlations between Dark Energy Survey galaxies and CMB lensing from South Pole Telescope + Planck [Internet]. Physical Review D. 2019 ; 100 043501/1-043501/18.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1103/PhysRevD.100.043501
Vancouver
Omori Y, Lima MVBT. Dark Energy Survey Year 1 Results: Tomographic cross-correlations between Dark Energy Survey galaxies and CMB lensing from South Pole Telescope + Planck [Internet]. Physical Review D. 2019 ; 100 043501/1-043501/18.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1103/PhysRevD.100.043501
Artigo de periodico
Improved limits on Lorentz invariance violation from astrophysical gamma-ray sources (2019)
Lang, Rodrigo Guedes; Martínez-Huerta, Humberto; Souza, Vitor de
Source: Physical Review D. Unidade: IFSC
Subjects: ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
LANG, Rodrigo Guedes e MARTÍNEZ-HUERTA, Humberto e SOUZA, Vitor de. Improved limits on Lorentz invariance violation from astrophysical gamma-ray sources. Physical Review D, v. 99, n. 4, p. 043015-1-043015-9, 2019Tradução . . Disponível em: https://doi.org/10.1103/PhysRevD.99.043015. Acesso em: 15 nov. 2024.
APA
Lang, R. G., Martínez-Huerta, H., & Souza, V. de. (2019). Improved limits on Lorentz invariance violation from astrophysical gamma-ray sources. Physical Review D, 99( 4), 043015-1-043015-9. doi:10.1103/PhysRevD.99.043015
NLM
Lang RG, Martínez-Huerta H, Souza V de. Improved limits on Lorentz invariance violation from astrophysical gamma-ray sources [Internet]. Physical Review D. 2019 ; 99( 4): 043015-1-043015-9.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1103/PhysRevD.99.043015
Vancouver
Lang RG, Martínez-Huerta H, Souza V de. Improved limits on Lorentz invariance violation from astrophysical gamma-ray sources [Internet]. Physical Review D. 2019 ; 99( 4): 043015-1-043015-9.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1103/PhysRevD.99.043015
Artigo de periodico
Dark Energy Survey Year 1 Results: Cross-correlation between Dark Energy Survey Y1 galaxy weak lensing and South Pole Telescope + Planck CMB weak lensing (2019)
Omori, Y; Lima, Marcos Vinicius Borges Teixeira
Source: Physical Review D. Unidade: IF
Subjects: COSMOLOGIA, GALÁXIAS, LENTES GRAVITACIONAIS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
OMORI, Y e LIMA, Marcos Vinicius Borges Teixeira. Dark Energy Survey Year 1 Results: Cross-correlation between Dark Energy Survey Y1 galaxy weak lensing and South Pole Telescope + Planck CMB weak lensing. Physical Review D, v. 100, p. 043517/1-043517/16, 2019Tradução . . Disponível em: https://doi.org/10.1103/PhysRevD.100.043517. Acesso em: 15 nov. 2024.
APA
Omori, Y., & Lima, M. V. B. T. (2019). Dark Energy Survey Year 1 Results: Cross-correlation between Dark Energy Survey Y1 galaxy weak lensing and South Pole Telescope + Planck CMB weak lensing. Physical Review D, 100, 043517/1-043517/16. doi:10.1103/PhysRevD.100.043517
NLM
Omori Y, Lima MVBT. Dark Energy Survey Year 1 Results: Cross-correlation between Dark Energy Survey Y1 galaxy weak lensing and South Pole Telescope + Planck CMB weak lensing [Internet]. Physical Review D. 2019 ; 100 043517/1-043517/16.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1103/PhysRevD.100.043517
Vancouver
Omori Y, Lima MVBT. Dark Energy Survey Year 1 Results: Cross-correlation between Dark Energy Survey Y1 galaxy weak lensing and South Pole Telescope + Planck CMB weak lensing [Internet]. Physical Review D. 2019 ; 100 043517/1-043517/16.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1103/PhysRevD.100.043517
Artigo de periodico
Dark Energy Survey year 1 results: Joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions (2019)
Abbott, T M C; Lima, Marcos Vinicius Borges Teixeira
Source: Physical Review D. Unidade: IF
Subjects: COSMOLOGIA, GALÁXIAS, LENTES GRAVITACIONAIS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
ABBOTT, T M C e LIMA, Marcos Vinicius Borges Teixeira. Dark Energy Survey year 1 results: Joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions. Physical Review D, v. 100, p. 023541/1-023541/21, 2019Tradução . . Disponível em: https://doi.org/10.1103/PhysRevD.100.023541. Acesso em: 15 nov. 2024.
APA
Abbott, T. M. C., & Lima, M. V. B. T. (2019). Dark Energy Survey year 1 results: Joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions. Physical Review D, 100, 023541/1-023541/21. doi:10.1103/PhysRevD.100.023541
NLM
Abbott TMC, Lima MVBT. Dark Energy Survey year 1 results: Joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions [Internet]. Physical Review D. 2019 ; 100 023541/1-023541/21.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1103/PhysRevD.100.023541
Vancouver
Abbott TMC, Lima MVBT. Dark Energy Survey year 1 results: Joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions [Internet]. Physical Review D. 2019 ; 100 023541/1-023541/21.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1103/PhysRevD.100.023541

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