Filtros : "MATÉRIA ESCURA" "Reino Unido" Removido: "2002" Limpar

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  • Source: Journal of Cosmology and Astroparticle Physics. Unidade: IFSC

    Subjects: RAIOS GAMA, MATÉRIA ESCURA, ASTROFÍSICA

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      ANGEL, Silvia Lucía Correa et al. Constraining gamma-ray lines from dark matter annihilation using Fermi-LAT and H.E.S.S. data. Journal of Cosmology and Astroparticle Physics, v. 2024, p. 028-1-028-12, 2024Tradução . . Disponível em: https://doi.org/10.1088/1475-7516/2024/04/028. Acesso em: 26 jul. 2024.
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      Angel, S. L. C., Gambini, G., Guedes, L., Queiroz, F. da S., & Souza, V. de. (2024). Constraining gamma-ray lines from dark matter annihilation using Fermi-LAT and H.E.S.S. data. Journal of Cosmology and Astroparticle Physics, 2024, 028-1-028-12. doi:10.1088/1475-7516/2024/04/028
    • NLM

      Angel SLC, Gambini G, Guedes L, Queiroz F da S, Souza V de. Constraining gamma-ray lines from dark matter annihilation using Fermi-LAT and H.E.S.S. data [Internet]. Journal of Cosmology and Astroparticle Physics. 2024 ; 2024 028-1-028-12.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1088/1475-7516/2024/04/028
    • Vancouver

      Angel SLC, Gambini G, Guedes L, Queiroz F da S, Souza V de. Constraining gamma-ray lines from dark matter annihilation using Fermi-LAT and H.E.S.S. data [Internet]. Journal of Cosmology and Astroparticle Physics. 2024 ; 2024 028-1-028-12.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1088/1475-7516/2024/04/028
  • Source: Journal of Cosmology and Astroparticle Physics. Unidade: IFSC

    Subjects: RAIOS GAMA, MATÉRIA ESCURA, ASTROFÍSICA

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      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: 26 jul. 2024.
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      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 2024 jul. 26 ] 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 2024 jul. 26 ] Available from: https://doi.org/10.1088/1475-7516/2024/07/012
  • Source: Reports on Progress in Physics. Unidade: IF

    Assunto: MATÉRIA ESCURA

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      WANG, Bin et al. Further understanding the interaction between dark energy and dark matter: current status and future directions. Reports on Progress in Physics, v. 87, n. 3, 2024Tradução . . Disponível em: https://doi.org/10.1088/1361-6633/ad2527. Acesso em: 26 jul. 2024.
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      Wang, B., Abdalla, E., Atrio-Barandela, F., & Pavón, D. (2024). Further understanding the interaction between dark energy and dark matter: current status and future directions. Reports on Progress in Physics, 87( 3). doi:https://doi.org/10.1088/1361-6633/ad2527
    • NLM

      Wang B, Abdalla E, Atrio-Barandela F, Pavón D. Further understanding the interaction between dark energy and dark matter: current status and future directions [Internet]. Reports on Progress in Physics. 2024 ; 87( 3):[citado 2024 jul. 26 ] Available from: https://doi.org/10.1088/1361-6633/ad2527
    • Vancouver

      Wang B, Abdalla E, Atrio-Barandela F, Pavón D. Further understanding the interaction between dark energy and dark matter: current status and future directions [Internet]. Reports on Progress in Physics. 2024 ; 87( 3):[citado 2024 jul. 26 ] Available from: https://doi.org/10.1088/1361-6633/ad2527
  • Source: Classical and Quantum Gravity. Unidade: IFSC

    Subjects: MATÉRIA ESCURA, GRAVIDADE, FÍSICA DE ALTA ENERGIA, COSMOLOGIA

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      VANZELLA, Daniel Augusto Turolla. Gravity theories with local energy-momentum exchange: a closer look at Rastall-like gravity. Classical and Quantum Gravity, v. 40, n. 16, p. 165011-1-165011-24, 2023Tradução . . Disponível em: https://doi.org/10.1088/1361-6382/ace58a. Acesso em: 26 jul. 2024.
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      Vanzella, D. A. T. (2023). Gravity theories with local energy-momentum exchange: a closer look at Rastall-like gravity. Classical and Quantum Gravity, 40( 16), 165011-1-165011-24. doi:10.1088/1361-6382/ace58a
    • NLM

      Vanzella DAT. Gravity theories with local energy-momentum exchange: a closer look at Rastall-like gravity [Internet]. Classical and Quantum Gravity. 2023 ; 40( 16): 165011-1-165011-24.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1088/1361-6382/ace58a
    • Vancouver

      Vanzella DAT. Gravity theories with local energy-momentum exchange: a closer look at Rastall-like gravity [Internet]. Classical and Quantum Gravity. 2023 ; 40( 16): 165011-1-165011-24.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1088/1361-6382/ace58a
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IF

    Subjects: COSMOLOGIA, MATÉRIA ESCURA

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      LEMOS, Pablo e LIMA, Marcos Vinicius Borges Teixeira. Robust sampling for weak lensing and clustering analyses with the Dark Energy Survey. Monthly Notices of the Royal Astronomical Society, v. 521, n. 1, p. 1184–1199, 2023Tradução . . Disponível em: https://doi.org/10.1093/mnras/stac2786. Acesso em: 26 jul. 2024.
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      Lemos, P., & Lima, M. V. B. T. (2023). Robust sampling for weak lensing and clustering analyses with the Dark Energy Survey. Monthly Notices of the Royal Astronomical Society, 521( 1), 1184–1199. doi:10.1093/mnras/stac2786
    • NLM

      Lemos P, Lima MVBT. Robust sampling for weak lensing and clustering analyses with the Dark Energy Survey [Internet]. Monthly Notices of the Royal Astronomical Society. 2023 ; 521( 1): 1184–1199.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1093/mnras/stac2786
    • Vancouver

      Lemos P, Lima MVBT. Robust sampling for weak lensing and clustering analyses with the Dark Energy Survey [Internet]. Monthly Notices of the Royal Astronomical Society. 2023 ; 521( 1): 1184–1199.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1093/mnras/stac2786
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IF

    Subjects: COSMOLOGIA, MATÉRIA ESCURA

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      UPSDELL, E W e LIMA, Marcos Vinicius Borges Teixeira. The XMM cluster survey: exploring scaling relations and completeness of the dark energy survey year 3 redMaPPer cluster catalogue. Monthly Notices of the Royal Astronomical Society, v. 522, n. 4, p. 5267–5290, 2023Tradução . . Disponível em: https://doi.org/10.1093/mnras/stad1220. Acesso em: 26 jul. 2024.
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      Upsdell, E. W., & Lima, M. V. B. T. (2023). The XMM cluster survey: exploring scaling relations and completeness of the dark energy survey year 3 redMaPPer cluster catalogue. Monthly Notices of the Royal Astronomical Society, 522( 4), 5267–5290. doi:10.1093/mnras/stad1220
    • NLM

      Upsdell EW, Lima MVBT. The XMM cluster survey: exploring scaling relations and completeness of the dark energy survey year 3 redMaPPer cluster catalogue [Internet]. Monthly Notices of the Royal Astronomical Society. 2023 ; 522( 4): 5267–5290.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1093/mnras/stad1220
    • Vancouver

      Upsdell EW, Lima MVBT. The XMM cluster survey: exploring scaling relations and completeness of the dark energy survey year 3 redMaPPer cluster catalogue [Internet]. Monthly Notices of the Royal Astronomical Society. 2023 ; 522( 4): 5267–5290.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1093/mnras/stad1220
  • Source: Journal of Cosmology and Astroparticle Physics. Unidade: IFSC

    Subjects: TELESCÓPIOS, GALÁXIAS, MATÉRIA ESCURA, RAIOS GAMA, ASTROFÍSICA

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      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: 26 jul. 2024.
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      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 2024 jul. 26 ] 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 2024 jul. 26 ] Available from: https://doi.org/10.1088/1475-7516/2023/03/025
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IF

    Subjects: COSMOLOGIA, MATÉRIA ESCURA

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      PRAT, Judit e LIMA, Marcos Vinicius Borges Teixeira. Non-local contribution from small scales in galaxy–galaxy lensing: comparison of mitigation schemes. Monthly Notices of the Royal Astronomical Society, v. 522, n. 1, p. 412–425, 2023Tradução . . Disponível em: https://doi.org/10.1093/mnras/stad847. Acesso em: 26 jul. 2024.
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      Prat, J., & Lima, M. V. B. T. (2023). Non-local contribution from small scales in galaxy–galaxy lensing: comparison of mitigation schemes. Monthly Notices of the Royal Astronomical Society, 522( 1), 412–425. doi:10.1093/mnras/stad847
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      Prat J, Lima MVBT. Non-local contribution from small scales in galaxy–galaxy lensing: comparison of mitigation schemes [Internet]. Monthly Notices of the Royal Astronomical Society. 2023 ; 522( 1): 412–425.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1093/mnras/stad847
    • Vancouver

      Prat J, Lima MVBT. Non-local contribution from small scales in galaxy–galaxy lensing: comparison of mitigation schemes [Internet]. Monthly Notices of the Royal Astronomical Society. 2023 ; 522( 1): 412–425.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1093/mnras/stad847
  • Source: Journal of Cosmology and Astroparticle Physics. Unidades: IFSC, ICMC

    Subjects: OBSERVATÓRIOS, RAIOS GAMA, MATÉRIA ESCURA, ASTROFÍSICA

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      FORTES, Guilherme Nishina et al. Present and future constraints on secluded dark matter in the Galactic Halo with TeV Gamma-ray observatories. Journal of Cosmology and Astroparticle Physics, v. 2023, p. 043-1-043-18, 2023Tradução . . Disponível em: https://doi.org/10.1088/1475-7516/2023/07/043. Acesso em: 26 jul. 2024.
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      Fortes, G. N., Queiroz, F. da S., Siqueira, C. M., & Viana, A. (2023). Present and future constraints on secluded dark matter in the Galactic Halo with TeV Gamma-ray observatories. Journal of Cosmology and Astroparticle Physics, 2023, 043-1-043-18. doi:10.1088/1475-7516/2023/07/043
    • NLM

      Fortes GN, Queiroz F da S, Siqueira CM, Viana A. Present and future constraints on secluded dark matter in the Galactic Halo with TeV Gamma-ray observatories [Internet]. Journal of Cosmology and Astroparticle Physics. 2023 ; 2023 043-1-043-18.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1088/1475-7516/2023/07/043
    • Vancouver

      Fortes GN, Queiroz F da S, Siqueira CM, Viana A. Present and future constraints on secluded dark matter in the Galactic Halo with TeV Gamma-ray observatories [Internet]. Journal of Cosmology and Astroparticle Physics. 2023 ; 2023 043-1-043-18.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1088/1475-7516/2023/07/043
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IF

    Subjects: MATÉRIA ESCURA, GALÁXIAS, COSMOLOGIA

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      CHAN, Hei Yin Jowett et al. The diversity of core-halo structure in the fuzzy dark matter model. Monthly Notices of the Royal Astronomical Society, v. 511, n. 1, p. 943–952, 2022Tradução . . Disponível em: https://doi.org/10.1093/mnras/stac063. Acesso em: 26 jul. 2024.
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      Chan, H. Y. J., Ferreira, E. G. M., May, S., Hayashi, K., & Chiba, M. (2022). The diversity of core-halo structure in the fuzzy dark matter model. Monthly Notices of the Royal Astronomical Society, 511( 1), 943–952. doi:10.1093/mnras/stac063
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      Chan HYJ, Ferreira EGM, May S, Hayashi K, Chiba M. The diversity of core-halo structure in the fuzzy dark matter model [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 511( 1): 943–952.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1093/mnras/stac063
    • Vancouver

      Chan HYJ, Ferreira EGM, May S, Hayashi K, Chiba M. The diversity of core-halo structure in the fuzzy dark matter model [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 511( 1): 943–952.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1093/mnras/stac063
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IF

    Subjects: ASTROFÍSICA, COSMOLOGIA, AGLOMERADOS (GALÁXIA), MATÉRIA ESCURA, ESTRUTURA DO UNIVERSO

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      SANTI, Natali Soler Matubaro de et al. Mimicking the halo–galaxy connection using machine learning. Monthly Notices of the Royal Astronomical Society, v. 514, n. 2, p. 2463-2478, 2022Tradução . . Disponível em: https://doi.org/10.1093/mnras/stac1469. Acesso em: 26 jul. 2024.
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      Santi, N. S. M. de, Rodrigues, N. V. N., Dorta, A. D. M., Abramo, L. R., Tucci, B., & Artale, M. C. (2022). Mimicking the halo–galaxy connection using machine learning. Monthly Notices of the Royal Astronomical Society, 514( 2), 2463-2478. doi:10.1093/mnras/stac1469
    • NLM

      Santi NSM de, Rodrigues NVN, Dorta ADM, Abramo LR, Tucci B, Artale MC. Mimicking the halo–galaxy connection using machine learning [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 514( 2): 2463-2478.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1093/mnras/stac1469
    • Vancouver

      Santi NSM de, Rodrigues NVN, Dorta ADM, Abramo LR, Tucci B, Artale MC. Mimicking the halo–galaxy connection using machine learning [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 514( 2): 2463-2478.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1093/mnras/stac1469
  • Source: European Physical Journal C. Unidade: IF

    Subjects: ASTROFÍSICA, MATÉRIA ESCURA, ARGÔNIO, INFRAVERMELHO, FOTOLUMINESCÊNCIA, PARTÍCULAS ELEMENTARES, ESPALHAMENTO

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      AALSETH, C. E. e ALBUQUERQUE, Ivone e AVE, M. SiPM-matrix readout of two-phase argon detectors using electroluminescence in the visible and near infrared range. European Physical Journal C, v. 81, 2021Tradução . . Disponível em: https://doi.org/10.1140/epjc/s10052-020-08801-2. Acesso em: 26 jul. 2024.
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      Aalseth, C. E., Albuquerque, I., & Ave, M. (2021). SiPM-matrix readout of two-phase argon detectors using electroluminescence in the visible and near infrared range. European Physical Journal C, 81. doi:10.1140/epjc/s10052-020-08801-2
    • NLM

      Aalseth CE, Albuquerque I, Ave M. SiPM-matrix readout of two-phase argon detectors using electroluminescence in the visible and near infrared range [Internet]. European Physical Journal C. 2021 ; 81[citado 2024 jul. 26 ] Available from: https://doi.org/10.1140/epjc/s10052-020-08801-2
    • Vancouver

      Aalseth CE, Albuquerque I, Ave M. SiPM-matrix readout of two-phase argon detectors using electroluminescence in the visible and near infrared range [Internet]. European Physical Journal C. 2021 ; 81[citado 2024 jul. 26 ] Available from: https://doi.org/10.1140/epjc/s10052-020-08801-2
  • Source: Journal of Cosmology and Astroparticle Physics. Unidades: EEL, IAG, IFSC, EACH, IF

    Subjects: RAIOS GAMA, TELESCÓPIOS, MATÉRIA ESCURA

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      ACHARYYA, A. et al. Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre. Journal of Cosmology and Astroparticle Physics, v. 2021, n. Ja 2021, p. 057-1-057-62, 2021Tradução . . Disponível em: https://doi.org/10.1088/1475-7516/2021/01/057. Acesso em: 26 jul. 2024.
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      Acharyya, A., Batista, R. A., Arbeletche, L. B., Catalani, F., Dal Pino, E. M. de G., Souza, V. de, et al. (2021). Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre. Journal of Cosmology and Astroparticle Physics, 2021( Ja 2021), 057-1-057-62. doi:10.1088/1475-7516/2021/01/057
    • NLM

      Acharyya A, Batista RA, Arbeletche LB, Catalani F, Dal Pino EM de G, Souza V de, Giler AGD, Gonçalves DAF, Kherlakian MC, Martínez-Huerta H, Silva RN da, Santos EM, Peixoto CJT, Viana A. Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre [Internet]. Journal of Cosmology and Astroparticle Physics. 2021 ; 2021( Ja 2021): 057-1-057-62.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1088/1475-7516/2021/01/057
    • Vancouver

      Acharyya A, Batista RA, Arbeletche LB, Catalani F, Dal Pino EM de G, Souza V de, Giler AGD, Gonçalves DAF, Kherlakian MC, Martínez-Huerta H, Silva RN da, Santos EM, Peixoto CJT, Viana A. Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre [Internet]. Journal of Cosmology and Astroparticle Physics. 2021 ; 2021( Ja 2021): 057-1-057-62.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1088/1475-7516/2021/01/057
  • Source: Astrophysical Journal. Unidade: IFSC

    Subjects: RAIOS GAMA, TELESCÓPIOS, MATÉRIA ESCURA

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      ABDALLAH, H. e TANAKA, T. e VIANA, Aion. Search for dark matter annihilation signals from unidentified fermi-LAT objects with H.E.S.S. Astrophysical Journal, v. 918, n. 1, p. 017-1-017-14, 2021Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/abff59. Acesso em: 26 jul. 2024.
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      Abdallah, H., Tanaka, T., & Viana, A. (2021). Search for dark matter annihilation signals from unidentified fermi-LAT objects with H.E.S.S. Astrophysical Journal, 918( 1), 017-1-017-14. doi:10.3847/1538-4357/abff59
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      Abdallah H, Tanaka T, Viana A. Search for dark matter annihilation signals from unidentified fermi-LAT objects with H.E.S.S. [Internet]. Astrophysical Journal. 2021 ; 918( 1): 017-1-017-14.[citado 2024 jul. 26 ] Available from: https://doi.org/10.3847/1538-4357/abff59
    • Vancouver

      Abdallah H, Tanaka T, Viana A. Search for dark matter annihilation signals from unidentified fermi-LAT objects with H.E.S.S. [Internet]. Astrophysical Journal. 2021 ; 918( 1): 017-1-017-14.[citado 2024 jul. 26 ] Available from: https://doi.org/10.3847/1538-4357/abff59
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IF

    Subjects: COSMOLOGIA, MÉTODOS NUMÉRICOS, MATÉRIA ESCURA, GALÁXIAS, ESTRUTURA DO UNIVERSO, POLARIZAÇÃO (ASTRONOMIA)

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      SCHIEWALDT, Beatriz Tucci et al. The physical origins of low-mass spin bias. Monthly Notices of the Royal Astronomical Society, v. 500, p. 2777-2785, 2021Tradução . . Disponível em: https://doi.org/10.1093/mnras/staa3319. Acesso em: 26 jul. 2024.
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      Schiewaldt, B. T., Dorta, A. D. M., Abramo, L. R., Sato-Polito, G., & Artale, M. C. (2021). The physical origins of low-mass spin bias. Monthly Notices of the Royal Astronomical Society, 500, 2777-2785. doi:10.1093/mnras/staa3319
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      Schiewaldt BT, Dorta ADM, Abramo LR, Sato-Polito G, Artale MC. The physical origins of low-mass spin bias [Internet]. Monthly Notices of the Royal Astronomical Society. 2021 ; 500 2777-2785.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1093/mnras/staa3319
    • Vancouver

      Schiewaldt BT, Dorta ADM, Abramo LR, Sato-Polito G, Artale MC. The physical origins of low-mass spin bias [Internet]. Monthly Notices of the Royal Astronomical Society. 2021 ; 500 2777-2785.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1093/mnras/staa3319
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IF

    Subjects: COSMOLOGIA, MÉTODOS NUMÉRICOS, ESTRUTURA DO UNIVERSO, RELATIVIDADE (FÍSICA), GALÁXIAS, MATÉRIA ESCURA, POLARIZAÇÃO (ASTRONOMIA)

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      GUANDALIN, Caroline Macedo et al. Observing relativistic features in large-scale structure surveys - I. Multipoles of the power spectrum. Monthly Notices of the Royal Astronomical Society, v. 501, n. 2, p. 2547-2561, 2021Tradução . . Disponível em: https://doi.org/10.1093/mnras/staa3890. Acesso em: 26 jul. 2024.
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      Guandalin, C. M., Adamek, J., Bull, P., Clarkson, C., Abramo, L. R., & Coates, L. (2021). Observing relativistic features in large-scale structure surveys - I. Multipoles of the power spectrum. Monthly Notices of the Royal Astronomical Society, 501( 2), 2547-2561. doi:10.1093/mnras/staa3890
    • NLM

      Guandalin CM, Adamek J, Bull P, Clarkson C, Abramo LR, Coates L. Observing relativistic features in large-scale structure surveys - I. Multipoles of the power spectrum [Internet]. Monthly Notices of the Royal Astronomical Society. 2021 ; 501( 2): 2547-2561.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1093/mnras/staa3890
    • Vancouver

      Guandalin CM, Adamek J, Bull P, Clarkson C, Abramo LR, Coates L. Observing relativistic features in large-scale structure surveys - I. Multipoles of the power spectrum [Internet]. Monthly Notices of the Royal Astronomical Society. 2021 ; 501( 2): 2547-2561.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1093/mnras/staa3890
  • Source: Journal of Cosmology and Astroparticle Physics (JCAP). Unidade: IF

    Subjects: ASTROFÍSICA, MATÉRIA ESCURA, SUPERNOVAS, NEUTRINOS, ARGÔNIO

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      AGNES, P. e ALBUQUERQUE, Ivone e AVE, M. Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos. Journal of Cosmology and Astroparticle Physics (JCAP), v. 2021, p. 23 , 2021Tradução . . Disponível em: https://doi.org/10.1088/1475-7516/2021/03/043. Acesso em: 26 jul. 2024.
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      Agnes, P., Albuquerque, I., & Ave, M. (2021). Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos. Journal of Cosmology and Astroparticle Physics (JCAP), 2021, 23 . doi:10.1088/1475-7516/2021/03/043
    • NLM

      Agnes P, Albuquerque I, Ave M. Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos [Internet]. Journal of Cosmology and Astroparticle Physics (JCAP). 2021 ; 2021 23 .[citado 2024 jul. 26 ] Available from: https://doi.org/10.1088/1475-7516/2021/03/043
    • Vancouver

      Agnes P, Albuquerque I, Ave M. Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos [Internet]. Journal of Cosmology and Astroparticle Physics (JCAP). 2021 ; 2021 23 .[citado 2024 jul. 26 ] Available from: https://doi.org/10.1088/1475-7516/2021/03/043
  • Source: Journal of Cosmology and Astroparticle Physics. Unidades: EEL, IAG, IFSC, EACH, IF

    Subjects: RAIOS GAMA, TELESCÓPIOS, MATÉRIA ESCURA

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    • ABNT

      ABDALLAH, H. et al. Sensitivity of the Cherenkov Telescope Array for probing cosmology and fundamental physics with gamma-ray propagation. Journal of Cosmology and Astroparticle Physics, v. 2021, p. 048-1-048-63, 2021Tradução . . Disponível em: https://doi.org/10.1088/1475-7516/2021/02/048. Acesso em: 26 jul. 2024.
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      Abdallah, H., Batista, R. A., Arbeletche, L. B., Catalani, F., Dal Pino, E. M. de G., Lang, R. G., et al. (2021). Sensitivity of the Cherenkov Telescope Array for probing cosmology and fundamental physics with gamma-ray propagation. Journal of Cosmology and Astroparticle Physics, 2021, 048-1-048-63. doi:10.1088/1475-7516/2021/02/048
    • NLM

      Abdallah H, Batista RA, Arbeletche LB, Catalani F, Dal Pino EM de G, Lang RG, Souza V de, Giler AGD, Gonçalves DAF, Kherlakian MC, Martínez-Huerta H, Silva RN da, Santos EM, Peixoto CJT, Pimentel DR de M, Viana A. Sensitivity of the Cherenkov Telescope Array for probing cosmology and fundamental physics with gamma-ray propagation [Internet]. Journal of Cosmology and Astroparticle Physics. 2021 ; 2021 048-1-048-63.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1088/1475-7516/2021/02/048
    • Vancouver

      Abdallah H, Batista RA, Arbeletche LB, Catalani F, Dal Pino EM de G, Lang RG, Souza V de, Giler AGD, Gonçalves DAF, Kherlakian MC, Martínez-Huerta H, Silva RN da, Santos EM, Peixoto CJT, Pimentel DR de M, Viana A. Sensitivity of the Cherenkov Telescope Array for probing cosmology and fundamental physics with gamma-ray propagation [Internet]. Journal of Cosmology and Astroparticle Physics. 2021 ; 2021 048-1-048-63.[citado 2024 jul. 26 ] Available from: https://doi.org/10.1088/1475-7516/2021/02/048
  • Source: Astrophysical Journal Letters. Unidade: IF

    Subjects: ASTROFÍSICA, COSMOLOGIA, MATÉRIA ESCURA, GALÁXIAS

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    • ABNT

      HAYASHI, Kohei e FERREIRA, Elisa G. M. e CHAN, Hei Yin Jowett. Narrowing the Mass Range of Fuzzy Dark Matter with Ultrafaint Dwarfs. Astrophysical Journal Letters, v. 912, n. 1, 2021Tradução . . Disponível em: https://doi.org/10.3847/2041-8213/abf501. Acesso em: 26 jul. 2024.
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      Hayashi, K., Ferreira, E. G. M., & Chan, H. Y. J. (2021). Narrowing the Mass Range of Fuzzy Dark Matter with Ultrafaint Dwarfs. Astrophysical Journal Letters, 912( 1). doi:10.3847/2041-8213/abf501
    • NLM

      Hayashi K, Ferreira EGM, Chan HYJ. Narrowing the Mass Range of Fuzzy Dark Matter with Ultrafaint Dwarfs [Internet]. Astrophysical Journal Letters. 2021 ; 912( 1):[citado 2024 jul. 26 ] Available from: https://doi.org/10.3847/2041-8213/abf501
    • Vancouver

      Hayashi K, Ferreira EGM, Chan HYJ. Narrowing the Mass Range of Fuzzy Dark Matter with Ultrafaint Dwarfs [Internet]. Astrophysical Journal Letters. 2021 ; 912( 1):[citado 2024 jul. 26 ] Available from: https://doi.org/10.3847/2041-8213/abf501
  • Source: Journal of Cosmology and Astroparticle Physics (JCAP). Unidade: IF

    Subjects: ASTROFÍSICA, FÍSICA DE PARTÍCULAS, RAIOS CÓSMICOS, MATÉRIA ESCURA

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    • ABNT

      PRIHTIADI, H. et al. Measurement of the cosmic muon annual and diurnal flux variation with the COSINE-100 detector. Journal of Cosmology and Astroparticle Physics (JCAP), v. 2, 2021Tradução . . Disponível em: https://doi.org/10.1088/1475-7516/2021/02/013. Acesso em: 26 jul. 2024.
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      Prihtiadi, H., Carlin Filho, N., França, L. E. F. de M., Manzato, B. B., & Pitta, R. L. C. (2021). Measurement of the cosmic muon annual and diurnal flux variation with the COSINE-100 detector. Journal of Cosmology and Astroparticle Physics (JCAP), 2. doi:10.1088/1475-7516/2021/02/013
    • NLM

      Prihtiadi H, Carlin Filho N, França LEF de M, Manzato BB, Pitta RLC. Measurement of the cosmic muon annual and diurnal flux variation with the COSINE-100 detector [Internet]. Journal of Cosmology and Astroparticle Physics (JCAP). 2021 ; 2[citado 2024 jul. 26 ] Available from: https://doi.org/10.1088/1475-7516/2021/02/013
    • Vancouver

      Prihtiadi H, Carlin Filho N, França LEF de M, Manzato BB, Pitta RLC. Measurement of the cosmic muon annual and diurnal flux variation with the COSINE-100 detector [Internet]. Journal of Cosmology and Astroparticle Physics (JCAP). 2021 ; 2[citado 2024 jul. 26 ] Available from: https://doi.org/10.1088/1475-7516/2021/02/013

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