First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Photometric Pipeline and Light-curve Data Release (2019)
- Authors:
- Autor USP: LIMA, MARCOS VINICIUS BORGES TEIXEIRA - IF
- Unidade: IF
- DOI: 10.3847/1538-4357/ab06c1
- Subjects: COSMOLOGIA; MATÉRIA ESCURA; SUPERNOVAS
- Keywords: COSMOLOGY; OBSERVATIONS - SUPERNOVAE; GENERAL – TECHNIQUES: PHOTOMETRIC
- Agências de fomento:
- Language: Inglês
- Imprenta:
- Source:
- Título: The Astrophysical Journal
- ISSN: 2041-8213
- Volume/Número/Paginação/Ano: v. 874, n. 1, March, p. 106/1-106/12, 2019
- Este artigo possui versão em acesso aberto
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- PDF de acesso aberto
- Versão do Documento: Versão publicada (Published version)
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Status: Artigo possui acesso gratuito no site do editor (Bronze Open Access) -
ABNT
BROUT, D e LIMA, Marcos Vinicius Borges Teixeira. First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Photometric Pipeline and Light-curve Data Release. The Astrophysical Journal, v. 874, n. 1, p. 106/1-106/12, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab06c1. Acesso em: 12 mar. 2026. -
APA
Brout, D., & Lima, M. V. B. T. (2019). First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Photometric Pipeline and Light-curve Data Release. The Astrophysical Journal, 874( 1), 106/1-106/12. doi:10.3847/1538-4357/ab06c1 -
NLM
Brout D, Lima MVBT. First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Photometric Pipeline and Light-curve Data Release [Internet]. The Astrophysical Journal. 2019 ; 874( 1): 106/1-106/12.[citado 2026 mar. 12 ] Available from: https://doi.org/10.3847/1538-4357/ab06c1 -
Vancouver
Brout D, Lima MVBT. First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Photometric Pipeline and Light-curve Data Release [Internet]. The Astrophysical Journal. 2019 ; 874( 1): 106/1-106/12.[citado 2026 mar. 12 ] Available from: https://doi.org/10.3847/1538-4357/ab06c1 - Is every strong lens model unhappy in its own way?: uniform modelling of a sample of 13 quadruply+ imaged quasars
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