Dark Energy Survey identification of a low-mass active galactic nucleus at redshift 0.823 from optical variability (2020)
- Authors:
- USP affiliated authors: LIMA, MARCOS VINICIUS BORGES TEIXEIRA - IF ; SILVA, MICHEL AGUENA DA - IF
- Unidade: IF
- DOI: 10.1093/mnras/staa1803
- Assunto: BURACOS NEGROS
- Agências de fomento:
- Language: Inglês
- Imprenta:
- Source:
- Título: Monthly Notices of the Royal Astronomical Society
- Volume/Número/Paginação/Ano: v. 496, Issue 3, p. 3636–3647, 2020
- Este periódico é de acesso aberto
- Este artigo NÃO é de acesso aberto
-
ABNT
GUO, Hengxiao e SILVA, Michel Aguena da e LIMA, Marcos Vinicius Borges Teixeira. Dark Energy Survey identification of a low-mass active galactic nucleus at redshift 0.823 from optical variability. Monthly Notices of the Royal Astronomical Society, v. 496, p. 3636–3647, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/staa1803. Acesso em: 23 jan. 2026. -
APA
Guo, H., Silva, M. A. da, & Lima, M. V. B. T. (2020). Dark Energy Survey identification of a low-mass active galactic nucleus at redshift 0.823 from optical variability. Monthly Notices of the Royal Astronomical Society, 496, 3636–3647. doi:10.1093/mnras/staa1803 -
NLM
Guo H, Silva MA da, Lima MVBT. Dark Energy Survey identification of a low-mass active galactic nucleus at redshift 0.823 from optical variability [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 496 3636–3647.[citado 2026 jan. 23 ] Available from: https://doi.org/10.1093/mnras/staa1803 -
Vancouver
Guo H, Silva MA da, Lima MVBT. Dark Energy Survey identification of a low-mass active galactic nucleus at redshift 0.823 from optical variability [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 496 3636–3647.[citado 2026 jan. 23 ] Available from: https://doi.org/10.1093/mnras/staa1803 - Studying Type II supernovae as cosmological standard candles using the Dark Energy Survey
- Supernova host galaxies in the dark energy survey: I. Deep coadds, photometry, and stellar masses
- Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing
- Candidate periodically variable quasars from the Dark Energy Survey and the Sloan Digital Sky Survey
- Dark energy survey year 3 results: weak lensing shape catalogue
- Probing Galaxy Evolution in Massive Clusters Using ACT and DES: Splashback as a Cosmic Clock
- Pushing automated morphological classifications to their limits with the Dark Energy Survey
- The impact of spectroscopic incompleteness in direct calibration of redshift distributions for weak lensing surveys
- Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertainty
- The mass and galaxy distribution around SZ-selected clusters
Informações sobre o DOI: 10.1093/mnras/staa1803 (Fonte: oaDOI API)
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