Candidate periodically variable quasars from the Dark Energy Survey and the Sloan Digital Sky Survey (2020)
- Authors:
- USP affiliated authors: LIMA, MARCOS VINICIUS BORGES TEIXEIRA - IF ; SILVA, MICHEL AGUENA DA - IF
- Unidade: IF
- Subjects: COSMOLOGIA; AGLOMERADOS DE GALÁXIAS; QUASARES; BURACOS NEGROS; ONDAS GRAVITACIONAIS
- Agências de fomento:
- Language: Inglês
- Imprenta:
-
ABNT
YU-CHING CHEN, e SILVA, Michel Aguena da e LIMA, Marcos Vinicius Borges Teixeira. Candidate periodically variable quasars from the Dark Energy Survey and the Sloan Digital Sky Survey. . São Paulo: Instituto de Física, Universidade de São Paulo. Disponível em: https://arxiv.org/pdf/2008.12329.pdf. Acesso em: 23 jan. 2026. , 2020 -
APA
Yu-Ching Chen,, Silva, M. A. da, & Lima, M. V. B. T. (2020). Candidate periodically variable quasars from the Dark Energy Survey and the Sloan Digital Sky Survey. São Paulo: Instituto de Física, Universidade de São Paulo. Recuperado de https://arxiv.org/pdf/2008.12329.pdf -
NLM
Yu-Ching Chen, Silva MA da, Lima MVBT. Candidate periodically variable quasars from the Dark Energy Survey and the Sloan Digital Sky Survey [Internet]. 2020 ;[citado 2026 jan. 23 ] Available from: https://arxiv.org/pdf/2008.12329.pdf -
Vancouver
Yu-Ching Chen, Silva MA da, Lima MVBT. Candidate periodically variable quasars from the Dark Energy Survey and the Sloan Digital Sky Survey [Internet]. 2020 ;[citado 2026 jan. 23 ] Available from: https://arxiv.org/pdf/2008.12329.pdf - 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 identification of a low-mass active galactic nucleus at redshift 0.823 from optical variability
- Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing
- 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
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