Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertainty (2022)
- Authors:
- USP affiliated authors: LIMA, MARCOS VINICIUS BORGES TEIXEIRA - IF ; SILVA, MICHEL AGUENA DA - IF
- Unidade: IF
- DOI: 10.1103/PhysRevD.105.023515
- Assunto: COSMOLOGIA
- Agências de fomento:
- Language: Inglês
- Imprenta:
- Publisher: American Physical Society
- Publisher place: New York
- Date published: 2022
- Source:
- Título: Physical Review D
- Volume/Número/Paginação/Ano: v. 105, 023515, 2022
- Este periódico é de acesso aberto
- Este artigo NÃO é de acesso aberto
-
ABNT
SECCO, L F e AGUENA, Michel e LIMA, Marcos Vinicius Borges Teixeira. Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertainty. Physical Review D, v. 105, 2022Tradução . . Disponível em: https://doi.org/10.1103/PhysRevD.105.023515. Acesso em: 23 jan. 2026. -
APA
Secco, L. F., Aguena, M., & Lima, M. V. B. T. (2022). Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertainty. Physical Review D, 105. doi:10.1103/PhysRevD.105.023515 -
NLM
Secco LF, Aguena M, Lima MVBT. Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertainty [Internet]. Physical Review D. 2022 ; 105[citado 2026 jan. 23 ] Available from: https://doi.org/10.1103/PhysRevD.105.023515 -
Vancouver
Secco LF, Aguena M, Lima MVBT. Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertainty [Internet]. Physical Review D. 2022 ; 105[citado 2026 jan. 23 ] Available from: https://doi.org/10.1103/PhysRevD.105.023515 - Studying Type II supernovae as cosmological standard candles using the Dark Energy Survey
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- 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
- 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
- The mass and galaxy distribution around SZ-selected clusters
Informações sobre o DOI: 10.1103/PhysRevD.105.023515 (Fonte: oaDOI API)
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