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 do periódico: Physical Review D
- Volume/Número/Paginação/Ano: v. 105, 023515, 2022
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: hybrid
- Licença: publisher-specific-oa
-
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: 30 abr. 2024. -
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 2024 abr. 30 ] 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 2024 abr. 30 ] Available from: https://doi.org/10.1103/PhysRevD.105.023515 - Constraints on the Physical Properties of GW190814 through Simulations Based on DECam Follow-up Observations by the Dark Energy Survey
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Informações sobre o DOI: 10.1103/PhysRevD.105.023515 (Fonte: oaDOI API)
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