Measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel’dovich effect with SPT-3G and DES (2023)
- Authors:
- Autor USP: LIMA, MARCOS VINICIUS BORGES TEIXEIRA - IF
- Unidade: IF
- DOI: 10.1103/PhysRevD.107.042004
- Subjects: COSMOLOGIA; GALÁXIAS
- Agências de fomento:
- Language: Inglês
- Imprenta:
- Publisher: American Physical Society
- Publisher place: New York
- Date published: 2023
- Source:
- Título do periódico: Physical Review D
- Volume/Número/Paginação/Ano: v. 107, 042004, 2023
- 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
SCHIAPPUCCI, E e LIMA, Marcos Vinicius Borges Teixeira. Measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel’dovich effect with SPT-3G and DES. Physical Review D, v. 107, 2023Tradução . . Disponível em: https://doi.org/10.1103/PhysRevD.107.042004. Acesso em: 11 jun. 2024. -
APA
Schiappucci, E., & Lima, M. V. B. T. (2023). Measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel’dovich effect with SPT-3G and DES. Physical Review D, 107. doi:10.1103/PhysRevD.107.042004 -
NLM
Schiappucci E, Lima MVBT. Measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel’dovich effect with SPT-3G and DES [Internet]. Physical Review D. 2023 ; 107[citado 2024 jun. 11 ] Available from: https://doi.org/10.1103/PhysRevD.107.042004 -
Vancouver
Schiappucci E, Lima MVBT. Measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel’dovich effect with SPT-3G and DES [Internet]. Physical Review D. 2023 ; 107[citado 2024 jun. 11 ] Available from: https://doi.org/10.1103/PhysRevD.107.042004 - Measuring cosmological parameters with type IA supernovae in redmagic galaxie
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- The STRong lensing insights into the dark energy survey (STRIDES) 2016 follow-up campaign. II.: new quasar lenses from double component fitting.
- Survey geometry and the internal consistency of recent cosmic shear measurements
- Star-galaxy classi cation in the dark energy survey Y1 dataset
Informações sobre o DOI: 10.1103/PhysRevD.107.042004 (Fonte: oaDOI API)
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