A measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic sunyaev-zel’dovich effect with SPT-3G and DES (2022)
- Authors:
- Autor USP: LIMA, MARCOS VINICIUS BORGES TEIXEIRA - IF
- Unidade: IF
- Subjects: AGLOMERADOS DE GALÁXIAS; ASTROFÍSICA
- Keywords: ENERGIA ESCURA
- Language: Inglês
- Imprenta:
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ABNT
SCHIAPPUCCI, E. e LIMA, Marcos Vinicius Borges Teixeira. A measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic sunyaev-zel’dovich effect with SPT-3G and DES. . São Paulo: Instituto de Física, Universidade de São Paulo. Disponível em: https://arxiv.org/pdf/2207.11937.pdf. Acesso em: 07 fev. 2026. , 2022 -
APA
Schiappucci, E., & Lima, M. V. B. T. (2022). A measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic sunyaev-zel’dovich effect with SPT-3G and DES. São Paulo: Instituto de Física, Universidade de São Paulo. Recuperado de https://arxiv.org/pdf/2207.11937.pdf -
NLM
Schiappucci E, Lima MVBT. A measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic sunyaev-zel’dovich effect with SPT-3G and DES [Internet]. 2022 ;[citado 2026 fev. 07 ] Available from: https://arxiv.org/pdf/2207.11937.pdf -
Vancouver
Schiappucci E, Lima MVBT. A measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic sunyaev-zel’dovich effect with SPT-3G and DES [Internet]. 2022 ;[citado 2026 fev. 07 ] Available from: https://arxiv.org/pdf/2207.11937.pdf - Is every strong lens model unhappy in its own way?: uniform modelling of a sample of 13 quadruply+ imaged quasars
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