Measurement of the splashback feature around SZ-selected galaxy clusters with DES, SPT and ACT (2018)
- Authors:
- Autor USP: LIMA, MARCOS VINICIUS BORGES TEIXEIRA - IF
- Unidade: IF
- Subjects: GALÁXIAS; COSMOLOGIA; ENERGIA ESCURA
- Language: Inglês
- Imprenta:
-
ABNT
SHIN, T. e LIMA, Marcos Vinicius Borges Teixeira. Measurement of the splashback feature around SZ-selected galaxy clusters with DES, SPT and ACT. . São Paulo: Instituto de Física, Universidade de São Paulo. Disponível em: https://arxiv.org/abs/1811.06081. Acesso em: 16 abr. 2024. , 2018 -
APA
Shin, T., & Lima, M. V. B. T. (2018). Measurement of the splashback feature around SZ-selected galaxy clusters with DES, SPT and ACT. São Paulo: Instituto de Física, Universidade de São Paulo. Recuperado de https://arxiv.org/abs/1811.06081 -
NLM
Shin T, Lima MVBT. Measurement of the splashback feature around SZ-selected galaxy clusters with DES, SPT and ACT [Internet]. 2018 ;[citado 2024 abr. 16 ] Available from: https://arxiv.org/abs/1811.06081 -
Vancouver
Shin T, Lima MVBT. Measurement of the splashback feature around SZ-selected galaxy clusters with DES, SPT and ACT [Internet]. 2018 ;[citado 2024 abr. 16 ] Available from: https://arxiv.org/abs/1811.06081 - Discovery of two gravitationally lensed quasars in the dark energy survey
- Optical-SZE scaling relations for DES optically selected clusters within the SPT-SZ survey
- Structure formation and cosmic acceleration
- Galaxy bias from the Dark Energy Survey Science verification data: combining galaxy density maps and weak lensing maps
- The Dark Energy Survey: more than dark energy - an overview
- The thirteenth data release of the sloan digital sky survey: first spectroscopic data from the SDSS-IV survey mapping nearby galaxies at apache point observatory
- A Search for kilonovae in the dark energy survey
- Weak lensing magnification in the dark energy survey science verification data
- The electromagnetic counterpart of the binary neutron star merger LIGO/VIRGO GW170817. I. discovery of the optical counterpart using the dark energy camera
- Dark energy survey year 1 results: cross-correlation redshifts in the DES - calibration of the weak lensing source redshift distributions
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