Galaxy bias from galaxy-galaxy lensing in the DES science verification data (2016)
- Authors:
- Autor USP: LIMA, MARCOS VINICIUS BORGES TEIXEIRA - IF
- Unidade: IF
- Subjects: CLUSTERS; GALÁXIAS; GRAVIDADE
- Language: Inglês
- Imprenta:
-
ABNT
PRAT, J. e LIMA, Marcos Vinicius Borges Teixeira. Galaxy bias from galaxy-galaxy lensing in the DES science verification data. . São Paulo: Instituto de Física, Universidade de São Paulo. Disponível em: https://arxiv.org/pdf/1609.08167.pdf. Acesso em: 18 set. 2024. , 2016 -
APA
Prat, J., & Lima, M. V. B. T. (2016). Galaxy bias from galaxy-galaxy lensing in the DES science verification data. São Paulo: Instituto de Física, Universidade de São Paulo. Recuperado de https://arxiv.org/pdf/1609.08167.pdf -
NLM
Prat J, Lima MVBT. Galaxy bias from galaxy-galaxy lensing in the DES science verification data [Internet]. 2016 ;[citado 2024 set. 18 ] Available from: https://arxiv.org/pdf/1609.08167.pdf -
Vancouver
Prat J, Lima MVBT. Galaxy bias from galaxy-galaxy lensing in the DES science verification data [Internet]. 2016 ;[citado 2024 set. 18 ] Available from: https://arxiv.org/pdf/1609.08167.pdf - A dark energy camera search for missing supergiants in the LMC after the advanced LIGO gravitational wave event GW150914
- BAO from angular clustering: optimization and mitigation of theoretical systematics
- Density split statistics: joint model of counts and lensing in cells
- Quasar accretion disk sizes with continuum reverberation mapping from the dark energy survey
- Dark energy survey year 1 results: galaxy sample for BAO measurement
- Dark energy survey year 1 results: a precise 'H' IND. 0' measurement from DES Y1, BAO, and D/H Data
- Dark energy survey year 1 results: weak lensing shape catalogues
- First cosmological results using type Ia supernovae from the dark energy survey: analysis, systematic uncertainties, and validation
- Quasar accretion disk sizes from continuum reverberation mapping in the DES standard star fields
- The LABOCA/ACT survey of clusters at all redshifts: multi-wavelength analysis of background submillimeter galaxies
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