Dark energy survey year 1 results: galaxy clustering for combined probes (2017)
- Autores:
- Autor USP: LIMA, MARCOS VINICIUS BORGES TEIXEIRA - IF
- Unidade: IF
- Assuntos: GALÁXIAS; COSMOLOGIA; ENERGIA ESCURA
- Idioma: Inglês
- Imprenta:
-
ABNT
ELVIN-POOLE, J. e LIMA, Marcos Vinicius Borges Teixeira. Dark energy survey year 1 results: galaxy clustering for combined probes. . São Paulo: Instituto de Física, Universidade de São Paulo. Disponível em: https://arxiv.org/abs/1708.01536. Acesso em: 19 abr. 2024. , 2017 -
APA
Elvin-Poole, J., & Lima, M. V. B. T. (2017). Dark energy survey year 1 results: galaxy clustering for combined probes. São Paulo: Instituto de Física, Universidade de São Paulo. Recuperado de https://arxiv.org/abs/1708.01536 -
NLM
Elvin-Poole J, Lima MVBT. Dark energy survey year 1 results: galaxy clustering for combined probes [Internet]. 2017 ;[citado 2024 abr. 19 ] Available from: https://arxiv.org/abs/1708.01536 -
Vancouver
Elvin-Poole J, Lima MVBT. Dark energy survey year 1 results: galaxy clustering for combined probes [Internet]. 2017 ;[citado 2024 abr. 19 ] Available from: https://arxiv.org/abs/1708.01536 - 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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