Dark energy survey year 1 results: galaxy sample for BAO measurement (2017)
- Authors:
- Autor USP: LIMA, MARCOS VINICIUS BORGES TEIXEIRA - IF
- Unidade: IF
- Subjects: GALÁXIAS; COSMOLOGIA; ENERGIA ESCURA
- Language: Inglês
- Imprenta:
-
ABNT
CROCCE, M. e LIMA, Marcos Vinicius Borges Teixeira. Dark energy survey year 1 results: galaxy sample for BAO measurement. . São Paulo: Instituto de Física, Universidade de São Paulo. Disponível em: https://arxiv.org/abs/1712.06211. Acesso em: 27 dez. 2025. , 2017 -
APA
Crocce, M., & Lima, M. V. B. T. (2017). Dark energy survey year 1 results: galaxy sample for BAO measurement. São Paulo: Instituto de Física, Universidade de São Paulo. Recuperado de https://arxiv.org/abs/1712.06211 -
NLM
Crocce M, Lima MVBT. Dark energy survey year 1 results: galaxy sample for BAO measurement [Internet]. 2017 ;[citado 2025 dez. 27 ] Available from: https://arxiv.org/abs/1712.06211 -
Vancouver
Crocce M, Lima MVBT. Dark energy survey year 1 results: galaxy sample for BAO measurement [Internet]. 2017 ;[citado 2025 dez. 27 ] Available from: https://arxiv.org/abs/1712.06211 - First cosmology results using type Ia supernovae from the dark energy survey: photometric pipeline and light curve data release
- First cosmology results using type Ia supernova from the dark energy survey: simulations to correct supernova distance biases
- Galaxies in x-ray selected clusters and groups in dark energy survey data II: hierarchical bayesian modeling of the red-sequence galaxy luminosity function
- First cosmology results using type Ia supernovae from the dark energy survey: constraints on cosmological parameters
- Stellar mass as a galaxy cluster mass proxy: application to the dark energy survey redMaPPer clusters
- Dark energy survey year 1 results: constraints on intrinsic alignments and their colour dependence from galaxy clustering and weak lensing
- A search for optical emission from binary-black-hole merger GW170814 with the dark energy camera
- Is every strong lens model unhappy in its own way?: uniform modelling of a sample of 13 quadruply+ imaged quasars
- Spectral variability of a sample of extreme variability quasars and implications for the 'MG' IND. II' broad-line region
- Three new VHS-DES quasars at 6.7 < z < 6.9 and emission line properties at z > 6:5
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
