Candidate massive galaxies at z∼4 in the dark energy survey (2018)
- Authors:
- Autor USP: LIMA, MARCOS VINICIUS BORGES TEIXEIRA - IF
- Unidade: IF
- Subjects: GALÁXIAS; COSMOLOGIA; ENERGIA ESCURA
- Language: Inglês
- Imprenta:
-
ABNT
GUARNIERI, Pierandrea e LIMA, Marcos Vinicius Borges Teixeira. Candidate massive galaxies at z∼4 in the dark energy survey. . São Paulo: Instituto de Física, Universidade de São Paulo. Disponível em: https://arxiv.org/abs/1811.12422. Acesso em: 13 maio 2024. , 2018 -
APA
Guarnieri, P., & Lima, M. V. B. T. (2018). Candidate massive galaxies at z∼4 in the dark energy survey. São Paulo: Instituto de Física, Universidade de São Paulo. Recuperado de https://arxiv.org/abs/1811.12422 -
NLM
Guarnieri P, Lima MVBT. Candidate massive galaxies at z∼4 in the dark energy survey [Internet]. 2018 ;[citado 2024 maio 13 ] Available from: https://arxiv.org/abs/1811.12422 -
Vancouver
Guarnieri P, Lima MVBT. Candidate massive galaxies at z∼4 in the dark energy survey [Internet]. 2018 ;[citado 2024 maio 13 ] Available from: https://arxiv.org/abs/1811.12422 - First cosmological results using type Ia supernovae from the dark energy survey: effects of chromatic corrections to supernova photometry on measurements of cosmological parameters
- First cosmological results using type Ia supernovae from the dark energy survey: simulations to correct supernova distance biases
- Dark energy survey year 1 results: validation of weak lensing cluster member contamination estimates from P(z) decomposition
- Dark Energy Survey Year 1 results: detection of intra-cluster light at redshift ∼ 0.25
- First cosmological results using type Ia supernovae from the dark energy survey: measurement of the hubble constant
- Cosmological lensing ratios with DES Y1, SPT and planck
- Dark energy survey year 1 results: tomographic cross-correlations between DES galaxies and CMB lensing from SPT+planck
- UV-luminous, star-forming hosts of z~2 reddened quasars in the dark energy survey
- Dark energy survey year 1 results: measurement of the galaxy angular power spectrum
- Dark energy survey year 1 results: weak lensing mass calibration of redMaPPer galaxy clusters
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