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Evolution of clustering length, large-scale bias, and host halo mass at 2 < z < 5 in the VIMOS Ultra Deep Survey (VUDS)
- Source :
- Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, EDP Sciences, 2015, 583, ⟨10.1051/0004-6361/201425343⟩, Astronomy and Astrophysics-A&A, 2015, 583, ⟨10.1051/0004-6361/201425343⟩, NASA Astrophysics Data System
- Publication Year :
- 2015
- Publisher :
- EDP Sciences, 2015.
-
Abstract
- We investigate the evolution of galaxy clustering for galaxies in the redshift range 2.0<br />Comment: 19 pages, 10 figures, submitted to A&A
- Subjects :
- Large-scale structure of Universe
statistical [methods]
Population
Dark matter
Cosmology: observations
Galaxies: evolution
Methods: statistical
Astronomy and Astrophysics
Space and Planetary Science
Astrophysics
Correlation function (astronomy)
01 natural sciences
Cosmology: observation
0103 physical sciences
Cluster analysis
education
010303 astronomy & astrophysics
evolution [galaxies]
Physics
education.field_of_study
010308 nuclear & particles physics
Astronomy and Astrophysic
observations [cosmology]
Redshift
Galaxy
Amplitude
large-scale structure of Universe
Halo
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Astrophysics - Cosmology and Nongalactic Astrophysics
Subjects
Details
- Language :
- English
- ISSN :
- 00046361
- Database :
- OpenAIRE
- Journal :
- Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, EDP Sciences, 2015, 583, ⟨10.1051/0004-6361/201425343⟩, Astronomy and Astrophysics-A&A, 2015, 583, ⟨10.1051/0004-6361/201425343⟩, NASA Astrophysics Data System
- Accession number :
- edsair.doi.dedup.....0442efe1a3c219d6afae03e71fdf8d45