The VIMOS Public Extragalactic Redshift Survey (VIPERS). Exploring the dependence of the three-point correlation function on stellar mass and luminosity at $0.5 < z < 1.1$
Résumé
Aims. The three-point correlation function (3PCF) is a powerful probe to investigate the clustering of matter in the Universe in a complementary way with respect to lower-order statistics, providing additional information with respect to the two-point correlation function and allowing us to shed light on biasing, non-linear processes, and deviations from Gaussian statistics. In this paper, we analyse the first data release of the VIMOS Public Extragalactic Redshift Survey (VIPERS), determining the dependence of the three-point correlation function on luminosity and stellar mass at z = [ 0.5,1.1 ].Methods. We exploit the VIPERS Public Data Release 1, consisting of more than 50 000 galaxies with B-band magnitudes in the range − 21.6 ≲ MB − 5log (h) ≲ − 19.9 and stellar masses in the range 9.8 ≲ log (M⋆ [ h-2M⊙ ] ) ≲ 10.7. We measure both the connected 3PCF and the reduced 3PCF in redshift space, probing different configurations and scales, in the range 2.5
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https://hal.science/hal-01582680
Soumis le : vendredi 11 mai 2018-14:21:04
Dernière modification le : dimanche 17 mars 2024-17:38:24
Archivage à long terme le : lundi 24 septembre 2018-14:25:13
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Identifiants
- HAL Id : hal-01582680 , version 1
- ARXIV : 1603.08924
- DOI : 10.1051/0004-6361/201628589
- INSPIRE : 1436466
Citer
M. Moresco, F. Marulli, L. Moscardini, E. Branchini, A. Cappi, et al.. The VIMOS Public Extragalactic Redshift Survey (VIPERS). Exploring the dependence of the three-point correlation function on stellar mass and luminosity at $0.5 < z < 1.1$. Astronomy and Astrophysics - A&A, 2017, 604, pp.A133. ⟨10.1051/0004-6361/201628589⟩. ⟨hal-01582680⟩
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