The VIMOS Public Extragalactic Redshift Survey (VIPERS). Exploring the dependence of the three-point correlation function on stellar mass and luminosity at $0.5 < z < 1.1$
- Creators
- Moresco, M.
- Marulli, F.
- Moscardini, L.
- Branchini, E.
- Cappi, A.
- Davidzon, I.
- Granett, B.R.
- de La Torre, S.
- Guzzo, L.
- Abbas, U.
- Adami, C.
- Arnouts, S.
- Bel, J.
- Bolzonella, M.
- Bottini, D.
- Coupon, J.
- Cucciati, O.
- de Lucia, G.
- Franzetti, P.
- Fritz, A.
- Fumana, M.
- Garilli, B.
- Ilbert, O.
- Iovino, A.
- Krywult, J.
- Le Brun, V.
- Fèvre, O. Le
- Małek, K.
- Mccracken, H.J.
- Polletta, M.
- Pollo, A.
- Scodeggio, M.
- Tasca, L.A.M.
- Tojeiro, R.
- Vergani, D.
- Zanichelli, A.
- Others:
- Joseph Louis LAGRANGE (LAGRANGE) ; Université Nice Sophia Antipolis (1965 - 2019) (UNS) ; COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur ; COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)
- Laboratoire d'Astrophysique de Marseille (LAM) ; Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
- Centre de Physique Théorique - UMR 7332 (CPT) ; Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS)
- Université de Toulon (UTLN)
- Institut d'Astrophysique de Paris (IAP) ; Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
Description
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
Abstract
International audience
Additional details
- URL
- https://hal.archives-ouvertes.fr/hal-01582680
- URN
- urn:oai:HAL:hal-01582680v1
- Origin repository
- UNICA