Stellar-to-halo mass relation of cluster galaxies

Niemiec, Anna; Jullo, Eric; Limousin, Marceau; Giocoli, Carlo; Erben, Thomas; Hildebrant, Hendrik; Kneib, Jean-Paul; Leauthaud, Alexie; Makler, Martin; Moraes, Bruno; Pereira, Maria E.  S.; Shan, Huanyuan; Rozo, Eduardo; Rykoff, Eli; Van Waerbeke, Ludovic

doi:10.1093/mnras/stx1667

Title: Stellar-to-halo mass relation of cluster galaxies

Journal Article · Tue Jul 04 00:00:00 EDT 2017 · Monthly Notices of the Royal Astronomical Society

DOI:https://doi.org/10.1093/mnras/stx1667· OSTI ID:1390599

Niemiec, Anna ^[1]; Jullo, Eric ^[1]; Limousin, Marceau ^[1];

^[2]; Erben, Thomas ^[3]; Hildebrant, Hendrik ^[3]; Kneib, Jean-Paul ^[4]; Leauthaud, Alexie ^[5]; Makler, Martin ^[6]; Moraes, Bruno ^[7]; Pereira, Maria E. S. ^[6]; Shan, Huanyuan ^[8]; Rozo, Eduardo ^[9]; Rykoff, Eli ^[10]; Van Waerbeke, Ludovic ^[11]

Aix-Marseille Univ., and CNRS/IN2P3, Marseille (France)
Aix-Marseille Univ., and CNRS/IN2P3, Marseille (France); Alma Mater Studorium Univ. di Bologna (Italy)
Argelander Inst. for Astronomy, Bonn (Germany)
Ecole Polytechnique Federale Lausanne (Switzlerland)
Univ. of California, Santa Cruz, CA (United States)
Ministerio da Ciencia, Tecnologia e Inovacao (MCTI), Rio de Janiero (Brazil). Centro Brasileiro de Pesquisas Fisicas (CBPF)
Univ. College London (United Kingdom)
Argelander Inst. for Astronomy, Bonn (Germany); Ecole Polytechnique Federale Lausanne (Switzlerland)
Univ. of Arizona, Tucson, AZ (United States)
SLAC National Accelerator Lab., Menlo Park, CA (United States)
Univ. of British Columbia, Vancouver, BC (Canada)

In the formation of galaxy groups and clusters, the dark matter haloes containing satellite galaxies are expected to be tidally stripped in gravitational interactions with the host. We use galaxy-galaxy weak lensing to measure the average mass of dark matter haloes of satellite galaxies as a function of projected distance to the centre of the host, since stripping is expected to be greater for satellites closer to the centre of the cluster. We further classify the satellites according to their stellar mass: assuming that the stellar component of the galaxy is less disrupted by tidal stripping, stellar mass can be used as a proxy of the infall mass. We study the stellar to halo mass relation of satellites as a function of the cluster-centric distance to measure tidal stripping. We use the shear catalogues of the DES science veri cation archive, the CFHTLenS and the CFHT Stripe 82 surveys, and we select satellites from the redMaPPer catalogue of clusters. For galaxies located in the outskirts of clusters, we nd a stellar to halo mass relation in good agreement with the theoretical expectations from Moster, Naab & White (2013) for central galaxies. In the centre of the cluster, we nd that this relation is shifted to smaller halo mass for a given stellar mass. We interpret this nding as further evidence for tidal stripping of dark matter haloes in high density environments.

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Research Organization:: SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)

Sponsoring Organization:: USDOE

Grant/Contract Number:: AC02-76SF00515; Hi 1495/2-1

OSTI ID:: 1390599

Journal Information:: Monthly Notices of the Royal Astronomical Society, Vol. 471, Issue 1; ISSN 0035-8711

Publisher:: Royal Astronomical SocietyCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 24 works

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