%0 Generic %1 gillis2013cfhtlens %A Gillis, Bryan R. %A Hudson, Michael J. %A Erben, Thomas %A Heymans, Catherine %A Hildebrandt, Hendrik %A Hoekstra, Henk %A Kitching, Thomas D. %A Mellier, Yannick %A Miller, Lance %A van Waerbeke, Ludovic %A Bonnett, Christopher %A Coupon, Jean %A Fu, Liping %A Hilbert, Stefan %A Rowe, Barnaby T. P. %A Schrabback, Tim %A Semboloni, Elisabetta %A van Uitert, Edo %A Velander, Malin %D 2013 %K centrals lensing satellites weak %T CFHTLenS: The Environmental Dependence of Galaxy Halo Masses from Weak Lensing %U http://arxiv.org/abs/1301.7421 %X We use weak gravitational lensing to analyse the dark matter halos around satellite galaxies in galaxy groups in the CFHTLenS dataset. This dataset is derived from the CFHTLS-Wide survey, and encompasses 154 sq. deg of high-quality shape data. Using the photometric redshifts, we divide the sample of lens galaxies with stellar masses in the range 10^9 Msun to 10^10.5 Msun into those likely to lie in high-density environments (HDE) and those likely to lie in low-density environments (LDE). Through comparison with galaxy catalogues extracted from the Millennium Simulation, we show that the sample of HDE galaxies should primarily (~61%) consist of satellite galaxies in groups, while the sample of LDE galaxies should consist of mostly (~87%) non-satellite (field and central) galaxies. Comparing the lensing signals around samples of HDE and LDE galaxies matched in stellar mass, the lensing signal around HDE galaxies clearly shows a positive contribution from their host groups on their lensing signals at radii of ~500--1000 kpc, the typical separation between satellites and group centres. More importantly, the subhalos of HDE galaxies are less massive than those around LDE galaxies by a factor 0.65 +/- 0.12, significant at the 2.9 sigma level. A natural explanation is that the halos of satellite galaxies are stripped through tidal effects in the group environment. Our results are consistent with a typical tidal truncation radius of ~40 kpc.

@misc{gillis2013cfhtlens, abstract = {We use weak gravitational lensing to analyse the dark matter halos around satellite galaxies in galaxy groups in the CFHTLenS dataset. This dataset is derived from the CFHTLS-Wide survey, and encompasses 154 sq. deg of high-quality shape data. Using the photometric redshifts, we divide the sample of lens galaxies with stellar masses in the range 10^9 Msun to 10^10.5 Msun into those likely to lie in high-density environments (HDE) and those likely to lie in low-density environments (LDE). Through comparison with galaxy catalogues extracted from the Millennium Simulation, we show that the sample of HDE galaxies should primarily (~61%) consist of satellite galaxies in groups, while the sample of LDE galaxies should consist of mostly (~87%) non-satellite (field and central) galaxies. Comparing the lensing signals around samples of HDE and LDE galaxies matched in stellar mass, the lensing signal around HDE galaxies clearly shows a positive contribution from their host groups on their lensing signals at radii of ~500--1000 kpc, the typical separation between satellites and group centres. More importantly, the subhalos of HDE galaxies are less massive than those around LDE galaxies by a factor 0.65 +/- 0.12, significant at the 2.9 sigma level. A natural explanation is that the halos of satellite galaxies are stripped through tidal effects in the group environment. Our results are consistent with a typical tidal truncation radius of ~40 kpc.}, added-at = {2013-02-01T16:30:03.000+0100}, author = {Gillis, Bryan R. and Hudson, Michael J. and Erben, Thomas and Heymans, Catherine and Hildebrandt, Hendrik and Hoekstra, Henk and Kitching, Thomas D. and Mellier, Yannick and Miller, Lance and van Waerbeke, Ludovic and Bonnett, Christopher and Coupon, Jean and Fu, Liping and Hilbert, Stefan and Rowe, Barnaby T. P. and Schrabback, Tim and Semboloni, Elisabetta and van Uitert, Edo and Velander, Malin}, biburl = {https://www.bibsonomy.org/bibtex/231c64c0860bc12fed57d907e9ef92d4d/miki}, description = {[1301.7421] CFHTLenS: The Environmental Dependence of Galaxy Halo Masses from Weak Lensing}, interhash = {1e033cc84b890c600592baba1361eca9}, intrahash = {31c64c0860bc12fed57d907e9ef92d4d}, keywords = {centrals lensing satellites weak}, note = {cite arxiv:1301.7421Comment: Submitted to MNRAS. 14 pages, 9 figures, 5 tables}, timestamp = {2013-02-01T16:30:03.000+0100}, title = {CFHTLenS: The Environmental Dependence of Galaxy Halo Masses from Weak Lensing}, url = {http://arxiv.org/abs/1301.7421}, year = 2013 }