Measuring subhalo mass in redMaPPer clusters with CFHT Stripe 82 Survey
Abstract
Here, we use the shear catalogue from the CFHT Stripe-82 Survey to measure the subhalo masses of satellite galaxies in redMaPPer clusters. Assuming a Chabrier initial mass function and a truncated NFW model for the subhalo mass distribution, we find that the subhalo mass to galaxy stellar mass ratio increases as a function of projected halo-centric radius rp, from Msub/Mstar = 4.43+6.63–2.23 at rp ε [0.1, 0.3] h–1 Mpc to Msub/Mstar = 75.40+19.73–19.09 at rp ε [0.6, 0.9] h–1 Mpc. We also investigate the dependence of subhalo masses on stellar mass by splitting satellite galaxies into two stellar mass bins: 10 < log (Mstar/h–1M⊙) < 10.5 and 11 < log (Mstar/h–1 M⊙) < 12. The best-fitting subhalo mass of the more massive satellite galaxy bin is larger than that of the less massive satellites: log(Msub/h–1M⊙) = 11.14+0.66–0.73 (Msub/Mstar = 19.5+19.8–17.9) versus log(Msub/h–1M⊙) = 12.38+0.16–0.16 (Msub/Mstar = 21.1+7.4–7.7).
- Authors:
-
- Chinese Academy of Sciences (CAS), Beijing (China)
- Ecole Polytechnique Federale de Lausanne (EPFL), Versoix (Switzerland)
- Ecole Polytechnique Federale de Lausanne (EPFL), Versoix (Switzerland); Aix-Marseille Univ., and CNRS, LAM, Marseille (France)
- Univ. of Massachusetts, Amherst, MA (United States)
- Univ. of Arizona, Tucson, AZ (United States)
- The Univ. of Tokyo, Chiba (Japan)
- Siena College, Loudonville, KY (United States)
- INAF, Astronomical Observatory of Trieste, Trieste (Italy)
- Argelander-Institut fur Astronomie Auf dem Hugel, Bonn (Germany)
- Univ. of British Columbia, Vancouver (Canada)
- Centro Brasileiro de Pesquisas Fisicas, Rio de Janeiro (Brazil)
- SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Univ. College London, London (United Kingdom); Ministry of Education of Brazil (Brazil)
- Publication Date:
- Research Org.:
- SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC)
- OSTI Identifier:
- 1256640
- Report Number(s):
- SLAC-PUB-16550
Journal ID: ISSN 0035-8711; arXiv:1507.01464
- Grant/Contract Number:
- AC02-76SF00515
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Volume: 458; Journal Issue: 3; Journal ID: ISSN 0035-8711
- Publisher:
- Royal Astronomical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS
Citation Formats
Li, Ran, Shan, Huanyuan, Kneib, Jean -Paul, Mo, Houjun, Rozo, Eduardo, Leauthaud, Alexie, Moustakas, John, Xie, Lizhi, Erben, Thomas, Van Waerbeke, Ludovic, Makler, Martin, Rykoff, Eli, and Moraes, Bruno. Measuring subhalo mass in redMaPPer clusters with CFHT Stripe 82 Survey. United States: N. p., 2016.
Web. doi:10.1093/mnras/stw494.
Li, Ran, Shan, Huanyuan, Kneib, Jean -Paul, Mo, Houjun, Rozo, Eduardo, Leauthaud, Alexie, Moustakas, John, Xie, Lizhi, Erben, Thomas, Van Waerbeke, Ludovic, Makler, Martin, Rykoff, Eli, & Moraes, Bruno. Measuring subhalo mass in redMaPPer clusters with CFHT Stripe 82 Survey. United States. https://doi.org/10.1093/mnras/stw494
Li, Ran, Shan, Huanyuan, Kneib, Jean -Paul, Mo, Houjun, Rozo, Eduardo, Leauthaud, Alexie, Moustakas, John, Xie, Lizhi, Erben, Thomas, Van Waerbeke, Ludovic, Makler, Martin, Rykoff, Eli, and Moraes, Bruno. Mon .
"Measuring subhalo mass in redMaPPer clusters with CFHT Stripe 82 Survey". United States. https://doi.org/10.1093/mnras/stw494. https://www.osti.gov/servlets/purl/1256640.
@article{osti_1256640,
title = {Measuring subhalo mass in redMaPPer clusters with CFHT Stripe 82 Survey},
author = {Li, Ran and Shan, Huanyuan and Kneib, Jean -Paul and Mo, Houjun and Rozo, Eduardo and Leauthaud, Alexie and Moustakas, John and Xie, Lizhi and Erben, Thomas and Van Waerbeke, Ludovic and Makler, Martin and Rykoff, Eli and Moraes, Bruno},
abstractNote = {Here, we use the shear catalogue from the CFHT Stripe-82 Survey to measure the subhalo masses of satellite galaxies in redMaPPer clusters. Assuming a Chabrier initial mass function and a truncated NFW model for the subhalo mass distribution, we find that the subhalo mass to galaxy stellar mass ratio increases as a function of projected halo-centric radius rp, from Msub/Mstar = 4.43+6.63–2.23 at rp ε [0.1, 0.3] h–1 Mpc to Msub/Mstar = 75.40+19.73–19.09 at rp ε [0.6, 0.9] h–1 Mpc. We also investigate the dependence of subhalo masses on stellar mass by splitting satellite galaxies into two stellar mass bins: 10 < log (Mstar/h–1M⊙) < 10.5 and 11 < log (Mstar/h–1 M⊙) < 12. The best-fitting subhalo mass of the more massive satellite galaxy bin is larger than that of the less massive satellites: log(Msub/h–1M⊙) = 11.14+0.66–0.73 (Msub/Mstar = 19.5+19.8–17.9) versus log(Msub/h–1M⊙) = 12.38+0.16–0.16 (Msub/Mstar = 21.1+7.4–7.7).},
doi = {10.1093/mnras/stw494},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 3,
volume = 458,
place = {United States},
year = {Mon Mar 07 00:00:00 EST 2016},
month = {Mon Mar 07 00:00:00 EST 2016}
}
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