Galaxies in X-ray selected clusters and groups in dark energy survey data. I. Stellar mass growth of bright central galaxies since z ∼ 1.2

Zhang, Y.; Miller, C.; McKay, T.; Evrard, A. E.; Das, R.; Gerdes, D.; Rooney, P.; Romer, A. K.; Bermeo-Hernandez, A.; Perfecto, R.; Song, J.; Desai, S.; Mohr, J.; Hennig, C.; Wilcox, H.; Bacon, D.; Capozzi, D.; Jeltema, T.; Hollowood, D.; others, and

doi:10.3847/0004-637X/816/2/98

Title: Galaxies in X-ray selected clusters and groups in dark energy survey data. I. Stellar mass growth of bright central galaxies since z ∼ 1.2

Journal Article · Sun Jan 10 00:00:00 EST 2016 · Astrophysical Journal

DOI:https://doi.org/10.3847/0004-637X/816/2/98· OSTI ID:22882302

Zhang, Y.; Miller, C.; McKay, T.; Evrard, A. E.; Das, R.; Gerdes, D. ^[1]; Rooney, P.; Romer, A. K.; Bermeo-Hernandez, A. ^[2]; Perfecto, R. ^[3]; Song, J. ^[4]; Desai, S.; Mohr, J.; Hennig, C. ^[5]; Wilcox, H.; Bacon, D.; Capozzi, D. ^[6]; Jeltema, T.; Hollowood, D. ^[7]; others, and

Department of Physics, University of Michigan, Ann Arbor, MI 48109 (United States)
Department of Physics and Astronomy, Pevensey Building, University of Sussex, Brighton, BN1 9QH (United Kingdom)
Department of Astronomy, Yale University, New Haven, CT, 06511-8903 (United States)
Korea Astronomy and Space Science Institute, 776, Daedeokdae-ro,Yuseong-gu, Daejeon, 305-348 (Korea, Republic of)
Department of Physics, Ludwig-Maximilians-Universität, Scheinerstr. 1, D-81679 München (Germany)
Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth, PO1 3FX (United Kingdom)
Department of Physics and Santa Cruz Institute for Particle Physics, University of California, Santa Cruz, CA 95064 (United States)

Using the science verification data of the Dark Energy Survey for a new sample of 106 X-ray selected clusters and groups, we study the stellar mass growth of bright central galaxies (BCGs) since redshift z ∼ 1.2. Compared with the expectation in a semi-analytical model applied to the Millennium Simulation, the observed BCGs become under-massive/under-luminous with decreasing redshift. We incorporate the uncertainties associated with cluster mass, redshift, and BCG stellar mass measurements into an analysis of a redshift-dependent BCG-cluster mass relation, m{sub ∗}∝(((M{sub 200})/(1.5×10{sup 14}M{sub ⊙}))){sup 0.24±0.08}(1+z){sup −0.19±0.34}, and compare the observed relation to the model prediction. We estimate the average growth rate since z = 1.0 for BCGs hosted by clusters of M{sub 200,z} = 10{sup 13.8} M{sub ⊙}; at z = 1.0: m{sub *,BCG} appears to have grown by 0.13 ± 0.11 dex, in tension at the ∼2.5σ significance level with the 0.40 dex growth rate expected from the semi-analytic model. We show that the build-up of extended intracluster light after z = 1.0 may alleviate this tension in BCG growth rates.

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OSTI ID:: 22882302

Journal Information:: Astrophysical Journal, Vol. 816, Issue 2; Other Information: Country of input: International Atomic Energy Agency (IAEA); Since 2009, the country of publication for this journal is the UK.; ISSN 0004-637X

Country of Publication:: United Kingdom

Language:: English

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