Galaxies in X-ray Selected Clusters and Groups in Dark Energy Survey Data: Stellar Mass Growth of Bright Central Galaxies Since z~1.2

Here, 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 Millenniu...

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Published in:The Astrophysical journal 2016-01, Vol.816 (2)
Main Authors: Zhang, Y., Miller, C., McKay, T., Rooney, P., Evrard, A. E., Romer, A. K., Perfecto, R., Song, J., Desai, S., Mohr, J., Wilcox, H., Bermeo-Hernandez, A., Jeltema, T., Hollowood, D., Bacon, D., Capozzi, D., Collins, C., Das, R., Gerdes, D., Hennig, C., Hilton, M., Hoyle, B., Kay, S., Liddle, A., Mann, R. G., Mehrtens, N., Nichol, R. C., Papovich, C., Sahlén, M., Soares-Santos, M., Stott, J., Viana, P. T., Abbott, T., Abdalla, F. B., Banerji, M., Bauer, A. H., Benoit-Lévy, A., Bertin, E., Brooks, D., Buckley-Geer, E., Burke, D. L., Rosell, A. Carnero, Castander, F. J., Diehl, H. T., Doel, P., Cunha, C. E., Eifler, T. F., Neto, A. Fausti, Fernandez, E., Flaugher, B., Fosalba, P., Frieman, J., Gaztanaga, E., Gruen, D., Gruendl, R. A., Honscheid, K., James, D., Kuehn, K., Kuropatkin, N., Lahav, O., Maia, M. A. G., Makler, M., Marshall, J. L., Martini, Paul, Miquel, R., Ogando, R., Plazas, A. A., Roodman, A., Rykoff, E. S., Sako, M., Sanchez, E., Scarpine, V., Schubnell, M., Sevilla, I., Smith, R. C., Sobreira, F., Suchyta, E., Swanson, M. E. C., Tarle, G., Thaler, J., Tucker, D., Vikram, V., Costa, L. N. da
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Language:English
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ASTRONOMY AND ASTROPHYSICS
galaxies: clusters: general
galaxies: evolution
galaxies: groups: general
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container_title The Astrophysical journal
container_volume 816
creator Zhang, Y.
Miller, C.
McKay, T.
Rooney, P.
Evrard, A. E.
Romer, A. K.
Perfecto, R.
Song, J.
Desai, S.
Mohr, J.
Wilcox, H.
Bermeo-Hernandez, A.
Jeltema, T.
Hollowood, D.
Bacon, D.
Capozzi, D.
Collins, C.
Das, R.
Gerdes, D.
Hennig, C.
Hilton, M.
Hoyle, B.
Kay, S.
Liddle, A.
Mann, R. G.
Mehrtens, N.
Nichol, R. C.
Papovich, C.
Sahlén, M.
Soares-Santos, M.
Stott, J.
Viana, P. T.
Abbott, T.
Abdalla, F. B.
Banerji, M.
Bauer, A. H.
Benoit-Lévy, A.
Bertin, E.
Brooks, D.
Buckley-Geer, E.
Burke, D. L.
Rosell, A. Carnero
Castander, F. J.
Diehl, H. T.
Doel, P.
Cunha, C. E.
Eifler, T. F.
Neto, A. Fausti
Fernandez, E.
Flaugher, B.
Fosalba, P.
Frieman, J.
Gaztanaga, E.
Gruen, D.
Gruendl, R. A.
Honscheid, K.
James, D.
Kuehn, K.
Kuropatkin, N.
Lahav, O.
Maia, M. A. G.
Makler, M.
Marshall, J. L.
Martini, Paul
Miquel, R.
Ogando, R.
Plazas, A. A.
Roodman, A.
Rykoff, E. S.
Sako, M.
Sanchez, E.
Scarpine, V.
Schubnell, M.
Sevilla, I.
Smith, R. C.
Sobreira, F.
Suchyta, E.
Swanson, M. E. C.
Tarle, G.
Thaler, J.
Tucker, D.
Vikram, V.
Costa, L. N. da
description Here, 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.
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S.</creatorcontrib><creatorcontrib>Sako, M.</creatorcontrib><creatorcontrib>Sanchez, E.</creatorcontrib><creatorcontrib>Scarpine, V.</creatorcontrib><creatorcontrib>Schubnell, M.</creatorcontrib><creatorcontrib>Sevilla, I.</creatorcontrib><creatorcontrib>Smith, R. C.</creatorcontrib><creatorcontrib>Sobreira, F.</creatorcontrib><creatorcontrib>Suchyta, E.</creatorcontrib><creatorcontrib>Swanson, M. E. C.</creatorcontrib><creatorcontrib>Tarle, G.</creatorcontrib><creatorcontrib>Thaler, J.</creatorcontrib><creatorcontrib>Tucker, D.</creatorcontrib><creatorcontrib>Vikram, V.</creatorcontrib><creatorcontrib>Costa, L. N. da</creatorcontrib><creatorcontrib>Brookhaven National Lab. (BNL), Upton, NY (United States)</creatorcontrib><creatorcontrib>Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)</creatorcontrib><collection>OSTI.GOV - Hybrid</collection><collection>OSTI.GOV</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Zhang, Y.</au><au>Miller, C.</au><au>McKay, T.</au><au>Rooney, P.</au><au>Evrard, A. E.</au><au>Romer, A. K.</au><au>Perfecto, R.</au><au>Song, J.</au><au>Desai, S.</au><au>Mohr, J.</au><au>Wilcox, H.</au><au>Bermeo-Hernandez, A.</au><au>Jeltema, T.</au><au>Hollowood, D.</au><au>Bacon, D.</au><au>Capozzi, D.</au><au>Collins, C.</au><au>Das, R.</au><au>Gerdes, D.</au><au>Hennig, C.</au><au>Hilton, M.</au><au>Hoyle, B.</au><au>Kay, S.</au><au>Liddle, A.</au><au>Mann, R. G.</au><au>Mehrtens, N.</au><au>Nichol, R. C.</au><au>Papovich, C.</au><au>Sahlén, M.</au><au>Soares-Santos, M.</au><au>Stott, J.</au><au>Viana, P. T.</au><au>Abbott, T.</au><au>Abdalla, F. B.</au><au>Banerji, M.</au><au>Bauer, A. H.</au><au>Benoit-Lévy, A.</au><au>Bertin, E.</au><au>Brooks, D.</au><au>Buckley-Geer, E.</au><au>Burke, D. L.</au><au>Rosell, A. Carnero</au><au>Castander, F. J.</au><au>Diehl, H. T.</au><au>Doel, P.</au><au>Cunha, C. E.</au><au>Eifler, T. F.</au><au>Neto, A. Fausti</au><au>Fernandez, E.</au><au>Flaugher, B.</au><au>Fosalba, P.</au><au>Frieman, J.</au><au>Gaztanaga, E.</au><au>Gruen, D.</au><au>Gruendl, R. A.</au><au>Honscheid, K.</au><au>James, D.</au><au>Kuehn, K.</au><au>Kuropatkin, N.</au><au>Lahav, O.</au><au>Maia, M. A. G.</au><au>Makler, M.</au><au>Marshall, J. L.</au><au>Martini, Paul</au><au>Miquel, R.</au><au>Ogando, R.</au><au>Plazas, A. A.</au><au>Roodman, A.</au><au>Rykoff, E. S.</au><au>Sako, M.</au><au>Sanchez, E.</au><au>Scarpine, V.</au><au>Schubnell, M.</au><au>Sevilla, I.</au><au>Smith, R. C.</au><au>Sobreira, F.</au><au>Suchyta, E.</au><au>Swanson, M. E. C.</au><au>Tarle, G.</au><au>Thaler, J.</au><au>Tucker, D.</au><au>Vikram, V.</au><au>Costa, L. N. da</au><aucorp>Brookhaven National Lab. (BNL), Upton, NY (United States)</aucorp><aucorp>Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Galaxies in X-ray Selected Clusters and Groups in Dark Energy Survey Data: Stellar Mass Growth of Bright Central Galaxies Since z~1.2</atitle><jtitle>The Astrophysical journal</jtitle><date>2016-01-10</date><risdate>2016</risdate><volume>816</volume><issue>2</issue><issn>1538-4357</issn><eissn>1538-4357</eissn><abstract>Here, 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.</abstract><cop>United States</cop><pub>Institute of Physics (IOP)</pub><oa>free_for_read</oa></addata></record>
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1538-4357
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subjects ASTRONOMY AND ASTROPHYSICS
galaxies: clusters: general
galaxies: evolution
galaxies: groups: general
title Galaxies in X-ray Selected Clusters and Groups in Dark Energy Survey Data: Stellar Mass Growth of Bright Central Galaxies Since z~1.2
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