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

Y. Zhang; C. Miller; T. McKay; P. Rooney; A. E. Evrard; A. K. Romer; R. Perfecto; J. Song; S. Desai; J. Mohr; H. Wilcox; A. Bermeo-Hernandez; T. Jeltema; D. Hollowood; D. Bacon; D. Capozzi; C. Collins; R. Das; D. Gerdes; C. Hennig; M. Hilton; B. Hoyle; S. Kay; A. Liddle; R. G. Mann; N. Mehrtens; R. C. Nichol; C. Papovich; M. Sahlén; M. Soares-Santos; J. Stott; P. T. Viana; T. Abbott; F. B. Abdalla; M. Banerji; A. H. Bauer; A. Benoit-Lévy; E. Bertin; D. Brooks; E. Buckley-Geer; D. L. Burke; A. Carnero Rosell; F. J. Castander; H. T. Diehl; P. Doel; C. E. Cunha; T. F. Eifler; A. Fausti Neto; E. Fernandez; B. Flaugher; P. Fosalba; J. Frieman; E. Gaztanaga; D. Gruen; R. A. Gruendl; K. Honscheid; D. James; K. Kuehn; N. Kuropatkin; O. Lahav; M. A. G. Maia; M. Makler; J. L. Marshall; Paul Martini; R. Miquel; R. Ogando; A. A. Plazas; A. Roodman; E. S. Rykoff; M. Sako; E. Sanchez; V. Scarpine; M. Schubnell; I. Sevilla; R. C. Smith; F. Sobreira; E. Suchyta; M. E. C. Swanson; G. Tarle; J. Thaler; D. Tucker; V. Vikram; L. N. da Costa

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

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

Y. Zhang, C. Miller, T. McKay, P. Rooney, A. E. Evrard, A. K. Romer, R. Perfecto, J. Song, S. Desai, J. Mohr, H. Wilcox, A. Bermeo-Hernandez, T. Jeltema, D. Hollowood, D. Bacon, D. Capozzi, C. Collins, R. Das, D. Gerdes, C. HennigM. Hilton, B. Hoyle, S. Kay, A. Liddle, R. G. Mann, N. Mehrtens, R. C. Nichol, C. Papovich, M. Sahlén, M. Soares-Santos, J. Stott, P. T. Viana, T. Abbott, F. B. Abdalla, M. Banerji, A. H. Bauer, A. Benoit-Lévy, E. Bertin, D. Brooks, E. Buckley-Geer, D. L. Burke, A. Carnero Rosell, F. J. Castander, H. T. Diehl, P. Doel, C. E. Cunha, T. F. Eifler, A. Fausti Neto, E. Fernandez, B. Flaugher, P. Fosalba, J. Frieman, E. Gaztanaga, D. Gruen, R. A. Gruendl, K. Honscheid, D. James, K. Kuehn, N. Kuropatkin, O. Lahav, M. A. G. Maia, M. Makler, J. L. Marshall, Paul Martini, R. Miquel, R. Ogando, A. A. Plazas, A. Roodman, E. S. Rykoff, M. Sako, E. Sanchez, V. Scarpine, M. Schubnell, I. Sevilla, R. C. Smith, F. Sobreira, E. Suchyta, M. E. C. Swanson, G. Tarle, J. Thaler, D. Tucker, V. Vikram, L. N. da Costa

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Abstract / Description of output

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}*∝ ({M}200}/{1.5×{10}14{M}⊙}) 0.24+/-0.08(1+z)-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 M200,z = 1013.8 M⊙ at z = 1.0: m*,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.

Original language	English
Pages (from-to)	98
Number of pages	20
Journal	Astrophysical Journal
Volume	816
Issue number	2
DOIs	https://doi.org/10.3847/0004-637X/816/2/98
Publication status	Published - 14 Jan 2016

Keywords / Materials (for Non-textual outputs)

galaxies: clusters: general
galaxies: evolution
galaxies: groups: general

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

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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., ... da Costa, L. N. (2016). 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. Astrophysical Journal, 816(2), 98. https://doi.org/10.3847/0004-637X/816/2/98

@article{fe1fdfd9ffea49b49d8f2dd11675749e,

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",

abstract = "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}*∝ ({M}200}/{1.5×{10}14{M}⊙}) 0.24+/-0.08(1+z)-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 M200,z = 1013.8 M⊙ at z = 1.0: m*,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.",

keywords = "galaxies: clusters: general, galaxies: evolution, galaxies: groups: general",

author = "Y. Zhang and C. Miller and T. McKay and P. Rooney and Evrard, {A. E.} and Romer, {A. K.} and R. Perfecto and J. Song and S. Desai and J. Mohr and H. Wilcox and A. Bermeo-Hernandez and T. Jeltema and D. Hollowood and D. Bacon and D. Capozzi and C. Collins and R. Das and D. Gerdes and C. Hennig and M. Hilton and B. Hoyle and S. Kay and A. Liddle and Mann, {R. G.} and N. Mehrtens and Nichol, {R. C.} and C. Papovich and M. Sahl{\'e}n and M. Soares-Santos and J. Stott and Viana, {P. T.} and T. Abbott and Abdalla, {F. B.} and M. Banerji and Bauer, {A. H.} and A. Benoit-L{\'e}vy and E. Bertin and D. Brooks and E. Buckley-Geer and Burke, {D. L.} and {Carnero Rosell}, A. and Castander, {F. J.} and Diehl, {H. T.} and P. Doel and Cunha, {C. E.} and Eifler, {T. F.} and {Fausti Neto}, A. and E. Fernandez and B. Flaugher and P. Fosalba and J. Frieman and E. Gaztanaga and D. Gruen and Gruendl, {R. A.} and K. Honscheid and D. James and K. Kuehn and N. Kuropatkin and O. Lahav and Maia, {M. A. G.} and M. Makler and Marshall, {J. L.} and Paul Martini and R. Miquel and R. Ogando and Plazas, {A. A.} and A. Roodman and Rykoff, {E. S.} and M. Sako and E. Sanchez and V. Scarpine and M. Schubnell and I. Sevilla and Smith, {R. C.} and F. Sobreira and E. Suchyta and Swanson, {M. E. C.} and G. Tarle and J. Thaler and D. Tucker and V. Vikram and {da Costa}, {L. N.}",

year = "2016",

month = jan,

day = "14",

doi = "10.3847/0004-637X/816/2/98",

language = "English",

volume = "816",

pages = "98",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "IOP Publishing",

number = "2",

}

Zhang, Y, Miller, C, McKay, T, Rooney, P, Evrard, AE, Romer, AK, 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, RG, Mehrtens, N, Nichol, RC, Papovich, C, Sahlén, M, Soares-Santos, M, Stott, J, Viana, PT, Abbott, T, Abdalla, FB, Banerji, M, Bauer, AH, Benoit-Lévy, A, Bertin, E, Brooks, D, Buckley-Geer, E, Burke, DL, Carnero Rosell, A, Castander, FJ, Diehl, HT, Doel, P, Cunha, CE, Eifler, TF, Fausti Neto, A, Fernandez, E, Flaugher, B, Fosalba, P, Frieman, J, Gaztanaga, E, Gruen, D, Gruendl, RA, Honscheid, K, James, D, Kuehn, K, Kuropatkin, N, Lahav, O, Maia, MAG, Makler, M, Marshall, JL, Martini, P, Miquel, R, Ogando, R, Plazas, AA, Roodman, A, Rykoff, ES, Sako, M, Sanchez, E, Scarpine, V, Schubnell, M, Sevilla, I, Smith, RC, Sobreira, F, Suchyta, E, Swanson, MEC, Tarle, G, Thaler, J, Tucker, D, Vikram, V & da Costa, LN 2016, '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', Astrophysical Journal, vol. 816, no. 2, pp. 98. https://doi.org/10.3847/0004-637X/816/2/98

TY - JOUR

T1 - 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

AU - Zhang, Y.

AU - Miller, C.

AU - McKay, T.

AU - Rooney, P.

AU - Evrard, A. E.

AU - Romer, A. K.

AU - Perfecto, R.

AU - Song, J.

AU - Desai, S.

AU - Mohr, J.

AU - Wilcox, H.

AU - Bermeo-Hernandez, A.

AU - Jeltema, T.

AU - Hollowood, D.

AU - Bacon, D.

AU - Capozzi, D.

AU - Collins, C.

AU - Das, R.

AU - Gerdes, D.

AU - Hennig, C.

AU - Hilton, M.

AU - Hoyle, B.

AU - Kay, S.

AU - Liddle, A.

AU - Mann, R. G.

AU - Mehrtens, N.

AU - Nichol, R. C.

AU - Papovich, C.

AU - Sahlén, M.

AU - Soares-Santos, M.

AU - Stott, J.

AU - Viana, P. T.

AU - Abbott, T.

AU - Abdalla, F. B.

AU - Banerji, M.

AU - Bauer, A. H.

AU - Benoit-Lévy, A.

AU - Bertin, E.

AU - Brooks, D.

AU - Buckley-Geer, E.

AU - Burke, D. L.

AU - Carnero Rosell, A.

AU - Castander, F. J.

AU - Diehl, H. T.

AU - Doel, P.

AU - Cunha, C. E.

AU - Eifler, T. F.

AU - Fausti Neto, A.

AU - Fernandez, E.

AU - Flaugher, B.

AU - Fosalba, P.

AU - Frieman, J.

AU - Gaztanaga, E.

AU - Gruen, D.

AU - Gruendl, R. A.

AU - Honscheid, K.

AU - James, D.

AU - Kuehn, K.

AU - Kuropatkin, N.

AU - Lahav, O.

AU - Maia, M. A. G.

AU - Makler, M.

AU - Marshall, J. L.

AU - Martini, Paul

AU - Miquel, R.

AU - Ogando, R.

AU - Plazas, A. A.

AU - Roodman, A.

AU - Rykoff, E. S.

AU - Sako, M.

AU - Sanchez, E.

AU - Scarpine, V.

AU - Schubnell, M.

AU - Sevilla, I.

AU - Smith, R. C.

AU - Sobreira, F.

AU - Suchyta, E.

AU - Swanson, M. E. C.

AU - Tarle, G.

AU - Thaler, J.

AU - Tucker, D.

AU - Vikram, V.

AU - da Costa, L. N.

PY - 2016/1/14

Y1 - 2016/1/14

N2 - 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}*∝ ({M}200}/{1.5×{10}14{M}⊙}) 0.24+/-0.08(1+z)-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 M200,z = 1013.8 M⊙ at z = 1.0: m*,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.

AB - 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}*∝ ({M}200}/{1.5×{10}14{M}⊙}) 0.24+/-0.08(1+z)-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 M200,z = 1013.8 M⊙ at z = 1.0: m*,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.

KW - galaxies: clusters: general

KW - galaxies: evolution

KW - galaxies: groups: general

U2 - 10.3847/0004-637X/816/2/98

DO - 10.3847/0004-637X/816/2/98

M3 - Article

SN - 0004-637X

VL - 816

SP - 98

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2

ER -

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

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Keywords / Materials (for Non-textual outputs)

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