TY - JOUR
T1 - Evidence for the universality of properties of red-sequence galaxies in x-ray- and red-sequence-selected clusters at z ∼ 1
AU - Foltz, R.
AU - Rettura, A.
AU - Wilson, G.
AU - Van Der Burg, R. F.J.
AU - Muzzin, A.
AU - Lidman, C.
AU - Demarco, R.
AU - Nantais, Julie
AU - Degroot, A.
AU - Yee, H.
N1 - Publisher Copyright:
© 2015. The American Astronomical Society. All rights reserved..
PY - 2015/10/20
Y1 - 2015/10/20
N2 - We study the slope, intercept, and scatter of the color-magnitude and color-mass relations for a sample of 10 infrared red-sequence-selected clusters at z ∼ 1. The quiescent galaxies in these clusters formed the bulk of their stars above z 3 with an age spread Δt 1 Gyr. We compare UVJ color-color and spectroscopic-based galaxy selection techniques, and find a 15% difference in the galaxy populations classified as quiescent by these methods. We compare the color-magnitude relations from our red-sequence selected sample with X-ray- and photometric-redshift-selected cluster samples of similar mass and redshift. Within uncertainties, we are unable to detect any difference in the ages and star formation histories of quiescent cluster members in clusters selected by different methods, suggesting that the dominant quenching mechanism is insensitive to cluster baryon partitioning at z ∼ 1.
AB - We study the slope, intercept, and scatter of the color-magnitude and color-mass relations for a sample of 10 infrared red-sequence-selected clusters at z ∼ 1. The quiescent galaxies in these clusters formed the bulk of their stars above z 3 with an age spread Δt 1 Gyr. We compare UVJ color-color and spectroscopic-based galaxy selection techniques, and find a 15% difference in the galaxy populations classified as quiescent by these methods. We compare the color-magnitude relations from our red-sequence selected sample with X-ray- and photometric-redshift-selected cluster samples of similar mass and redshift. Within uncertainties, we are unable to detect any difference in the ages and star formation histories of quiescent cluster members in clusters selected by different methods, suggesting that the dominant quenching mechanism is insensitive to cluster baryon partitioning at z ∼ 1.
KW - galaxies: clusters: general
KW - galaxies: elliptical and lenticular, cD
KW - galaxies: evolution
KW - galaxies: formation
KW - galaxies: stellar content
UR - http://www.scopus.com/inward/record.url?scp=84946060669&partnerID=8YFLogxK
U2 - 10.1088/0004-637X/812/2/138
DO - 10.1088/0004-637X/812/2/138
M3 - Article
AN - SCOPUS:84946060669
SN - 0004-637X
VL - 812
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
M1 - 138
ER -