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Evolution of the Early-Type Galaxy Fraction in Clusters since z = 0.8
Luc Simard, Douglas Clowe, Vandana Desai +13
We study the morphological content of a large sample of high-redshift clusters to determine its dependence on cluster mass and redshift. Quantitative morphologies are based on bulg…
A Relationship between Supermassive Black Hole Mass and the Total Gravitational Mass of the Host Galaxy
Kaushala Bandara, David Crampton, Luc Simard
We investigate the correlation between the mass of a central supermassive black hole and the total gravitational mass of the host galaxy (M_tot). The results are based on 43 galaxy…
The Rest-Frame Optical Luminosity Function of Cluster Galaxies at z<0.8 and the Assembly of the Cluster Red Sequence
Gregory Rudnick, Anja von der Linden, Roser Pello +12
We present the rest-frame optical luminosity function (LF) of red sequence galaxies in 16 clusters at 0.4<z<0.8 drawn from the ESO Distant Cluster Survey (EDisCS). We compare our c…
The ESO Distant Cluster Sample: galaxy evolution and environment out to z=1
Bianca M. Poggianti, Alfonso Aragon-Salamanca, Steven Bamford +25
The ESO Distant Cluster Survey (EDisCS, P.I. Simon D.M. White, LP 166.A-0162) is an ESO large programme aimed at studying clusters and cluster galaxies at z=0.4-1. How different is…
The mass-metallicity relation in galaxy clusters: the relative importance of cluster membership versus local environment
Sara L. Ellison, Luc Simard, Nicolas B. Cowan +3
Using a large (14,857), homogenously selected sample of cluster galaxies identified in the Sloan Digital Sky Survey Data Release 4 (SDSS DR4), we investigate the impact of cluster…
Frequency and properties of bars in cluster and field galaxies at intermediate redshifts
Fabio D. Barazza, Pascale Jablonka, Vandana Desai +15
We present a study of large-scale bars in field and cluster environments out to redshifts of ~0.8 using a final sample of 945 moderately inclined disk galaxies drawn from the EDisC…