Preprint
Evidence for a change in the dominant satellite galaxy quenching mechanism at z=1
Abstract
We present an analysis of galaxies in groups and clusters at $0.810^{10.3}M_\odot$, we find $f_{\rm convert}\sim 0.4$ in the groups and
$\sim 0.6$ in the clusters, similar to comparable measurements at $z=0$. This
Authors
Balogh ML; McGee SL; Mok A; Muzzin A; van der Burg RFJ; Bower RG; Finoguenov A; Hoekstra H; Lidman C; Mulchaey JS
Publication date
November 23, 2015
DOI
10.48550/arxiv.1511.07344
Preprint server
arXiv