The GaLAxy Cluster Evolution Survey (GLACE): overview and status report

Aimed at understanding the evolution of galaxies in clusters, the GLACE
survey is mapping a set of key optical lines in several galaxy clusters
at z~0.40, 0.63 and 0.85, using the Tunable Filters (TF) of the OSIRIS
instrument. This study will address key questions about the physical
processes acting upon the infalling galaxies during the course of
hierarchical growth of clusters.