The Environmental Effects of Large Scale Structures Around the Galaxy Cluster RXJ0152.7-1357 at z=0.84

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Scientific paper

Large scale ~10 Mpc filaments of galaxies associated with X-ray luminous clusters at z~1 have recently been discovered in ground based wide-field observations. This make it possible to investigate the fundamental properties of galaxies mass, structure and stellar content in a variety of environments field, groups, clusters and compare the environmental effects on galaxy properties at z~1 to those a z~0. We propose to observe filamentary structures around the galaxy cluster RX J0152.7-1357 at z=0.84 in two filters with the Wide Field Camera WFC on the ACS to track down morphological and stellar population differences in the cluster environment and in the less massive substructures in the filaments, providing key elements to understand how the correlations we observe between galaxy properties and galaxy location within a cluster are established and evolve with redshift.

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