We investigate the role of environment on star formation rates (SFRs) of galaxies at various cosmic densities in well-studied clusters. We present the star-forming main sequence for 163 galaxies in four EDisCS clusters in the range 0.4 < z 109.75 M_{sun} show little dependence on environment. At face value, the similarities in the SFR distributions in the three environments may indicate that the process of finally shutting down star formation is rapid, however, the depth of our data and size of our sample make it difficult to conclusively test this scenario. Despite having significant H{alpha}_ emission, 21 galaxies are classified as UVJ-quiescent and may represent a demonstration of the quenching of star formation caught in the act.
Cone search capability for table J/MNRAS/509/5382/tablee1 (Properties of our core galaxy sample)
Cone search capability for table J/MNRAS/509/5382/tablee2 (Properties of out infalling galaxy sample)
Cone search capability for table J/MNRAS/509/5382/tablee3 (Properties of our field galaxy sample)