Deep VLT imaging of four z~1 clusters reveals a relative excess of faint, low-mass passive galaxies compared to the field, with a composite cluster SMF slope alpha=-0.54 versus alpha=0.12 in the field.
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Insights into environmental quenching at $z\sim1$: an enhancement of faint, low-mass passive galaxies in clusters
Deep VLT imaging of four z~1 clusters reveals a relative excess of faint, low-mass passive galaxies compared to the field, with a composite cluster SMF slope alpha=-0.54 versus alpha=0.12 in the field.