At 0.5<z<0.8, massive passive galaxies below 2e11 solar masses show no size-environment correlation, while the most massive galaxies in the densest quartile show a deficit of compact (high surface density) systems and an excess of puffy ones.
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The VIMOS Public Extragalactic Redshift Survey (VIPERS) -- Environment-size relation of massive passive galaxies at 0.5 < z < 0.8
At 0.5<z<0.8, massive passive galaxies below 2e11 solar masses show no size-environment correlation, while the most massive galaxies in the densest quartile show a deficit of compact (high surface density) systems and an excess of puffy ones.