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Fig. 6

image

Surface brightness of the break radius (μbreak, top row) andcentral surface brightness of the inner (μ0,i, central row) and outer profiles (μ0,o, bottom row) as a function of the stellar mass. Left column: distribution of μbreak, μ0,i and μ0,o of Type-III S0 galaxies at 0.2 < z < 0.6 and at z ~ 0 with the stellar mass. The solid vertical black lines in the left panel represent the fixed value at which we compare the linear fits in the right panel. Right column: comparison of the PDDs of μbreak, μ0,i and μ0,o at fixed stellar mass log10(MM) = 10.5. Grey histogram with black solid line: PDDs for the Type-III S0 galaxies in the local Universe selected from E08 and G11 samples. Red histogram with dashed line: PDDs for the Type-III S0 galaxies at 0.4 < z < 0.6 from the SHARDS sample. The probabilities (p-value) that both samples have compatible values at fixed stellar mass of log10(MM) = 10.5 are p = 0.04 (μbreak), p = 0.004 (μ0,i) and p = 0.035 (μ0,o). We refer to the legend in the panels for a key of the different lines and symbols.

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