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Fig. 8


Distribution of the Type-III S0 galaxies at 0.2 < z < 0.6 vs. the local sample from E08 and G11 in the μbreakRbreak diagram. The relation fitted was in logarithmic scale for the x-axis. Left panel: diagram and 2D model analysis for the μbreak values with maximum inclination correction (C = 1, optically transparent). Right panel: diagram and 2D model analysis for the μbreak values without inclination correction, removing the objects with stellar masses larger than the local sample (SHARDS10009610 and SHARDS20000827). Dashed lines: contours of equal redshift for the surface brightness at the break radius (μbreak) as a functionof Rbreak and redshift (from Eq. 1). Dashed-dotted lines: detection limit for Type-III profiles as a function of redshift. Consult the legend in the figure for the redshift colour classification and 3D fit results.

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