Fig. 16.
Distribution of log(S3S2) as a function of log(q) inferred with IZI is shown in shades of grey, while its linear fit is given by the dotted magenta line. The green dashed line illustrates the D91 calibration used as a prior. The shaded regions represent the 16th and 84th percentiles of the distribution in each stellar mass bin taking into account the number of galaxies lying in the bin.
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