Fig. 1
Left: stellar-mass distribution of our final sample of 18 galaxies (red histogram) compared to that of the parent sample (cyan dashed histogram). The number of galaxies is normalized for a better visualization. Right: main sequence of galaxies. Blue dots represent the parent sample, and red triangles indicate our final kinematical sample. Symbols with arrows denote lower limits to SFR measures (see Sect. 2). Shadowed regions indicate the 68% confidence contours of the main-sequence fit by Wuyts et al. (2011) (solid cyan line) at 0.5 <z< 1.5.
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