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Fig. 9.

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S/N-disk effective radius-B/D selection plot for galaxies from the kinematics sample. The disk size selection criterion is represented as the vertical line. The S/N selection criterion depends on the FWHM, which varies with redshift and MUSE field. As an example, we show the S/N limit used for a typical FWHM of 0.65″. Points are colour-coded according to their bulge-to-disk ratio computed at one effective radius. The grey areas give an idea of the galaxies eliminated by the size and S/N selection criteria. We also show the ten galaxies eliminated by selection criterion v (orange crosses) and the three we decided to keep (orange circles).

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