Upper panel: comparison between stellar masses estimated in this work from WISE photometry, , and those derived from the i magnitude and (g − i)₀ colour following Gavazzi et al. (2013a), extracted from the GOLDMine database . Blue dots and purple diamonds correspond to the HeViCS SFDs and BGC galaxies, respectively. The dotted line shows the one-to-one relation. Lower panel: distribution of the residuals of the two stellar mass estimates for the HeViCS dwarfs (blue histogram) and BGC galaxies (purple histogram). The resulting gaussian fit is overlaid to both histograms.