Comparisons between stellar masses estimated through (a) the extinction-dependent, and extinction-independent relations of Eq. (6) based on the MCMC fitting (Table 3) which utilize the WISE band-1 photometry and the u − r or the g − r color, (b) the calibration of Wen et al. (2013) which uses the WISE band 1 and the u − r color and (c) based on SED fitting from Chang et al. (2015), Salim et al. (2018), and MPA-JHU (Kauffmann et al. 2003; Brinchmann et al. 2004; Tremonti et al. 2004). In each subplot, the ordinate indicates the logarithm of the ratio (log (M_⋆, y/M_⋆, x)) between the compared M_⋆ estimations, and the abscissa the logarithm of the M_⋆ as indicated in the axes labels. Red error bars represent the modes and 68% percentiles of the distribution of galaxies within bins of log M_⋆/M_⊙ ≃ 0.6 (8 bins within the range 7 < log M_⋆/M_⊙ < 12). The log M_⋆y/M_⋆x modes and 68% percentiles for all the galaxies compared in each panel are shown at the top right of each subplot. The points are color-coded based on the galaxies’ nebular E(B − V). The black dashed line represents equality.