Left: total stellar mass from SED fit vs. black hole mass obtained using the bolometric luminosity for our infrared sample of 264 galaxies with both known redshifts/distances and stellar masses (red filled triangles). The data points and bisector linear regression fit of Marleau et al. (2013) (dashed line) are plotted for L_bol/L_Edd = 0.1. Also shown are the fit for L_bol/L_Edd = 1.0 (dotted line) and for L_bol/L_Edd = 0.01 (solid line). Middle: same as left, but showing previously identified AGN of type 1 and type-2, respectively shown as green filled triangles and blue filled triangles, and the AGN candidates identified from the IR diagnostic only, shown as red filled triangles. Also shown are the two low-metallicity and heavily obscured BCDs that were originally identified by Griffith et al. (2011) (magenta filled circles). Right: same as left, but showing the BCDs (cyan filled triangles), the two low-metallicity and heavily obscured BCDs that were originally identified by Griffith et al. (2011) (magenta filled circles), and the BCD MRK 709 S with X-ray and radio emission indicative of AGN activity (yellow filled circle).