Comparison between our M_* and M_BH from Eq. (9) and parameters α and β from Table 3 for star-forming galaxies and results from models in the literature. Data from this work are shown as solid lines and are color-coded according to redshift as in Figs. 3 and 4. The relations from Savorgnan & Graham (2016) use the M_* of the bulge. The gray shaded area is the confidence range for Savorgnan & Graham (2016), and the light green are is the confidence range for Shankar et al. (2016).