Relation between central black hole mass and stellar mass of the host galaxy. The plot is adapted from Sahu et al. (2019). The data points were taken from Sahu et al. (2019) for ETGs and Davis et al. (2018) for LTGs. NGC 4486b and NGC 4342 are tidally stripped galaxies (with significantly decreased host galaxy mass) and are therefore masked in grey. The scaling relations for ETGs and LTGs are visualised as shaded areas. For the ETG FCC 47, the colours indicate the measurement method of this study: orange indicates constant M_*/L, blue is for varying M_*/L with fixed MW-like IMF, and green is for varying M_*/L with free IMF.