Extended Data Fig. 6: The comparison between the stellar masses derived from SED-fitting and those derived based on K-band luminosities.
From: Black holes regulate cool gas accretion in massive galaxies
The SED-based estimation M⋆ is taken from the MPA-JHU catalog and the K-band luminosity based estimation of M⋆ is derived from the relation among M⋆, LK and Re given by Ref. 21. The dashed line denotes the ‘1:1’ line shifted by the mean mass difference of 0.32 dex. The error bars refer to 1-σ error.
