Extended Data Fig. 2: The relation between BH masses and other major galactic parameters for the BH and galaxy sample.
From: Black holes regulate cool gas accretion in massive galaxies
The relation between MBH and M⋆, Σstar, Mbulge, and SSFR for the BH sample (red filled dots) and the full galaxy sample (blue contours) are shown in Panels a, b, c, and d, respectively. The best-fitted relation for the galaxy sample, the full galaxy, and the HI-detected galaxy sample are respectively drawn in solid orange, darkviolet, and black lines in each panel. These relations are used to derive the residuals of the corresponding galactic parameters after controlling for MBH in the bottom row of Fig. 3, and Extended Data Fig. 3. The median error of the galaxy sample is shown in the upper right in each panel. The error bars refer to 1-σ errors.
