Secular evolution and a non-evolving black hole to galaxy mass ratio in the last 7 Gyr
Mauricio Cisternas, Knud Jahnke, Angela Bongiorno, Katherine J., Inskip, Chris D. Impey, Anton M. Koekemoer, Andrea Merloni, Mara Salvato,, Jonathan R. Trump

TL;DR
This study finds that the ratio of black hole mass to galaxy stellar mass has remained essentially unchanged over the last 7 billion years, suggesting secular processes drive galaxy evolution rather than major mergers.
Contribution
It provides new observational constraints on the black hole to galaxy mass ratio up to z~0.9, showing no significant evolution and highlighting the role of secular processes in galaxy growth.
Findings
Black hole to galaxy mass ratio shows no evolution up to z~0.9.
No substantial stellar mass addition needed since z~0.9.
Secular processes likely drive bulge growth in galaxies.
Abstract
We present new constraints on the ratio of black hole (BH) mass to total galaxy stellar mass at 0.3<z<0.9 for a sample of 32 type-1 active galactic nuclei (AGNs) from the XMM-COSMOS survey covering the range M_BH/M_sun~10^(7.2--8.7). Virial M_BH estimates based on H_beta are available from the COSMOS Magellan/IMACS survey. We use high-resolution Hubble Space Telescope (HST) imaging to decompose the light of each type-1 AGN and host galaxy, and employ a specially-built mass-to-light ratio to estimate the stellar masses (M_*). The M_BH-M_* ratio shows a zero offset with respect to the local relation for galactic bulge masses, and we also find no evolution in the mass ratio M_BH/M_*=(1+z)^{0.02+-0.34} up to z~0.9. Interestingly, at the high-M_BH end there is a positive offset from the z=0 relation, which can be fully explained by a mass function bias with a cosmic scatter of 0.3,…
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