H0LiCOW VII: cosmic evolution of the correlation between black hole mass and host galaxy luminosity

Xuheng Ding, Tommaso Treu, Sherry H. Suyu, Kenneth C. Wong, Takahiro Morishita, Daeseong Park, Dominique Sluse, Matthew W. Auger, Adriano Agnello, Vardha N. Bennert, Thomas E. Collett

Research output: Contribution to journalArticlepeer-review

125 Downloads (Pure)


Strongly lensed active galactic nuclei (AGN) provide a unique opportunity to make progress in the study of the evolution of the correlation between the mass of supermassive black holes (MBH) and their host galaxy luminosity (Lhost). We demonstrate the power of lensing by analysing two systems for which state-of-the-art lens modelling techniques have been applied to deep Hubble Space Telescope imaging data. We use (i) the reconstructed images to infer the total and bulge luminosity of the host and (ii) published broad-line spectroscopy to estimate MBH using the so-called virial method. We then enlarge our sample with new calibration of previously published measurements to study the evolution of the correlation out to z ∼ 4.5. Consistent with previous work, we find that without taking into account passive luminosity evolution, the data points lie on the local relation. Once the passive luminosity evolution is taken into account, we find that black holes in the more distant Universe reside in less luminous galaxies than today. Fitting this offset as MBH/Lhost ∝ (1 + z)γ, and taking into account selection effects, we obtain γ = 0.6 ± 0.1 and 0.8 ± 0.1 for the case of MBH -Lbulge and MBH -Ltotal, respectively. To test for systematic uncertainties and selection effects we also consider a reduced sample that is homogeneous in data quality. We find consistent results but with considerably larger uncertainty due to the more limited sample size and redshift coverage (γ = 0.7 ± 0.4 and 0.2 ± 0.5 for MBH -Lbulge and MBH -Ltotal, respectively), highlighting the need to gather more high-quality data for high-redshift lensed quasar hosts. Our result is consistent with a scenario where the growth of the black hole predates that of the host galaxy.
Original languageEnglish
Pages (from-to)90-103
Number of pages14
JournalMonthly Notices of the Royal Astronomical Society
Issue number1
Early online date2 Aug 2017
Publication statusPublished - 21 Nov 2017


  • black hole physics
  • galaxies: active
  • galaxies: evolution


Dive into the research topics of 'H0LiCOW VII: cosmic evolution of the correlation between black hole mass and host galaxy luminosity'. Together they form a unique fingerprint.

Cite this