Extended Data Fig. 4: Comparison of simulated AGNs and their host galaxies with SDSS observations. | Nature Astronomy

Extended Data Fig. 4: Comparison of simulated AGNs and their host galaxies with SDSS observations.

From: Galaxy and black hole co-evolution in dark matter haloes not captured by cosmological simulations

Extended Data Fig. 4

Panels (a)-(e) show the distributions of (a) AGN luminosity, (b) Eddington ratio, (c) black hole-to-stellar mass ratio, (d) stellar mass, and (e) specific star formation rate, while panel (f) shows stellar mass versus star formation rate. The sample is restricted to galaxies with LAGN > 1042erg s−1, M* > 109 M ⊙ and z < 0.15. SDSS distributions are weighted by 1/Vmax to correct for sample incompleteness.

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