Massive Black Holes at High Redshifts

Black holes with masses Mbh ∼ 10M⊙ dominate the accretion history of the Universe. These black hole masses are typical of those found in radio-selected galaxies today, suggesting that the giant elliptical hosts of low redshift radio galaxies were the hosts of powerful, mostly radio-quiet, quasars in the high redshift Universe. The reason that all radio galaxies are found in such hosts may be the correlation of black hole mass with radio luminosity, but it is emphasized that accretion rate too plays an important role in the production of powerful radio jets. The tight K − z relation of luminous, high redshift, radio galaxies is probably a selection effect due to the selection on high black hole masses and high accretion rates. Luminous radio galaxies are the radio-loud part of the “quasar-2” population, and the ratio of radio-loud quasars to luminous radio galaxies, about 1:1, is so far our only good estimate of the relative numbers of quasar-1s and quasar-2s. The numbers of radio-quiet and radiointermediate quasar-2s are still uncertain, but a much larger population than the quasar-1s would conflict with constraints from the present-day black hole mass density. A comparison of the number densities of dark matter haloes and the high redshift quasars, however, suggests that there are plenty of dark haloes capable of hosting the known high redshift AGN and thus room for a significant, but not huge, quasar-2 population. 1.