Quasar clustering at redshift 6
  Large-scale surveys over the last years have revealed about 300 QSOs at
redshift above 6. Follow-up observations identified surprising properties, such
as the very high black hole (BH) masses, spatial correlations with surrounding
cold gas of the host galaxy, or high CIV-MgII velocity shifts. In particular,
the discovery of luminous high-redshift quasars suggests that at least some
black holes likely have large masses at birth and grow efficiently. We aim at
quantifying quasar pairs at high redshift for a large sample of objects. This
provides a new key constraint on a combination of parameters related to the
origin and assembly for the most massive black holes: BH formation efficiency
and clustering, growth efficiency and relative contribution of BH mergers.
  We observed 116 spectroscopically confirmed QSOs around redshift 6 with the
simultaneous 7-channel imager GROND in order to search for companions. Applying
identical colour-colour cuts as for those which led to the spectroscopically
confirmed QSO, we perform LePHARE fits to the 26 best QSO pair candidates, and
obtained spectroscopic observations for 11 of those. e do not find any QSO pair
with a companion brighter than M1450(AB) < -26 mag within our 0.1-3.3 h^-1 cMpc
search radius, in contrast to the serendipitous findings in the redshift range
4--5. However, a low fraction of such pairs at this luminosity and redshift is
consistent with indications from present-day cosmological-scale galaxy
evolution models. In turn, the incidence of L- and T-type brown dwarfs which
occupy a similar colour space as z ~ 6 QSOs, is higher than expected, by a
factor of 5 and 20, respectively.
