Observing galaxy mergers at the epoch of reionization
  The galaxies with photometric redshifts observed in a close angular proximity
might be either projection coincidences, strongly lensed images of the same
galaxy, or separate galaxies that are in a stage of merging. We search for the
groups of galaxies in the Hubble Ultra Deep Field (HUDF09) in $z\sim7$ and
$z\sim8$ drop-out samples. We find no close pairs among 50 galaxies in the
$z\sim7$ sample, while in the $z\sim8$ sample we find that 6 out of 22 galaxies
have a companion within $\sim1'$ (3 pairs). Adopting a numerical simulation and
performing forward modeling we show that even though mergers are unlikely to
have such a high fraction, the projection coincidences and the strong lensing
are even less likely mechanisms to account for all of three pairs.
Alternatively, there is a possibility of the contamination in the drop-out
catalog from lower redshifts, which potentially can account for all of the
groups. Finally, we make projection on the sensitivity to mergers of the James
Webb Space Telescope, and discuss the possible applications of the
high-redshift merging galaxies for decreasing cosmic variance effect on the
luminosity function and for improving the accuracy of photometric redshifts in
general.
