AKARI NEP-Deep: galaxy clustering through the AKARI IRC filters
  We present a preliminary analysis of clustering of galaxies luminous in the
near- and mid-infrared as seen by seven various ilters of the AKARI IRC
instrument from 2 $\mu$m to 24 $\mu$m in the the AKARI NEP-Deep field. We
compare populations of galaxies detected in different filters and their
clustering properties. We conclude that different AKARI filters allow to trace
different populations composed mainly of star-forming galaxies located in
different environments. In particular, the mid-infrared filters at redshift z
$\sim$ 0.8 and higher trace a population of strongly evolving galaxies located
in massive haloes which might have ended as elliptical galaxies today.
