Initial analysis of extragalactic fields using a new AKARI/IRC analysis
  pipeline
  We present the first results of a new data analysis pipeline for processing
extragalactic AKARI/IRC images. The main improvements of the pipeline over the
standard analysis are the removal of Earth shine and image distortion
correction. We present the differential number counts of the AKARI/IRC S11
filter IRAC validation field. The differential number counts are consistent
with S11 AKARI NEP deep and 12 microns WISE NEP number counts, and with a
phenomenological backward evolution galaxy model, at brighter fluxes densities.
There is a detection of deeper galaxies in the IRAC validation field.
