Radio-Infrared Correlation for Local Dusty Galaxies and Dusty AGNs from
  the AKARI All Sky Survey
  We use the new release of the AKARI Far-Infrared all sky Survey matched with
the NVSS radio database to investigate the local ($z<0.25$) far infrared-radio
correlation (FIRC) of different types of extragalactic sources. To obtain the
redshift information for the AKARI FIS sources we crossmatch the catalogue with
the SDSS DR8. This also allows us to use emission line properties to divide
sources into four categories: i) star-forming galaxies (SFGs), ii) composite
galaxies (displaying both star-formation and active nucleus components), iii)
Seyfert galaxies, and iv) low-ionization nuclear emission-line region (LINER)
galaxies.
  We find that the Seyfert galaxies have the lowest FIR/radio flux ratios and
display excess radio emission when compared to the SFGs. We conclude that FIRC
can be used to separate SFGs and AGNs only for the most radio-loud objects.
