摘要：We aim to use the a new and improved version of AKARI all sky survey catalogue of
far-infrared sources to recalibrate the formula to derive the total infrared luminosity.
We cross-match the faint source catalogue (FSC) of IRAS with the new AKARI-FIS and
obtained a sample of 2430 objects. Then we calculate the total infrared (TIR) luminosity
LTIR from the formula previously estimated
from IRAS data and compare it with total infrared luminosity from AKARI FIS bands to
obtain new coefficients for the general relation to convert FIR luminosity from AKARI
bands to the TIR luminosity.
关键词：infrared: galaxies;galaxies: star formation;galaxies: evolution
