Total infrared luminosity estimation from local galaxies in AKARI all sky survey

Abstract

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 $L_{\text{TIR}}$ from the Sanders at al. (1996) formula 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.

arXiv comment4 pages, 4 figures

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Cited by in corpus (5)

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• Radio-Infrared Correlation for Local Dusty Galaxies and Dusty AGNs from the AKARI All Sky Survey
• Broad-velocity-width Molecular Features in the Galactic Plane
• Estimating Galaxy Star Formation Rates from Murchison Widefield Array Radio Continuum Emission