Total Infrared Luminosity Estimation of Resolved and Unresolved Galaxies

TL;DR

This paper develops new relations to estimate the total infrared luminosity of galaxies using specific Spitzer bands, accounting for metallicity and star formation rate, to improve accuracy in both resolved and unresolved galaxies.

Contribution

It introduces novel relations for TIR luminosity estimation from Spitzer bands, incorporating metallicity and star formation rate effects, enhancing previous methods.

Findings

New relations for TIR luminosity from 8 and 24 micron bands.

Metallicity and star formation rate influence TIR estimates.

Improved accuracy for unresolved galaxy measurements.

Abstract

The total infrared (TIR) luminosity from galaxies can be used to examine both star formation and dust physics. We provide here new relations to estimate the TIR luminosity from various Spitzer bands, in particular from the 8 micron and 24 micron bands. To do so, we use 45" subregions within a subsample of nearby face-on spiral galaxies from the Spitzer Infrared Nearby Galaxies Survey (SINGS) that have known oxygen abundances as well as integrated galaxy data from the SINGS, the Local Volume Legacy Survey (LVL) and Engelbracht et al. (2008) samples. Taking into account the oxygen abundances of the subregions, the star formation rate intensity, and the relative emission of the polycyclic aromatic hydrocarbons at 8 micron, the warm dust at 24 micron and the cold dust at 70 micron and 160 micron we derive new relations to estimate the TIR luminosity from just one or two of the Spitzer bands. We also show that the metallicity and the star formation intensity must be taken into account when estimating the TIR luminosity from two wave bands, especially when data longward of 24 micron are not available.