Spectral energy distributions of an AKARI-SDSS-GALEX sample of galaxies

TL;DR

This study analyzes the spectral energy distributions of 363 nearby galaxies across 13 bands from UV to far-IR to understand dust attenuation and star formation rates, using the CIGALE code for detailed modeling.

Contribution

It provides a comprehensive analysis of dust attenuation laws and star formation rate calibrations in a large, multi-wavelength galaxy sample, highlighting the need for time-dependent dust attenuation models.

Findings

Dust attenuation law slightly steeper than starburst galaxies

Time-dependent dust attenuation improves fit quality

17% of dust luminosity from old stars not related to recent star formation

Abstract

The nearby universe remains the best laboratory to understand physical properties of galaxies and is a reference for any comparison with high redshift observations. The all sky (or very large) surveys performed from the ultraviolet (UV) to the far-infrared (far-IR) gives us large datasets with a very large wavelength coverage to perform a reference study. We want to investigate dust attenuation characteristics as well as star formation rate (SFR) calibrations on a sample of nearby galaxies observed over 13 bands from 0.15 to 160 microns. A sample of 363 galaxies is built from the AKARI /FIS all sky survey cross-correlated with SDSS and GALEX surveys. Broad band spectral energy distributions are fitted with the CIGALE code optimized to analyze variations in dust attenuation curves and SFR measurements and based on an energetic budget between the stellar and dust emission. Our galaxy sample is primarily selected in far-IR and mostly constituted of massive, actively star forming galaxies. There is some evidence for a dust attenuation law slightly steeper than that used for starburst galaxies but we are unable to constrain the presence or not of a bump at 220 nm. We confirm that a time dependent dust attenuation is necessary to perform the best fits. Various calibrations of the dust attenuation in the UV as a function of UV-optical colours are discussed. A calibration of the current star formation rate combining UV and total IR emissions is proposed with an accurate estimation of dust heating by old stars: for the whole sample 17 % of the total dust luminosity is not related to the recent star formation