# A Universal Relation of Dust Obscuration Across Cosmic Time

## TL;DR

This study uncovers a universal empirical relation linking dust obscuration, galaxy size, metallicity, and infrared luminosity, valid across cosmic time, revealing key parameters influencing dust attenuation in star-forming galaxies.

## Contribution

It introduces a new empirical relation for IRX that is universal over cosmic time and depends on IR luminosity, size, and metallicity, but not stellar mass.

## Key findings

- IRX correlates with stellar mass, SFR, metallicity, IR luminosity, and galaxy size.
- The empirical relation has a scatter of about 0.17 dex and is valid up to redshift 3.
- Dust obscuration is primarily governed by IR luminosity, metallicity, and galaxy size.

## Abstract

We investigate dust obscuration as parameterised by the infrared excess IRX$\equiv$$L_{\rm IR}/L_{\rm UV}$ in relation to global galaxy properties, using a sample of $\sim$32$\,$000 local star-forming galaxies (SFGs) selected from SDSS, GALEX and WISE. We show that IRX generally correlates with stellar mass ($M_\ast$), star formation rate (SFR), gas-phase metallicity ($Z$), infrared luminosity ($L_{\rm IR}$) and the half-light radius ($R_{\rm e}$). A weak correlation of IRX with axial ratio (b/a) is driven by the inclination and thus seen as a projection effect. By examining the tightness and the scatter of these correlations, we find that SFGs obey an empirical relation of the form $IRX$=$10^\alpha\,(L_{\rm IR})^{\beta}\,R_{\rm e}^{-\gamma}\,(b/a)^{-\delta}$ where the power-law indices all increase with metallicity. The best-fitting relation yields a scatter of $\sim$0.17$\,$dex and no dependence on stellar mass. Moreover, this empirical relation also holds for distant SFGs out to $z=3$ in a population-averaged sense, suggesting it to be universal over cosmic time. Our findings reveal that IRX approximately increases with $L_{\rm IR}/R_{\rm e}^{[1.3 - 1.5]}$ instead of $L_{\rm IR}/R_{\rm e}^{2}$ (i.e., surface density). We speculate this may be due to differences in the spatial extent of stars versus star formation and/or complex star-dust geometries. We conclude that not stellar mass but IR luminosity, metallicity and galaxy size are the key parameters jointly determining dust obscuration in SFGs.