The SEDs and Host Galaxies of the dustiest GRB afterglows

TL;DR

This study investigates the properties of dustiest gamma-ray burst (GRB) afterglows and their host galaxies, revealing a diverse, often massive and evolved galaxy population that was previously underrepresented due to observational biases.

Contribution

It provides the first detailed analysis of heavily dust-obscured GRB hosts, showing they are often massive, luminous, and chemically evolved, challenging prior selection biases.

Findings

Dustiest GRB hosts are more luminous and massive than optically-bright ones.

Dust along sight-lines is likely in the diffuse ISM, not near the GRB.

GRBs trace star formation better than optically-selected samples.

Abstract

(Abridged) Until recently the information inferred from gamma-ray burst follow-up observations was mostly limited to optically bright afterglows, biasing all demographic studies against sight-lines that contain large amounts of dust. Here, we present GRB afterglow and host observations for a sample of bursts that are exemplary of previously missed ones because of high visual extinction along the sight-line. This facilitates an investigation of the properties, geometry and location of the absorbing dust of these poorly-explored host galaxies, and a comparison to hosts from optically-selected samples. The hosts of the dustiest afterglows are diverse in their properties, but on average redder, more luminous and massive than the hosts of optically-bright events. We hence probe a different galaxy population, suggesting that previous host samples miss most of the massive, chemically-evolved and metal-rich members. This also indicates that the dust along the sight-line is often related to host properties, and thus probably located in the diffuse ISM or interstellar clouds and not in the immediate GRB environment. Some of the hosts in our sample, are blue, young or of small stellar mass illustrating that even apparently non-extinguished galaxies possess very dusty sight-lines due to a patchy dust distribution. The presented observations establish a population of luminous, massive and correspondingly chemically-evolved GRB hosts. This suggests that GRBs trace the global star-formation rate better than studies based on optically-selected host samples indicate, and the previously-claimed deficiency of high-mass host galaxies was at least partially a selection effect.