activity
20102024
most citedThe SEDs and Host Galaxies of the dustiest GRB afterglows

184 citations · 2k across the 30 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

7 papers · 1 filter

astro-ph.CO2013★ 78 cited

The Galaxy Counterparts of the two high-metallicity DLAs at z=2.412 and z=2.583 towards Q0918+1636

J. P. U. Fynbo, S. Geier, L. Christensen +9

The quasar Q0918+1636 (z=3.07) has two intervening high-metallicity Damped Lyman-alpha Absorbers (DLAs) along the line of sight, at redshifts of z=2.412 and 2.583. The z=2.583 DLA…

astro-ph.CO2013★ 93 cited

Molecular Hydrogen in the Damped Lyman-alpha System towards GRB 120815A at z=2.36

T. Krühler, C. Ledoux, J. P. U. Fynbo +32

We present the discovery of molecular hydrogen (H_2), including the presence of vibrationally-excited H_2^* in the optical spectrum of the afterglow of GRB 120815A at z=2.36 obtain…

astro-ph.CO2012

TOUGH: Observational aspects of gamma-ray burst host galaxies

Jens Hjorth, Daniele Malesani, Andreas O. Jaunsen +11

GRB-selected galaxies are broadly known to be faint, blue, young, star-forming dwarf galaxies. This insight, however, is based in part on heterogeneous samples of optically selecte…

astro-ph.CO2012★ 82 cited

The optically unbiased GRB host (TOUGH) survey. VI. Radio observations at z<1 and consistency with typical star-forming galaxies

Michał J. Michałowski, A. Kamble, J. Hjorth +19

The objective of this paper is to determine the level of obscured star formation activity and dust attenuation in a sample of gamma-ray burst (GRB) hosts; and to test the hypothesi…

astro-ph.CO2011★ 184 cited

The SEDs and Host Galaxies of the dustiest GRB afterglows

T. Krühler, J. Greiner, P. Schady +18

(Abridged) Until recently the information inferred from gamma-ray burst follow-up observations was mostly limited to optically bright afterglows, biasing all demographic studies ag…

astro-ph.CO2011★ 72 cited

GRB 090426: Discovery of a jet break in a short burst afterglow

A. Nicuesa Guelbenzu, S. Klose, A. Rossi +14

Context: The link between the duration of GRBs and the nature of their progenitors remains disputed. Short bursts (with durations of less than ~2 s) are less frequently observed, t…