activity
19952012
most citedThe Quadruple Gravitational Lens PG1115+080: Time Delays and Models

244 citations · 1.9k across the 38 of their papers we have counts for

collaborators

39 papers

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★ 193 cited

The optically unbiased GRB host (TOUGH) survey. I. Survey design and catalogs

Jens Hjorth, Daniele Malesani, Páll Jakobsson +11

Long-duration gamma-ray bursts (GRBs) are powerful tracers of star-forming galaxies. We have defined a homogeneous subsample of 69 Swift GRB-selected galaxies spanning a very wide…

astro-ph.IM2011★ 14 cited

A study of NIR atmospheric properties at Paranal Observatory

G. Lombardi, E. Mason, C. Lidman +2

In order to maximize the scientific return of the telescopes located at the Paranal Observatory, we analyse the properties of the atmosphere above Paranal in the near-infrared (NIR…

astro-ph2008★ 52 cited

Photometry and spectroscopy of GRB 060526: A detailed study of the afterglow and host galaxy of a z=3.2 gamma-ray burst

C. C. Thöne, D. A. Kann, G. Jóhannesson +58

Aims: With this paper we want to investigate the highly variable afterglow light curve and environment of gamma-ray burst (GRB) 060526 at . Methods: We present one of the…

astro-ph2008★ 72 cited

Early spectroscopic identification of SN 2008D

D. Malesani, J. P. U. Fynbo, J. Hjorth +27

SN 2008D was discovered while following up an unusually bright X-ray transient in the nearby spiral galaxy NGC 2770. We present early optical spectra (obtained 1.75 days after the…

astro-ph2008★ 45 cited

The extreme, red afterglow of GRB 060923A: Distance or dust?

N. R. Tanvir, A. J. Levan, E. Rol +16

Gamma-ray bursts are powerful probes of the early universe, but locating and identifying very distant GRBs remains challenging. We report here the discovery of the K-band afterglow…