activity
19962008
most citedUV star-formation rates of GRB host galaxies

295 citations · 1.7k across the 28 of their papers we have counts for

collaborators
Showing 2001Show all

7 papers · 1 filter

astro-ph2001

Strategies for prompt searches for GRB afterglows: the discovery of the GRB 001011 optical/near-infrared counterpart using colour-colour selection

J. Gorosabel, J. U. Fynbo, J. Hjorth +25

We report the discovery of the optical and near-infrared counterparts to GRB 001011. The GRB 001011 error box determined by Beppo-SAX was simultaneously imaged in the near-infrared…

astro-ph2001

A novel approach for extracting time-delays from lightcurves of lensed quasar images

I. Burud, P. Magain, S. Sohy +1

We present a new method to estimate time delays from light curves of lensed quasars. The method is based on chi^2 minimization between the data and a numerical model light curve. A…

astro-ph2001

Constraints on the optical afterglow emission of the short/hard burst GRB 010119

J. Gorosabel, M. I. Andersen, J. Hjorth +7

We report optical observations of the short/hard burst GRB 010119 error box, one of the smallest error boxes reported to date for short/hard GRBs. Limits of R > 22.3 and I > 21.2 a…

astro-ph2001

The Jet and the Supernova in GRB990712

G. Bjornsson, J. Hjorth, P. Jakobsson +2

The optical light curve of the afterglow following the gamma-ray burst GRB990712 is re-examined. Recently published polarization measurements of that source require a collimated ou…

astro-ph2001

The Host Galaxy and Optical Light Curve of the Gamma-Ray Burst GRB 980703

S. Holland, J. P. U. Fynbo, J. Hjorth +10

We present deep HST/STIS and ground-based photometry of the host galaxy of the gamma-ray burst GRB 980703 taken 17, 551, 710, and 716 days after the burst. We find that the host is…

astro-ph2001

The extraordinarily bright optical afterglow of GRB 991208 and its host galaxy

A. J. Castro-Tirado, V. V. Sokolov, J. Gorosabel +50

Observations of the extraordinarily bright optical afterglow (OA) of GRB 991208 started 2.1 d after the event. The flux decay constant of the OA in the R-band is -2.30 +/- 0.07 up…