activity
20012005
most citedThe line-of-sight towards GRB 030429 at z = 2.66: Probing the matter at stellar, galactic and intergalactic scales

129 citations · 274 across the 5 of their papers we have counts for

collaborators

8 papers

astro-ph20058 cited

The red optical afterglow of GRB 030725

G. Pugliese, P. Møller, J. Gorosabel +6

We present a photometric study of the optical counterpart of the long-duration Gamma Ray Burst (GRB) 030725, which triggered the HETE FREGATE and WXM instruments on July 25th, 2003…

astro-ph200533 cited

Late-epoch optical and near-infrared observations of the GRB000911 afterglow and its host galaxy

N. Masetti, E. Palazzi, E. Pian +28

We present the results of an optical and near-infrared (NIR) monitoring campaign of the counterpart of Gamma-Ray Burst (GRB) 000911, located at redshift z=1.06, from 5 days to more…

astro-ph2004129 cited

The line-of-sight towards GRB 030429 at z = 2.66: Probing the matter at stellar, galactic and intergalactic scales

P. Jakobsson, J. Hjorth, J. P. U. Fynbo +21

We report the discovery of the optical afterglow (OA) of the long-duration gamma-ray burst GRB 030429, and present a comprehensive optical/near-infrared dataset used to probe the m…

astro-ph200354 cited

Delayed soft X-ray emission lines in the afterglow of GRB 030227

D. Watson, J. N. Reeves, J. Hjorth +2

Strong, delayed X-ray line emission is detected in the afterglow of GRB 030227, appearing near the end of the XMM-Newton observation, nearly twenty hours after the burst. The obser…

astro-ph200250 cited

The Afterglow of GRB010222: A Case of Continuous Energy Injection

G. Bjornsson, J. Hjorth, K. Pedersen +1

The optical lightcurve of GRB010222 exhibited one of the slowest decays of any gamma-ray burst to date. Its broadband properties have been difficult to explain with conventional af…

astro-ph2002

Deep Ly-alpha imaging of two z=2.04 GRB host galaxy fields

J. P. U. Fynbo, P. Moller, B. Thomsen +8

We report on the results of deep narrow-band Ly-alpha, U and I imaging of the fields of two GRBs at z=2.04 (GRB 000301C and GRB 000926). We find that the host galaxy of GRB 000926…