activity
19972026
most citedA very energetic supernova associated with the gamma-ray burst of 29 March 2003

1.5k citations · 15.4k across the 209 of their papers we have counts for

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Showing 2003Show all

17 papers · 1 filter

astro-ph2003

The polarization evolution of the optical afterglow of GRB 030329

J. Greiner, S. Klose, K. Reinsch +23

We report 31 polarimetric observations of the afterglow of GRB 030329 with high signal-to-noise and high sampling frequency. The data imply that the afterglow magnetic field has sm…

astro-ph2003★ 116 cited

Evolution of the polarization of the optical afterglow of the gamma-ray burst GRB 030329

J. Greiner, S. Klose, K. Reinsch +23

We report 31 polarimetric observations of the afterglow of GRB 030329 with high signal-to-noise and high sampling frequency. We establish the polarization light curve, detect susta…

astro-ph2003★ 28 cited

X-ray/optical observations of A0535+26/HDE 245770 in quiescence

M. Orlandini, C. Bartolini, S. Campana +10

We present the result of three BeppoSAX observations of the X-ray binary pulsar A0535+26 in its quiescent state. The source is quite well detected up to 200 keV (6 sigma detection…

astro-ph2003★ 19 cited

GRB 030227: the first multiwavelength afterglow of an INTEGRAL GRB

A. J. Castro-Tirado, J. Gorosabel, S. Guziy +39

We present multiwavelength observations of a gamma-ray burst detected by INTEGRAL (GRB 030227) between 5.3 hours and ~1.7 days after the event. Here we report the discovery of a di…

astro-ph2003★ 112 cited

Very high column density and small reddening towards GRB 020124 at z = 3.20

J. Hjorth, P. Møller, J. Gorosabel +27

We present optical and near-infrared observations of the dim afterglow of GRB 020124, obtained between 2 and 68 hours after the gamma-ray burst. The burst occurred in a very faint…

astro-ph2003★ 45 cited

The blue host galaxy of the red GRB 000418

J. Gorosabel, S. Klose, L. Christensen +25

We report on multi-band (UBVRIZJsKs) observations of the host galaxy of the April 18, 2000 gamma-ray burst. The Spectral Energy Distribution (SED) is analysed by fitting empirical…