activity
19971999
most citedDiscovery of the peculiar supernova 1998bw in the error box of GRB980425

1.9k citations · 2.2k across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph1999★ 77 cited

The X-ray, Optical and Infrared Counterpart to GRB 980703

P. M. Vreeswijk, T. J. Galama, A. Owens +36

We report on X-ray, optical and infrared follow-up observations of GRB 980703. We detect a previously unknown X-ray source in the GRB error box; assuming a power law decline we fin…

astro-ph1999★ 1 cited

Spectral Energy Distributions and Light Curves of GRB 990123 and its Afterglow

T. J. Galama, M. S. Briggs, R. A. M. J. Wijers +38

Gamma-ray bursts (GRBs) are thought to result from the interaction of an extremely relativistic outflow interacting with a small amount of material surrounding the site of the expl…

astro-ph1998★ 1.9k cited

Discovery of the peculiar supernova 1998bw in the error box of GRB980425

T. J. Galama, P. M. Vreeswijk, J. van Paradijs +42

The discovery of X-ray, optical and radio afterglows of gamma-ray bursts (GRBs) and the measurements of the distances to some of them have established that these events come from G…

astro-ph1998★ 62 cited

The Rapid Decay of the Optical Emission from GRB 980326 and its Possible Implications

Paul J. Groot, Titus J. Galama, Paul M. Vreeswijk

We report the discovery of the optical counterpart to GRB 980326. Its rapid optical decay can be characterized by a power law with exponent -2.10 +/- 0.13 and a constant underlying…

astro-ph1998★ 42 cited

The 1.4 GHz light curve of GRB 970508

T. J. Galama, R. A. M. J. Wijers, M. Bremer +6

We report on Westerbork 1.4 GHz radio observations of the radio counterpart to -ray burst GRB~970508, between 0.80 and 138 days after this event. The 1.4 GHz light curve shows a…

astro-ph1997★ 84 cited

The decay of optical emission from the Gamma-Ray Burst GRB 970228

Titus J. Galama, Paul J. Groot, Jan van Paradijs +6

We present the R_c band light curve of the optical transient (OT) associated with GRB970228, based on re-evaluation of existing photometry. Data obtained until April 1997 suggested…