Abstract
We report on the status of our search for X-ray afterglows of gamma-ray bursts (GRBs) using the ROSAT all-sky survey (RASS) data. The number of potential X-ray afterglow candidates with respect to the expected number of beamed GRBs allows to constrain the relative beaming angles of GRB emission and afterglow emission at about 1-5 hrs after the GRB.
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APA
Greiner, J., Voges, W., Boller, T., & Hartmann, D. (1999). Search for GRB afterglows in the ROSAT all-sky survey. Astronomy and Astrophysics Supplement Series. EDP Sciences. https://doi.org/10.1051/aas:1999300
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