Deep infrared imaging of the putative X-ray counterpart to GRB920501

Details Deep infrared imaging of the putative X-ray counterpart to GRB920501 Deep infrared imaging of the putative X-ray counterpart to GRB920501

Aug 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..384..589b&link_type=abstract

Gamma-ray bursts: 3rd Huntsville symposium. AIP Conference Proceedings, Volume 384, pp. 589-593 (1996).

Physics

2

Gamma-Ray Sources, Gamma-Ray Bursts, Near Infrared

Scientific paper

If the quiescent X-ray counterpart found in the May 1, 1992 error box is truly associated with the gamma-ray burst, then it offers the best current hope of identifying the origin of these events. In an effort to discover the nature of the X-ray source, we have taken deep JHK images of the X-ray error circle using the Near Infrared Camera at the W. M. Keck Observatory. We tentatively conclude that the X-ray source is associated with an early-type galaxy which we have found in the error box.

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