Search for an Optical Counterpart of the Source of GRB 911001

Details Search for an Optical Counterpart of the Source of GRB 911001 Search for an Optical Counterpart of the Source of GRB 911001

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apj...446..357k&link_type=abstract

Astrophysical Journal v.446, p.357

Other

7

Gamma Rays: Bursts, Stars: Individual Constellation Name: X Draconis, Stars: Novae, Cataclysmic Variables, Stars: Variables: Other

Scientific paper

The positional error box of GRB 911001 is centered in the north ecliptic pole field (Fishman et al. 1994) which was extensively observed with the Tautenburg Schmidt telescope between 1990 and 1992 (more than 100 Schmidt plates). The plate taken nearest to the time after the occurrence of the burst is from 1991 October 2. We report here on the results of a search for variable objects within the error box of GRB 911001. We detected four objects, among them a possibly so far unknown cataclysmic variable. At the time of the occurrence of the GRB this object was presumably in a maximum state.

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