Multifrequency Observations of Gamma-Ray Burst
arXiv:astro-ph/9510015
Abstract
Neither a flaring nor a quiescent counterpart to a gamma-ray burst has yet been convincingly identified at any wavelength region. The present status of the search for counterparts of classical gamma-ray bursts is given. Particular emphasis is put on the search for flaring counterparts, i.e. emission during or shortly after the gamma-ray emission.
10 pages compressed and uuencoded postscript, including 1 figure Invited talk given at the Frascati Workshop 1995 on the "Multifrequency behaviour of high-energy cosmic sources", Vulcano, May 1995 (to appear in Mem. S. A. It.)