The cosmological gamma-ray burst (GRB) phenomenon is reviewed. The broad observational facts and empirical phenomenological relations of the GRB prompt emission and afterglow are outlined. A well-tested, successful fireball shock model is introduced in a pedagogical manner. Several important uncertainties in the current understanding of the phenomenon are reviewed, and prospects of how future experiments and extensive observational and theoretical efforts may address these problems are discussed.

pdf/gamma-ray-bursts-progress-problems-prospects-3h1xc90c2e.pdf

Gamma-Ray Bursts: Progress, Problems & Prospects

: The existence of either pre- or post-burst emission can provide substantial new information about the burst source and its local environment. We have data from several events serendipitously in or near the OSSE field of view at the time of the burst. We present pre- and post-burst flux limits from one such event, GRB 940301. The OSSE data for other periods when scheduled observations have included burst locations will enable us to search for pre- and post- burst emission on many time scales.

OSSE Limits on Pre- and Post-Burst Emission (Preprint)

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OSSE Limits on Pre- and Post-Burst Emission (Preprint)