S. Golenetskii

TL;DR: In this article, the temporal structure, fluxes, energy spectra and coordinates of the sources of gamma-ray bursts detected in the KONUS experiment on Venera 11 andVenera 12 space probes were presented.

TL;DR: Observations of the extraordinarily bright prompt optical and γ-ray emission of GRB 080319B that provide diagnostics within seconds of its formation, followed by broadband observations of the afterglow decay that continued for weeks.

TL;DR: In this article, the γ-ray burst detector Konus was used to detect hard X-ray bursts from the same source on 5 and 6 March, 1979, and the burst of 5 March was very intense, particularly in the initial phase and the second burst on 6 March was considerably weaker.

TL;DR: In this paper, the authors report on an even more intense burst on August 27, 1998, from a different soft gamma repeater, which displayed a hard energy spectrum at its peak, and was followed by a ~300 s long tail with a soft energy spectrum and a dramatic 5.16 s period.

TL;DR: In this paper, the authors reported the detection of an even more intense burst from a different soft γ-ray repeater, which was characterized by "hard" γ rays at its peak, followed by a tail 300's long with a soft spectrum and a clear periodicity of 5.16's.