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The RT-2 Experiment, a low energy gamma-ray telescope, onboard CORONAS-PHOTONsatellite is designed to study the temporal, spectral and spatial properties ofthe hard X-ray solar flares mainly in the energy range of 15 - 100 keV, whichis extendable upto 1000 keV. During the operational period of ~ 9 months, ithas been able to detect a few solar flares and at least four Gamma-Ray Bursts(GRBs). In this paper, we discuss the properties of the GRBs as observed byRT-2 in the energy band of 15 to ~ 1000 keV. We will present the results ofspectral and timing properties of the GRBs (specially for the GRB 090618) usingRT-2 detectors. Temporal analysis suggests that all four GRBs belong to thecategory of long duration bursts.

Nature of GRBs observed by RT-2 on-board CORONAS-PHOTON satellite