Debnath 2013 印度太阳卫星CORONAS-PHOTON看到了4个伽马暴

主要内容:
分别是 GRB 090618 , GRB 090820, GRB 090926A, and GRB 090929A (别的卫星也看到了的）

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Title:		Nature of GRBs observed by RT-2 on-board CORONAS-PHOTON satellite
Authors:		Debnath, D.; Nandi, A.; Chakrabarti, S. K.; Katoch, T. B.; Rao, A. R.
Affiliation:		AA(Indian Centre for Space Physics, Chalantika 43, Garia Station Rd., Kolkata 700084, India) AB(Space Astronomy Group, ISAC, HAL Airport Road, Bangalore 560017, India) AC(Indian Centre for Space Physics, Chalantika 43, Garia Station Rd., Kolkata 700084, India; S. N. Bose National Center for Basic Sciences, JD-Block, Salt Lake, Kolkata 700098, India) AD(Space Astronomy Group, ISAC, HAL Airport Road, Bangalore 560017, India; Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai) AE(Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai) 400005, India
Publication:		Astronomical Society of India Conference Series, Vol. 5, p. 91
Publication Date:		00/2012
Origin:		BASI
Keywords:		gamma-ray burst:general, instrumentation:detectors, supernovae:general
Bibliographic Code:		2012ASInC...5...91D

Abstract

The RT-2 Experiment, a low energy gamma-ray telescope, on-board CORONAS-PHOTON satellite is designed to study the temporal, spectral and spatial properties of the hard X-ray solar flares mainly in the energy range of 15 - 100 keV, which is extendable upto 1000 keV. During the operational period of ˜ 9 months, it has 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 by RT-2 in the energy band of 15 to ˜1000 keV. We will present the results of spectral and timing properties of the GRBs (specially for the GRB 090618) using RT-2 detectors. Temporal analysis suggests that all four GRBs belong to the category of long duration bursts.

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