Search for ultrahigh-energy cosmic gamma-ray bursts on the Baksan underground scintillation telescope

被引：0

作者：

Smirnov, D. V. ^{[1
]}

Petkov, V. B. ^{[1
]}

Karpov, S. N. ^{[1
]}

机构：

[1] Russian Acad Sci, Inst Nucl Res, Moscow 117312, Russia

来源：

ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 2006年 / 32卷 / 01期

关键词：

gamma-ray bursts; high energies; underground experiment;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Based on data from the Baksan underground scintillation telescope ( BUST) for the period 2001-2004, we searched for cosmic gamma-ray bursts (GRBs) at primary photon energies of 0.5 TeV or higher. We obtained constraints on the rate of bursts with durations of 1-10 s for fluences within the range 4.6 x 10(-3)-1.8 x 10(-2) erg cm(-2) in the declination band 30 degrees <= delta <= 80 degrees. We searched for ultrahigh-energy gamma rays from GRBs detected on spacecraft during and within +/- 2 h of the burst. No statistically significant excesses above the background of random coincidences were found. The derived constraints on the ultrahigh-energy gamma-ray fluence during GRBs lie within the range 4.6 x 10(-3)-3.7 x 10(-2) erg cm(-2).

引用

页码：1 / 6

页数：6

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