Large Area X-ray Proportional Counter instrument on AstroSat

被引:11
|
作者
Yadav, J. S. [1 ]
Agrawal, P. C. [2 ]
Antia, H. M. [1 ]
Manchanda, R. K. [3 ]
Paul, B. [4 ]
Misra, Ranjeev [5 ]
机构
[1] Tata Inst Fundamental Res, Homi Bhabha Rd, Bombay 400005, Maharashtra, India
[2] Univ Mumbai, UM DAE Ctr Excellence Basic Sci, Bombay 400098, Maharashtra, India
[3] Univ Mumbai, Bombay 400098, Maharashtra, India
[4] Raman Res Inst, Dept Astron & Astrophys, Bengaluru 560080, India
[5] Interuniv Ctr Astron & Astrophys, Pune 411007, Maharashtra, India
来源
CURRENT SCIENCE | 2017年 / 113卷 / 04期
关键词
Energy- and time-resolution; payloads; space observatory; X-ray sources; GRS; 1915+105;
D O I
10.18520/cs/v113/i04/591-594
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Large Area X-ray Proportional Counter (LAXPC) is one of the major AstroSat payloads. The instrument will provide high time-resolution X-ray observations in 3-80 keV energy band with moderate energy resolution. A cluster of three co-aligned identical LAXPC detectors is used in AstroSat to provide large collection area of more than 6000 sq. cm. The large detection volume (15 cm depth) filled with xenon gas at similar to 2 atm pressure, results in detection efficiency greater than 50% above 30 keV. With its broad energy range and fine-time resolution (10 mu s), LAXPC instrument is well suited for timing and spectral studies of a wide variety of known and transient X-ray sources in the sky. We have done extensive calibration of all LAXPC detectors using radioactive sources as well as GEANT4 simulation of LAXPC detectors. We describe in brief some of the results obtained during the payload verification phase along with LAXPC capabilities.
引用
收藏
页码:591 / 594
页数:4
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