The ART-XC Instrument on board the SRG Mission

被引：3
作者：
Pavlinsky, M. [1 ]
Akimov, V. [1 ]
Levin, V. [1 ]
Lapshov, I. [1 ]
Tkachenko, A. [1 ]
Semena, N. [1 ]
Buntov, M. [1 ]
Glushenko, A. [1 ]
Arefiev, V. [1 ]
Yaskovich, A. [1 ]
Sunyaev, R. [1 ]
Churazov, E. [1 ]
Sazonov, S. [1 ]
Revnivtsev, M. [1 ]
Lutovinov, A. [1 ]
Molkov, S. [1 ]
Kudelin, M. [1 ]
Garanin, S.
Grigorovich, S.
Litvin, D.
Lazarchuk, V.
Roiz, I.
Garin, M.
Babyshkin, V.
Lomakin, I.
Menderov, A.
Moskvinov, D.
Gubarev, M.
Ramsey, B.
Kilaru, K.
O'Dell, S. L.
Elsner, R.
机构：
[1] Space Res Inst, Moscow, Russia
来源：
SPACE TELESCOPES AND INSTRUMENTATION 2012: ULTRAVIOLET TO GAMMA RAY | 2012年 / 8443卷
关键词：
D O I：
10.1117/12.925376
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
Spectrum Roentgen Gamma (SRG) is an X-ray astrophysical observatory, developed by Russia in collaboration with Germany. The mission will be launched in 2014 from Baikonur, by a Zenit rocket with a Fregat booster and placed in a 6-month-period halo orbit around L2. The scientific payload consists of two independent telescopes - a soft-x-ray survey instrument, eROSITA, being provided by Germany and a medium-x-ray-energy survey instrument ART-XC being developed by Russia. ART-XC will consist of seven independent, but co-aligned, telescope modules with seven corresponding cadmium-telluride focal plane detectors. Each will operate over the approximate energy range of 630 keV, with an angular resolution of <1', a field of view of similar to 30' and an energy resolution about 10% at 14 keV. The NASA Marshall Space Flight Center (MSFC) will fabricate some of the mirror modules, to complement others fabricated by VNIIEF in Russia.
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页数：10
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