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.

引用

页数：10

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