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Status of ART-XC/SRG InstrumentSpectrum Roentgen Gamma (SRG) is an X-ray astrophysical observatory, developed by Russia in collaboration with Germany. The mission will be launched in March 2016 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. The NASA Marshall Space Flight Center (MSFC) is fabricating the flight mirror modules for the ART-XC/SRG. Each mirror module will be aligned with a focal plane CdTe double-sided strip detectors which will operate over the energy range of 6-30 keV, with an angular resolution of less than 1′, a field of view of approximately 34′ and an expected energy resolution of about 10 percent at 14 keV.
Document ID
20140011792
Acquisition Source
Marshall Space Flight Center
Document Type
Conference Paper
Authors
Pavlinsky, M.
(Institute of Space Research Moscow, Russian Federation)
Akimov, V.
(Institute of Space Research Moscow, Russian Federation)
Levin, V.
(Institute of Space Research Moscow, Russian Federation)
Lapshov, I.
(Institute of Space Research Moscow, Russian Federation)
Tkachenko, A.
(Institute of Space Research Moscow, Russian Federation)
Semena, N.
(Institute of Space Research Moscow, Russian Federation)
Buntov, M.
(Institute of Space Research Moscow, Russian Federation)
Glushenko, A.
(Institute of Space Research Moscow, Russian Federation)
Arefiev, V.
(Institute of Space Research Moscow, Russian Federation)
Yaskovich, A.
(Institute of Space Research Moscow, Russian Federation)
Sunyaev, R.
(Institute of Space Research Moscow, Russian Federation)
Churazov, E.
(Institute of Space Research Moscow, Russian Federation)
Gilfanov, M.
(Institute of Space Research Moscow, Russian Federation)
Grebenev, S.
(Institute of Space Research Moscow, Russian Federation)
Sazonov, S.
(Institute of Space Research Moscow, Russian Federation)
Revnivtsev, M.
(Institute of Space Research Moscow, Russian Federation)
Lutovinov, A.
(Institute of Space Research Moscow, Russian Federation)
Molkov, S.
(Institute of Space Research Moscow, Russian Federation)
Kudelin, M.
(Institute of Space Research Moscow, Russian Federation)
Drozdova, T.
(Institute of Space Research Moscow, Russian Federation)
Garanin, S.
(Russian Federal Nuclear Center Russian Federation)
Grigorovich, S.
(Russian Federal Nuclear Center Russian Federation)
Litvin, D.
(Russian Federal Nuclear Center Russian Federation)
Lazarchuk, V.
(Russian Federal Nuclear Center Russian Federation)
Roiz, I.
(Russian Federal Nuclear Center Russian Federation)
Garin, M.
(Russian Federal Nuclear Center Russian Federation)
Babyshkin, V.
(Max-Planck-Inst. fuer Astrophysik Munich, Germany)
Lomakin, I.
(Max-Planck-Inst. fuer Astrophysik Munich, Germany)
Menderov, A.
(Max-Planck-Inst. fuer Astrophysik Munich, Germany)
Moskvinov, D.
(Max-Planck-Inst. fuer Astrophysik Munich, Germany)
Gubarev, M.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Ramsey, B.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Kilaru, K.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
ODell, S. L.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Kolodziejczak, J.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Elsner, R.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
September 17, 2014
Publication Date
June 22, 2014
Subject Category
Astronomy
Report/Patent Number
M14-3776
Meeting Information
Meeting: SPIE Astronomical Telescopes and Instrumentation 2014
Location: Montreal, Quebec
Country: Canada
Start Date: June 22, 2014
End Date: June 27, 2014
Sponsors: International Society for Optical Engineering
Distribution Limits
Public
Copyright
Public Use Permitted.
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