Status of ART-XC / SRG instrument

M. Pavlinsky; V. Akimov; V. Levin; A. Krivchenko; A. Rotin; M. Kuznetsova; I. Lapshov; A. Tkachenko; N. Semena; M. Buntov; A. Glushenko; V. Arefiev; A. Yaskovich; S. Grebenev; S. Sazonov; M. Revnivtsev; A. Lutovinov; S. Molkov; R. Krivonos; D. Serbinov; M. Kudelin; T. Drozdova; S. Voronkov; R. Sunyaev; E. Churazov; M. Gilfanov; V. Babyshkin; I. Lomakin; A. Menderov; M. Gubarev; B. Ramsey; K. Kilaru; S. L. O’Dell; J. Kolodziejczak; R. Elsner; V. Zavlin; D. Swartz

doi:10.1117/12.2190184

4 September 2015 Status of ART-XC / SRG instrument

M. Pavlinsky, V. Akimov, V. Levin, A. Krivchenko, A. Rotin, M. Kuznetsova, I. Lapshov, A. Tkachenko, N. Semena, M. Buntov, A. Glushenko, V. Arefiev, A. Yaskovich, S. Grebenev, S. Sazonov, M. Revnivtsev, A. Lutovinov, S. Molkov, R. Krivonos, D. Serbinov, M. Kudelin, T. Drozdova, S. Voronkov, R. Sunyaev, E. Churazov, M. Gilfanov, V. Babyshkin, I. Lomakin, A. Menderov, M. Gubarev, B. Ramsey, K. Kilaru, S. L. O’Dell, J. Kolodziejczak, R. Elsner, V. Zavlin, D. Swartz

Author Affiliations +

Proceedings Volume 9603, Optics for EUV, X-Ray, and Gamma-Ray Astronomy VII; 96030C (2015) https://doi.org/10.1117/12.2190184
Event: SPIE Optical Engineering + Applications, 2015, San Diego, California, United States

Abstract

Spectrum Roentgen Gamma (SRG) is an X-ray astrophysical observatory, developed by Russia in collaboration with Germany. The mission will be launched in beginning 2017 from Baikonur 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 ART-XC flight mirror modules has been developed and fabricated at the NASA Marshall Space Flight Center (MSFC). Each mirror module will be aligned with a focal plane CdTe double-sided strip detector which will operate over the energy range of 6−30 keV, with an angular resolution of <1′, a field of view of ~34′ and an expected energy resolution of about 12% at 14 keV. The current status of the ART-XC/SRG instrument will be present.

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M. Pavlinsky, V. Akimov, V. Levin, A. Krivchenko, A. Rotin, M. Kuznetsova, I. Lapshov, A. Tkachenko, N. Semena, M. Buntov, A. Glushenko, V. Arefiev, A. Yaskovich, S. Grebenev, S. Sazonov, M. Revnivtsev, A. Lutovinov, S. Molkov, R. Krivonos, D. Serbinov, M. Kudelin, T. Drozdova, S. Voronkov, R. Sunyaev, E. Churazov, M. Gilfanov, V. Babyshkin, I. Lomakin, A. Menderov, M. Gubarev, B. Ramsey, K. Kilaru, S. L. O’Dell, J. Kolodziejczak, R. Elsner, V. Zavlin, and D. Swartz "Status of ART-XC / SRG instrument", Proc. SPIE 9603, Optics for EUV, X-Ray, and Gamma-Ray Astronomy VII, 96030C (4 September 2015); https://doi.org/10.1117/12.2190184

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