On-ground calibration of the ART-XC/SRG instrument

被引:1
|
作者
Tkachenko, A. [1 ]
Pavlinsky, M. [1 ]
Lapshov, I. [1 ]
Levin, V. [1 ]
Akimov, V. [1 ]
Krivchenko, A. [1 ]
Rotin, A. [1 ]
Kuznetsova, M. [1 ]
Semena, N. [1 ]
Semena, A. [1 ]
Serbinov, D. [1 ]
Krivonos, R. [1 ]
Shtykovsky, A. [1 ]
Yascovich, A. [1 ]
Oleinikov, V. [1 ]
Glushenko, A. [1 ]
Mereminsky, I. [1 ]
Molkov, S. [1 ]
Sazonov, S. [1 ]
Arefiev, V. [1 ]
机构
[1] Space Res Inst, Moscow, Russia
基金
俄罗斯科学基金会;
关键词
MIRROR MODULES;
D O I
10.1117/12.2312094
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Astronomical Roentgen Telescope - X-ray Concentrator (ART-XC) is a medium X-ray instrument with operating energy range 4-30 keV which will be launched onboard the Spectrum Roentgen Gamma (SRG) mission. ART-XC consists of seven co-aligned mirror modules coupled with seven focal plane CdTe double-sided strip detectors. The mirror modules were fabricated and calibrated at the NASA Marshall Space Flight Center (MSFC). The Russian Space Research Institute (IKI) developed and tested the X-ray detectors. Flight mirror modules and detector units were integrated into the ART-XC instrument in 2016. For more detailed studies we have used the spare mirror module and spare detector unit. We present some results of the on-ground calibration of the ART-XC spare detector unit without a mirror system and estimation of the detector efficiency.
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页数:6
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