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

来源：

SPACE TELESCOPES AND INSTRUMENTATION 2018: ULTRAVIOLET TO GAMMA RAY | 2018年 / 10699卷

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.

引用

页数：6

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