ART-XC/SRG: Status of the x-ray optics development

被引：7
|
作者：
Gubarev, M. [1 ]
Ramsey, B. [1 ]
Elsner, R. [1 ]
O'Dell, S. [1 ]
Kolodziejczak, J. [1 ]
McCracken, J. [1 ]
Zavlin, V. [2 ]
Swartz, D. [2 ]
Kilaru, K. [2 ]
Atkins, C. [3 ]
Pavlinskiy, M. [4 ]
Tkachenko, A. [4 ]
Lapshov, I. [4 ]
机构：
[1] NASA, George C Marshall Space Flight Ctr, Huntsville, AL 35812 USA
[2] NASA, George C Marshall Space Flight Ctr, Univ Space Res Assoc, Huntsville, AL 35812 USA
[3] Univ Alabama, Huntsville, AL 35899 USA
[4] Space Res Inst, Moscow, Russia
来源：
SPACE TELESCOPES AND INSTRUMENTATION 2014: ULTRAVIOLET TO GAMMA RAY | 2014年 / 9144卷
关键词：
Spectrum-Rontgen-Gamma; Astronomical Roentgen Telescope - X-ray Concentrator; x-ray optics; electroform nickel optics;
D O I：
10.1117/12.2056813
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The Astronomical Roentgen Telescope (ART) instrument is a hard-x-ray instrument with energy response up to 30 keV that is to be launched on board of the Spectrum Roentgen Gamma (SRG) Mission. The instrument consists of seven identical mirror modules coupled with seven CdTe strip focal-plane detectors. The mirror modules are being developed at the Marshall Space Flight Center (MSFC.) Each module has similar to 65 sq. cm effective area and an on-axis angular resolution of 30 arcseconds half power diameter (HPD) at 8 keV. The current status of the mirror module development and testing will be presented.
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页数：6
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