Analysis of the NGXO telescope X-ray Hartmann data

被引：3

作者：

Saha, Timo T. ^{[1
]}

Chan, Kai-Wing ^{[2
,3
]}

Mazzarella, James R. ^{[4
]}

McClelland, Ryan S. ^{[1
]}

Solly, Peter M. ^{[4
]}

Zhang, William W. ^{[1
]}

Burwitz, Vadim ^{[5
]}

Hartner, Gisela ^{[5
]}

La Caria, Marlis-Madeleine ^{[5
]}

Pelliciari, Carlo ^{[5
]}

机构：

[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

[2] Ctr Res & Explorat Space Sci & Technol, Baltimore, MD 21250 USA

[3] Univ Maryland Baltimore Cty, Baltimore, MD 21250 USA

[4] Stinger Ghaffarian Technol Inc, Greenbelt, MD 20770 USA

[5] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany

来源：

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

基金：

欧盟地平线“2020”;

关键词：

X-ray optics; X-ray telescopes; segmented mirrors; X-ray testing;

D O I：

10.1117/12.2312243

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Next Generation X-ray Optics (NGXO) team at the Goddard Space Flight Center (GSFC) has been developing a new silicon-based grazing incidence mirror technology for future high resolution X-ray astronomical missions. Recently, the GSFC team completed the construction of first few mirror modules that contain one pair of mirrors. One of the mirror pairs was tested in GSFC 600-m long beamline facility and PANTER (Neuried, Germany) 120-m long X-ray beamline facility. Both full aperture X-ray tests, Hartmann tests, and focal plane sweeps were completed. In this paper we present the data analysis process and compare the results from our models to measured X-ray centroid data, X-ray performance data, and out of focus images of the mirror pair.

引用

页数：10

共 9 条

[1]

Burwitz V., 2017, P SOC PHOTO-OPT INS

[2]

Chan K.-W., 2018, P SPIE, V10699

[3]

Chan Kai-Wing, 2017, P SOC PHOTO-OPT INS, V10399

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Colella, D ;

Hadjimichael, T ;

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Saha, T ;

Zhang, W .

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[5] Design and analysis of an x-ray mirror assembly using the meta-shell approach [J].

McClelland, Ryan S. ;

Bonafede, Joseph A. ;

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Solly, Peter M. ;

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SPACE TELESCOPES AND INSTRUMENTATION 2016: ULTRAVIOLET TO GAMMA RAY, 2016, 9905

[6]

Riveros R. E., 2017, P SOC PHOTO-OPT INS

[7]

Riveros R. E., 2018, P SPIE, V10699P

[8]

Zhang W. W., 2017, P SOC PHOTO-OPT INS

[9]

Zhang William W., 2018, P SPIE, V10699

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