The Astro-H soft X-ray mirror

David Robinson, T. Okajima, P. Serlemitsos, Y. Soong
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Abstract

The Astro-H is led by the Japanese Space Agency (JAXA) in collaboration with many other institutions including the NASA Goddard Space Flight Center. Goddard's contributions include two soft X-ray telescopes (SXTs). The telescopes have an effective area of 562 cm2 at 1 keV and 425 cm2 at 6 keV with an image quality requirement of 1.7 arc-minutes half power diameter (HPD). The engineering model has demonstrated 1.1 arc-minutes HPD error. The design of the SXT is based on the successful Suzaku mission mirrors with some enhancements to improve the image quality. Two major enhancements are bonding the X-ray mirror foils to alignment bars instead of allowing the mirrors to float, and fabricating alignment bars with grooves within 5 microns of accuracy. An engineering model SXT was recently built and subjected to several tests including vibration, thermal, and X-ray performance in a beamline. Several lessons were learned during this testing that will be incorporated in the flight design. Test results and optical performance are discussed, along with a description of the design of the SXT.
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Astro-H软x射线镜
Astro-H由日本航天局(JAXA)领导,与包括美国宇航局戈达德太空飞行中心在内的许多其他机构合作。戈达德的贡献包括两个软x射线望远镜(sxt)。该望远镜在1 keV时有效面积为562 cm2,在6 keV时有效面积为425 cm2,成像质量要求为1.7弧分半功率直径(HPD)。工程模型的HPD误差为1.1角分。SXT的设计基于成功的Suzaku任务镜,并进行了一些改进以提高图像质量。两个主要的改进是将x射线反射镜箔粘合到对准棒上,而不是让反射镜漂浮,以及制造精度在5微米以内的凹槽对准棒。最近建立了一个工程模型SXT,并进行了多次测试,包括振动、热学和光束线中的x射线性能。在这次测试中吸取了一些教训,这些教训将被纳入飞行设计中。讨论了测试结果和光学性能,并对SXT的设计进行了描述。
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