Resolve Instrument on X-ray Astronomy Recovery Mission (XARM)

Resolve Instrument on X-ray Astronomy Recovery Mission (XARM)
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DOI:
10.1007/s10909-018-1913-4
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发表时间:
2018-12
影响因子:
2
通讯作者:
Y. Ishisaki;Y. Ezoe;S. Yamada;Y. Ichinohe;R. Fujimoto;Y. Takei;S. Yasuda;M. Ishida;N. Yamasaki;Y. Maeda;M. Tsujimoto;R. Iizuka;S. Koyama;H. Noda;T. Tamagawa;M. Sawada;K. Sato;S. Kitamoto;A. Hoshino;G. Brown;M. Eckart;T. Hayashi;R. Kelley;C. Kilbourne;M. Leutenegger;H. Mori;T. Okajima;F. Porter;Y. Soong;D. McCammon;A. Szymkowiak;The Xarm Resolve Team
Y. Ishisaki;Y. Ezoe;S. Yamada;Y. Ichinohe;R. Fujimoto;Y. Takei;S. Yasuda;M. Ishida;N. Yamasaki;Y. Maeda;M. Tsujimoto;R. Iizuka;S. Koyama;H. Noda;T. Tamagawa;M. Sawada;K. Sato;S. Kitamoto;A. Hoshino;G. Brown;M. Eckart;T. Hayashi;R. Kelley;C. Kilbourne;M. Leutenegger;H. Mori;T. Okajima;F. Porter;Y. Soong;D. McCammon;A. Szymkowiak;The Xarm Resolve Team
中科院分区:
物理与天体物理3区
文献类型:
--
作者:
Y. Ishisaki;Y. Ezoe;S. Yamada;Y. Ichinohe;R. Fujimoto;Y. Takei;S. Yasuda;M. Ishida;N. Yamasaki;Y. Maeda;M. Tsujimoto;R. Iizuka;S. Koyama;H. Noda;T. Tamagawa;M. Sawada;K. Sato;S. Kitamoto;A. Hoshino;G. Brown;M. Eckart;T. Hayashi;R. Kelley;C. Kilbourne;M. Leutenegger;H. Mori;T. Okajima;F. Porter;Y. Soong;D. McCammon;A. Szymkowiak;The Xarm Resolve Team

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X射线天文学恢复使命(XARM)是ASTRO-H/Hitomi的恢复使命,预计最早将于2020财年发射。XARM上的Resolve仪器包括一个冷却到50 mK的6 × 6硅热敏电阻微量热计阵列和一个焦距为5.6 m的高通量X射线镜组件。Hitomi于2016年2月发射进入轨道,并观察了几个天体,尽管Hitomi的运行于2016年4月终止。Hitomi上的软X射线光谱仪(SXS)展示了轨道上大部分像素的高分辨率X射线光谱,约为5 eV FWHM。Resolve仪器计划主要是Hitomi SXS和软X射线望远镜设计的副本,尽管计划根据从Hitomi吸取的教训进行一些更改。我们报告的SXS性能和解决仪器的状态的简要总结。
The X-ray Astronomy Recovery Mission (XARM) is a recovery mission of ASTRO-H/Hitomi, which is expected to be launched in Japanese Fiscal Year of 2020 at the earliest. TheResolveinstrument on XARM consists of an array of 6 × 6 silicon-thermistor microcalorimeters cooled down to 50 mK and a high-throughput X-ray mirror assembly with the focal length of 5.6 m.Hitomiwas launched into orbit in February 2016 and observed several celestial objects, although the operation ofHitomiwas terminated in April 2016. The soft X-ray spectrometer (SXS) on Hitomi demonstrated high-resolution X-ray spectroscopy of ~ 5 eV FWHM in orbit for most of the pixels. TheResolveinstrument is planned to mostly be a copy of the Hitomi SXS and soft X-ray telescope designs, though several changes are planned based on the lessons learned fromHitomi. We report a brief summary of the SXS performance and the status of the Resolve instrument.