Status of resolve instrument for x-ray astronomy recovery mission (Conference Presentation)
Status of resolve instrument for x-ray astronomy recovery mission (Conference Presentation)
复制标题
X射线天文回收任务解析仪器现状(会议演讲)
DOI:
10.1117/12.2313440
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发表时间:
2018
期刊:
影响因子:
--
通讯作者:
N. Yamasaki
中科院分区:
文献类型:
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作者:
Y. Ishisaki;R. Kelley;H. Akamatsu;H. Awaki;T. Bialas;G. Brown;M. Chiao;E. Costantini;J. Herder;M. Dipirro;M. Eckart;Y. Ezoe;C. Ferrigno;R. Fujimoto;A. Furuzawa;S. Graham;M. Grim;T. Hayashi;A. Hoshino;Y. Ichinohe;R. Iizuka;K. Ishibashi;M. Ishida;K. Ishikawa;C. Kilbourne;S. Kitamoto;S. Koyama;M. Leutenegger;Y. Maeda;D. McCammon;I. Mitsuishi;H. Mori;S. Nakashima;H. Noda;T. Ohashi;T. Okajima;S. Paltani;F. Porter;Kosuke Sato;M. Sawada;H. Seta;P. Shirron;G. Sneiderman;Y. Soong;A. Szymkowiak;Y. Takei;T. Tamagawa;M. Tsujimoto;S. Ueda;C. Vries;S. Yamada;N. Yamasaki
The Resolve instrument onboard the X-ray Astronomy Recovery Mission (XARM) consists of an array of 6x6 silicon-thermistor microcalorimeters cooled down to 50 mK and a high-throughput X-ray mirror assembly with a focal length of 5.6 m. The XARM is a recovery mission of ASTRO-H/Hitomi, and is developed by international collaboration of Japan, USA, and Europe. The Soft X-ray Spectrometer (SXS) onboard Hitomi demonstrated high resolution X-ray spectroscopy of ~ 5 eV FWHM in orbit for most of the microcalorimeter pixels. The Resolve instrument 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 of Hitomi. The energy resolution budget of the microcalorimeters is updated, reflecting the Hitomi SXS results. We report the current status of the Resolve instrument.