Ray-tracing simulation and in-orbit performance of the ASTRO-H hard X-ray telescope (HXT)

HXT Team

研究成果: Conference contribution

1 引用 (Scopus)

抜粋

A ray-trace simulation code for the Hard X-ray Telescope (HXT) on board the Hitomi (ASTRO-H) satellite is being developed. The half power diameter and effective area simulated based on the code are consistent with ground measurements within 10%. The HXT observed the pulsar wind nebula G21.5-0.9 for 105 ksec. We confirmed that the encircled energy function and the half power diameter obtained from the data are consistent with the ground measurements.

元の言語English
ホスト出版物のタイトルSpace Telescopes and Instrumentation 2016
ホスト出版物のサブタイトルUltraviolet to Gamma Ray
編集者Jan-Willem A. den Herder, Tadayuki Takahashi, Marshall Bautz
出版者SPIE
ISBN(電子版)9781510601895
DOI
出版物ステータスPublished - 01-01-2016
イベントSpace Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray - Edinburgh, United Kingdom
継続期間: 26-06-201601-07-2016

出版物シリーズ

名前Proceedings of SPIE - The International Society for Optical Engineering
9905
ISSN(印刷物)0277-786X
ISSN(電子版)1996-756X

Other

OtherSpace Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray
United Kingdom
Edinburgh
期間26-06-1601-07-16

    フィンガープリント

All Science Journal Classification (ASJC) codes

  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics
  • Computer Science Applications
  • Applied Mathematics
  • Electrical and Electronic Engineering

これを引用

HXT Team (2016). Ray-tracing simulation and in-orbit performance of the ASTRO-H hard X-ray telescope (HXT). : J-W. A. den Herder, T. Takahashi, & M. Bautz (版), Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray [990541] (Proceedings of SPIE - The International Society for Optical Engineering; 巻数 9905). SPIE. https://doi.org/10.1117/12.2232135