抄録
The hard X-ray imager (HXI) is the focal plane detector onboard ASTRO-H to be launched in 2014. By combining with the hard X-ray telescope, the HXI will realize the focusing imaging in the energy range from 5 up to 80 keV. The sensitivity of the HXI for an isolated point source will be two orders of magnitude better compared with previous missions. The hybrid structure composed of four layers of double-sided silicon strip detectors (DSSD) and one layer of cadmium telluride double-sided strip detector (CdTe-DSD) enables high detection efficiency in the hard X-ray band. The DSSD and CdTe-DSD for ASTRO-H have been developed, and their spectral and imaging performances were evaluated. By using two-strip events for the reconstructions of spectra and images, energy resolution of 1.0 keV at 13.9 keV and 2.0 keV at 59.5 keV, and sub-strip spatial resolution were achieved.
本文言語 | English |
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ホスト出版物のタイトル | AIP Conference Proceedings |
ページ | 809-812 |
ページ数 | 4 |
巻 | 1505 |
DOI | |
出版ステータス | Published - 2012 |
イベント | 5th International Meeting on High Energy Gamma-Ray Astronomy - Heidelberg 継続期間: 2012 7月 9 → 2012 7月 13 |
Other
Other | 5th International Meeting on High Energy Gamma-Ray Astronomy |
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City | Heidelberg |
Period | 12/7/9 → 12/7/13 |
ASJC Scopus subject areas
- 物理学および天文学(全般)