In-flight performance of pulse processing system of the ASTRO-H soft x-ray spectrometer-Reference-Cited by-同舟云学术

In-flight performance of pulse processing system of the ASTRO-H soft x-ray spectrometer

Published:2016-07-18 Issue: Volume: Page:
ISSN:0277-786X
Container-title:SPIE Proceedings
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Author:

Ishisaki Yoshitaka¹,Yamada Shinya¹,Seta Hiromi¹,Tashiro Makoto S.²,Takeda Sawako²,Terada Yukikatsu²,Kato Yuka²,Tsujimoto Masahiro³,Koyama Shu³,MItsuda Kazuhisa³,Sawada Makoto⁴,Boyce Kevin R.⁵,Chiao Meng P.⁵,Watanabe Tomomi⁵,Leutenegger Maurice A.⁵,Eckart Megan E.⁵,Porter F. Scott⁵,Kilbourne Caroline A.⁵,Kelley Richard L.⁵

Affiliation:

1. Tokyo Metropolitan Univ. (Japan)

2. Saitama Univ. (Japan)

3. ISAS/JAXA (Japan)

4. Aoyama Gakuin Univ. (Japan)

5. NASA Goddard Space Flight Ctr. (United States)

Publisher

SPIE

Reference9 articles.

1. Takahashi, T. et al., “The astro-h x-ray astronomy satellite,” in [Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray], Proc. SPIE (2016).

2. Takeda, S. et al., “Performance verification and system integration tests of the pulse shape processor for the soft x- ray spectrometer onboard ASTRO-H,” in [Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray], Proc. SPIE 9144, 91445B (July 2014).

3. Development of a Digital Signal Processing System for the X-Ray Microcalorimeter Onboard ASTRO-H (II)

4. The Digital Processing System for the Soft X-Ray Spectrometer Onboard ASTRO-H —The Design and the Performance—

5. Kelley, R. L. et al., “The astro-h high-resolution soft x-ray spectrometer,” in [Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray], Proc. SPIE (2016).

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