Papers

Peer-reviewed
2016

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

SPACE TELESCOPES AND INSTRUMENTATION 2016: ULTRAVIOLET TO GAMMA RAY
  • Yoshitaka Ishisaki
  • Shinya Yamada
  • Hiromi Seta
  • Makoto S. Tashiro
  • Sawako Takeda
  • Yukikatsu Terada
  • Yuka Kato
  • Masahiro Tsujimoto
  • Shu Koyama
  • Kazuhisa Mitsuda
  • Makoto Sawada
  • Kevin R. Boyce
  • Meng P. Chiao
  • Tomomi Watanabe
  • Maurice A. Leutenegger
  • Megan E. Eckart
  • F. Scott Porter
  • Caroline A. Kilbourne
  • Richard L. Kelley
  • Display all

Volume
9905
Number
Language
English
Publishing type
Research paper (international conference proceedings)
DOI
10.1117/12.2234222
Publisher
SPIE-INT SOC OPTICAL ENGINEERING

We summarize results of the initial in-orbit performance of the pulse shape processor (PSP) of the soft x-ray spectrometer instrument onboard ASTRO-H (Hitomi). Event formats, kind of telemetry, and the pulse processing parameters are described, and the parameter settings in orbit are listed. PSP was powered-on two days after launch, and the event threshold was lowered in orbit. PSP worked fine in orbit, and there were no memory error nor SpaceWire communication error until the break-up of spacecraft. Time assignment, electrical crosstalk, and the event screening criteria are studied. It is confirmed that the event processing rate at 100% CPU load is similar to 200 c/s/array, compliant with the requirement on PSP.

Link information
DOI
https://doi.org/10.1117/12.2234222
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000387731500114&DestApp=WOS_CPL
ID information
  • DOI : 10.1117/12.2234222
  • ISSN : 0277-786X
  • Web of Science ID : WOS:000387731500114

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