Graduate University for Advanced Studies School of Physical Sciences
Japan Aerospace Exploration Agency Institute of Space and Astronautical Science
Japan Aerospace Exploration Agency Institute of Space and Astronautical Science
Japan Aerospace Exploration Agency Institute of Space and Astronautical Science
Tokyo Institute of Technology Graduate School of Science and Engineering
University of Tokyo Graduate School of Science
University of Tokyo Graduate School of Science
Japan Aerospace Exploration Agency Institute of Space and Astronautical Science
出版者
宇宙航空研究開発機構宇宙科学研究本部
出版者（英）
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA/ISAS)
雑誌名
第37回月・惑星シンポジウム
雑誌名(英)
Proceedings of the 37th ISAS Lunar and Planetary Symposium
ページ
263 - 266
発行年
2004-02
抄録（英）
HAYABUSA (MUSES-C) spacecraft was launched by the fifth M-V launch vehicle on 9 May 2003. The XRS onboard HAYABUSA has observed X-ray sources such as, supernova remnants, X-ray binaries and cosmic X-ray background for in-flight calibration and scientific observation. This paper shows results of X-ray background (XRB) observations, and introduces its scientific rationale. A model of XRB spectrum is continuum as, power-law, absorbed power-law, and constant. The XRS observed spectra is roughly consistent with the predicted model.
Cruising observation with XRS onboard HAYABUSA
