Proceedings of SPIE - The International Society for Optical Engineering 9905 2016年
Hard X-ray imaging polarimeters are developed for the X-ray γ-ray polaeimtery satellite PolariS. The imaging polarimter is scattering type, in which anisotropy in the direction of Compton scattering is employed to measure the hard X-ray (10-80 keV...
SPACE TELESCOPES AND INSTRUMENTATION 2016: ULTRAVIOLET TO GAMMA RAY 9905 2016年
Hard X-ray imaging polarimeters are developed for the X-ray gamma-ray polaeimtery satellite PolariS. The imaging polarimter is scattering type, in which anisotropy in the direction of Compton scattering is employed to measure the hard X-ray (10-80...
Hiroshi Tsunemi Kiyoshi Hayashida Takeshi Go Tsuru Tadayasu Dotani Hiroshi Nakajima Naohisa Anabuki Ryo Nagino Takaaki Tanaka Hiroyuki Uchida Masanobu Ozaki Chikara Natsukari Hiroshi Tomida Shutaro Ueda Masachika Iwai Masayoshi Nobukawa Junko S. Hiraga Takayoshi Kohmura Hiroshi Murakami Koji Mori Makoto Yamauchi Isamu Hatsukade Yusuke Nishioka Aya Bamba Kumiko K. Nobukawa John Doty
SPACE TELESCOPES AND INSTRUMENTATION 2016: ULTRAVIOLET TO GAMMA RAY 9905 2016年
We report here the performance of the SXI on ASTRO-H that was started its operation from March, 02 2016. The SXI consists of 4 CCDs that cover 38' x 38' sky region. They are P-channel back-illumination type CCD with a depletion layer of 200 mu m. ...
PROCEEDINGS OF THE 14TH INTERNATIONAL SYMPOSIUM ON NUCLEI IN THE COSMOS (NIC2016) 2016年
A neutron star (NS) is a natural laboratory to probe the nature of the ultra-dense matter. Its observational parameters, e.g., mass and radius, may constrain the equation of state of the supranuclear matter. Here, we analyzed the thermonuclear X-r...
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