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Soft x-ray imager (SXI) for Xtend onboard X-Ray Imaging and Spectroscopy Mission (XRISM)

Authors :
Takashi Sako
Jin Sato
Koki Okazaki
Kazunori Asakura
Kazutaka Yamaoka
Hirofumi Noda
Yukino Urabe
Masanobu Ozaki
Makoto Yamauchi
Takeshi Go Tsuru
Masayuki Yoshida
Shotaro Sakuma
Takayoshi Kohmura
Tessei Yoshida
Yusuke Nishioka
Shogo B. Kobayashi
Hideki Uchiyama
Maho Hanaoka
Kumiko K. Nobukawa
Yoshiaki Kanemaru
K. Mori
Tomokage Yoneyama
Kouichi Hagino
Mariko Saito
Isamu Hatsukade
Kengo Hattori
Ayami Ishikura
Toshiyuki Takaki
Junko S. Hiraga
Yuki Amano
Hironori Matsumoto
Hiroyuki Uchida
Hiroshi Nakajima
Hiroshi Tsunemi
Kiyoshi Hayashida
Masayoshi Nobukawa
Hiroshi Murakami
Hiroshi Tomida
Y. Terada
Takaaki Tanaka
Tadayasu Dotani
Hiromichi Okon
Hikari Kashimura
Source :
Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray.
Publication Year :
2020
Publisher :
SPIE, 2020.

Abstract

We report current status of developing Soft X-ray Imager (SXI), the X-ray CCD camera onboard X-Ray Imaging and Spectroscopy Mission (XRISM). Four flight model (FM) CCDs have been selected considering several items including energy resolution at 5.9keV, CTI, dark current, etc. We have also completed calibration campaign for all the FM CCDs. Initial analyses show that the response function for monochromatic X-rays is basically the same as that of Hitomi CCDs. The focal plane including the single-stage Stirling cooler has been assembled. Production of key parts in SXI sensor body such as contamination blocking filter and onboard calibration source has been finished and they are waiting for assemble. The digitized signals of the CCD are corrected step by step before conversion to X-ray energy. We are preparing calibration database for the correction such as CTI, gain, and line redistribution function.

Details

Database :
OpenAIRE
Journal :
Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray
Accession number :
edsair.doi...........8b284bcaef15125922935cd780afbdf9