TY - JOUR
T1 - Screening and selection of XRISM/Xtend flight model CCD
AU - the Xtend team
AU - Yoneyama, Tomokage
AU - Noda, Hirofumi
AU - Hanaoka, Maho
AU - Okazaki, Koki
AU - Asakura, Kazunori
AU - Hayashida, Kiyoshi
AU - Ishikura, Ayami
AU - Sakuma, Shotaro
AU - Hattori, Kengo
AU - Matsumoto, Hironori
AU - Mori, Koji
AU - Kanemaru, Yoshiaki
AU - Sato, Jin
AU - Takaki, Toshiyuki
AU - Uchida, Hiroyuki
AU - Tanaka, Takaaki
AU - Okon, Hiromichi
AU - Amano, Yuki
AU - Tsuru, Takeshi G.
AU - Tomida, Hiroshi
AU - Hiraga, Junko S.
AU - Urabe, Yukino
AU - Nobukawa, Kumiko K.
AU - Saito, Mariko
AU - Nobukawa, Masayoshi
AU - Sako, Takashi
AU - Uchiyama, Hideki
AU - Nakajima, Hiroshi
AU - Kashimura, Akira
AU - Kobayashi, Shogo B.
AU - Hagino, Kouichi
AU - Murakami, Hiroshi
N1 - Funding Information:
This work is supported by Japan Society for the Promotion of Science (JSPS) KAKANHI Grant Numbers 15H02090 , 16H03983 , 18K18767 , 19K21884 , 20H00176 , and 20H01947 .
PY - 2021/1/1
Y1 - 2021/1/1
N2 - X-ray Imaging Spectroscopy Mission (XRISM) is the next Japanese X-ray astronomical satellite to be launched in 2021 Japanese fiscal year. We are developing one of the XRISM instruments “Xtend”, which is an X-ray CCD camera combined with an X-ray telescope, and achieves the wide field of view of 38′×38′ in 0.4–13keV. In 2019, twelve flight-model (FM) candidate CCD chips were fabricated by Hamamatsu Photonics K.K. We conducted screening experiments to examine whether the FM candidates met requirements for the Xtend CCDs, and selected the four FM chips from them. We constructed a screening system, with which we can examine various CCD performances by illuminating characteristic X-ray lines in a ∼0.5–14keV band or optical lights. With this system, all the twelve candidates were confirmed to satisfy the requirements. We then selected four chips with the best performance, in terms of e.g., their charge transfer inefficiencies, energy resolutions, soft X-ray sensitivities, and optical light leakages. In this paper, we report an overview of the screening system, and procedures and results of the screening process.
AB - X-ray Imaging Spectroscopy Mission (XRISM) is the next Japanese X-ray astronomical satellite to be launched in 2021 Japanese fiscal year. We are developing one of the XRISM instruments “Xtend”, which is an X-ray CCD camera combined with an X-ray telescope, and achieves the wide field of view of 38′×38′ in 0.4–13keV. In 2019, twelve flight-model (FM) candidate CCD chips were fabricated by Hamamatsu Photonics K.K. We conducted screening experiments to examine whether the FM candidates met requirements for the Xtend CCDs, and selected the four FM chips from them. We constructed a screening system, with which we can examine various CCD performances by illuminating characteristic X-ray lines in a ∼0.5–14keV band or optical lights. With this system, all the twelve candidates were confirmed to satisfy the requirements. We then selected four chips with the best performance, in terms of e.g., their charge transfer inefficiencies, energy resolutions, soft X-ray sensitivities, and optical light leakages. In this paper, we report an overview of the screening system, and procedures and results of the screening process.
KW - Charge-coupled device
KW - P-channel CCD
KW - X-ray
KW - XRISM
KW - Xtend
UR - http://www.scopus.com/inward/record.url?scp=85091651332&partnerID=8YFLogxK
U2 - 10.1016/j.nima.2020.164676
DO - 10.1016/j.nima.2020.164676
M3 - Article
AN - SCOPUS:85091651332
VL - 985
JO - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
JF - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
SN - 0168-9002
M1 - 164676
ER -