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Screening and selection of XRISM/Xtend flight model CCD.

Authors :
Yoneyama, Tomokage
Noda, Hirofumi
Hanaoka, Maho
Okazaki, Koki
Asakura, Kazunori
Hayashida, Kiyoshi
Ishikura, Ayami
Sakuma, Shotaro
Hattori, Kengo
Matsumoto, Hironori
Mori, Koji
Kanemaru, Yoshiaki
Sato, Jin
Takaki, Toshiyuki
Uchida, Hiroyuki
Tanaka, Takaaki
Okon, Hiromichi
Amano, Yuki
Tsuru, Takeshi G.
Tomida, Hiroshi
Source :
Nuclear Instruments & Methods in Physics Research Section A. Jan2021, Vol. 985, pN.PAG-N.PAG. 1p.
Publication Year :
2021

Abstract

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 3 8 ′ × 3 8 ′ in 0.4–13 keV. 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 –14 keV 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. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
01689002
Volume :
985
Database :
Academic Search Index
Journal :
Nuclear Instruments & Methods in Physics Research Section A
Publication Type :
Academic Journal
Accession number :
147070743
Full Text :
https://doi.org/10.1016/j.nima.2020.164676