Use of a charge-injection technique to improve performance of the Soft X-ray Imager aboard ASTRO-H
Creators
- Nobukawa, Kumiko Kawabata1
- Tsuru, Takeshi Go1
- Nobukawa, Masayoshi1, 2
- Tanaka, Takaaki1
- Uchida, Hiroyuki1
- Tsunemi, Hiroshi3
- Hayashida, Kiyoshi3
- Anabuki, Naohisa3
- Nakajima, Hiroshi3
- Nagino, Ryo3
- Dotani, Tadayasu4
- Ozaki, Masanobu4
- Natsukari, Chikara4
- Tomida, Hiroshi5
- Kimura, Masashi5
- Yamauchi, Makoto6
- Mori, Koji6
- Hatsukade, Isamu6
- Nishioka, Yusuke6
- Kohmura, Takayoshi7
- and others
- 1. Department of Physics, Graduate School of Science, Kyoto University, Kitashirakawa Oiwake-cho, Sakyo-ku, Kyoto 606-8502 (Japan)
- 2. The Hakubi Center for Advanced Research, Kyoto University, Yoshida-Ushinomiya-cho, Sakyo-ku, Kyoto 606-8302 (Japan)
- 3. Department of Earth and Space Science, Graduate School of Science, Osaka University, 1-1 Machikaneyama-cho, Toyonaka, Osaka 560-0043 (Japan)
- 4. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa 252-5210 (Japan)
- 5. ISS Project Science Office, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 2-1 Sengen, Tsukuba, Ibaraki 305-8505 (Japan)
- 6. Department of Applied Physics, University of Miyazaki, 1-1 Gakuen Kibana-dai Nishi, Miyazaki 889-2192 (Japan)
- 7. Physics Department, Kogakuin University, 2665-1, Nakano-cho, Hachioji, Tokyo 192-0015 (Japan)
Description
We are developing the Soft X-ray Imager (SXI), a charge-coupled device (CCD) camera system to be deployed onboard the ASTRO-H satellite. Using an engineering model system in which design specifications were the same as those of the flight model, we measured charge transfer inefficiency (CTI) and the effects of charge trailing. The CCD was irradiated with monochromatic X-rays produced by a radio isotope (55Fe) and X-ray generator using alpha particles from 241Am. We used four targets for the X-ray generator: (C2F4)n, SiO2, Ti, and Ge. Since CTI degrades energy resolution, we adopted the charge-injection technique to the SXI. With this technique, injected charges fill traps, and subsequent signal charges are transferred with less loss of charge. However, the charge-injection technique can cause positional variations in gain on the CCD chip. Thus, we constructed a method for correcting CTI. We also evaluated the charge trailing effect and tested a method for correcting its effects. After applying these corrections to charge injection, variations in gain improved from 0.5% to 0.1% over the CCD chip, and the energy resolution (FWHM) improved from ∼220eV to ∼180eV at 5.9 keV. - Highlights: • We measured CTI and charge trailing in the energy band from <1keV to ∼10keV. • We developed a method for correcting CTI and charge trailing effects. • Our data with high statistics required exponential functions as CTI model. • After applying the corrections, the remaining positional variations over the CCD satisfy requirements for flight operations
Availability note (English)
Available from http://dx.doi.org/10.1016/j.nima.2014.05.091Additional details
Identifiers
- DOI
- 10.1016/j.nima.2014.05.091;
- PII
- S0168-9002(14)00644-5;
Publishing Information
- Journal Title
- Nuclear Instruments and Methods in Physics Research. Section A, Accelerators, Spectrometers, Detectors and Associated Equipment
- Journal Volume
- 765
- Journal Page Range
- p. 269-274
- ISSN
- 0168-9002
- CODEN
- NIMAER
Conference
- Title
- 9. international ''Hiroshima'' symposium on development and application of semiconductor tracking detectors
- Acronym
- HSTD-9 2013
- Dates
- 1-5 Sep 2013
- Place
- Hiroshima (Japan)
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 46125274
- Subject category
- S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ALPHA PARTICLES; AMERICIUM 241; CAMERAS; CHARGE-COUPLED DEVICES; DESIGN; ENERGY RESOLUTION; IMAGES; INJECTION; IRON 55; KEV RANGE 01-10; MONOCHROMATIC RADIATION; SATELLITES; SIGNALS; SILICA; SILICON OXIDES; SOFT X RADIATION
- Descriptors DEC
- ACTINIDE NUCLEI; ALPHA DECAY RADIOISOTOPES; AMERICIUM ISOTOPES; BETA DECAY RADIOISOTOPES; CHALCOGENIDES; CHARGED PARTICLES; ELECTROMAGNETIC RADIATION; ELECTRON CAPTURE RADIOISOTOPES; ENERGY RANGE; EVEN-ODD NUCLEI; HEAVY NUCLEI; INTAKE; INTERMEDIATE MASS NUCLEI; IONIZING RADIATIONS; IRON ISOTOPES; ISOTOPES; KEV RANGE; MINERALS; NUCLEI; ODD-EVEN NUCLEI; OXIDE MINERALS; OXIDES; OXYGEN COMPOUNDS; RADIATIONS; RADIOISOTOPES; RESOLUTION; SEMICONDUCTOR DEVICES; SILICON COMPOUNDS; SPONTANEOUS FISSION RADIOISOTOPES; X RADIATION; YEARS LIVING RADIOISOTOPES
Optional Information
- Copyright
- Copyright (c) 2014 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.