Department of Applied Physics, University of Miyazaki
Department of Applied Physics, University of Miyazaki
Department of Applied Physics, University of Miyazaki
Department of Applied Physics, University of Miyazaki
Department of Applied Physics, University of Miyazaki
Department of Applied Physics, University of Miyazaki
Department of Applied Physics, University of Miyazaki
Department of Applied Physics, University of Miyazaki
Department of Applied Physics, University of Miyazaki
Department of Applied Physics, University of Miyazaki
Department of Physics, Graduate School of Science, Kyoto University
Department of Physics, Graduate School of Science, Kyoto University
Department of Physics, Graduate School of Science, Kyoto University
Department of Physics, Graduate School of Science, Kyoto University
Department of Physics, Graduate School of Science, Kyoto University
Department of Earth and Space Science, Graduate School of Science, Osaka University
Department of Earth and Space Science, Graduate School of Science, Osaka University
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA)
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA)
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA)
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA)
Physics Department, Kogakuin University
Department of Physics, Faculty of Science, Rikkyo University
Department of Physics, Faculty of Science, Rikkyo University
SUZAKU XIS team
出版者
宇宙航空研究開発機構
出版者（英）
Japan Aerospace Exploration Agency (JAXA)
雑誌名
宇宙航空研究開発機構特別資料:
雑誌名(英)
JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H
巻
JAXA-SP-09-008E
ページ
414 - 415
発行年
2010-02-26
会議概要（会議名, 開催地, 会期, 主催者等）（英）
The 3rd Suzaku international Conference "Energetic Cosmos : from Suzaku to ASTRO-H" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan
抄録（英）
We report the XIS calibration on the data taken with the 2 x 2 mode and window option and the current status of the XIS Non-X-ray Background (NXB) database. The 2 x 2 mode and window option are useful for bright source observations to avoid telemetry saturation and event pile-up. The NXB database provides the best-estimated NXB spectrum for any specific observations obtained with the standard mode (Normal-Clock with no Window or Burst and 5 x 5(sub -) (3 x 3(sub -) Editing mode). The data taken with the 2 x 2 mode in the "SCI-off" era are fully calibrated, and there is no practical difference from those taken with the standard mode. A calibration study for the data taken with the 2 x 2 mode in the "SCI-on" era is on-going. The calibration for the data taken with the window option was significantly improved in the HEASOFT 6.6.2 released at 2009 April 1st. In the comparison with the standard-mode data, the gain difference around 6 keV becomes less than 10 and 15 eV in XIS 0,3 and XIS 1, respectively. We have been updating the NXB database every half a year. There is no drastic change in the light curves, but steady approximately 4 % year(sup -1) level increase and decrease are found in those of XIS 0,3 and XIS 1, respectively.
内容記述
著者人数: 25人(含チーム1)
内容記述（英）
Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science
Number of authors: 25
A report on the XIS calibration of the 2 × 2 mode and window option and the current status of the XIS NXB database
64574159.pdf
(891.69KB)
