A report on the XIS calibration of the 2 × 2 mode and window option and the current status of the XIS NXB database

• 池上, 嘉夫

• 森, 浩二

• 青山, 翔一

• 加藤, 豪

• 木村, 結樹

• 石崎, 良則

• 小川, 和輝

• 内山, 秀樹

• 小澤, 碧

• 松本, 浩典

• 鶴, 剛

• 小山, 勝二

• 常深, 博

• 堂谷, 忠靖

• 尾崎, 正伸

• 馬場, 彩

• 辻本, 匡弘

• 幸村, 孝由

• 北本, 俊二

• 村上, 弘志

• Ikegami, Yoshio

• Mori, Koji

• Aoyama, Shoichi

• Kimura, Shoichi

• Samukawa, Maina

• Yamashita, Toshiya

• Kato, Takeshi

• Kimura, Yuki

• Ishizaki, Yoshinori

• Ogawa, Kazuki

• Uchiyama, Hideki

• Ozawa, Midori

• Matsumoto, Hironori

• Tsuru, Takeshi Go

• Koyama, Katsuji

• Hayashida, Kiyoshi

• Tsunemi, Hiroshi

• Dotani, Tadayasu

• Ozaki, Masanobu

• Bamba, Aya

• Tsujimoto, Masahiro

• Kohmura, Takayoshi

• Kitamoto, Shunji

• Murakami, Hiroshi

• SUZAKU XIS team

抄録

The 3rd Suzaku international Conference "Energetic Cosmos : from Suzaku to ASTRO-H" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan

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.

著者人数: 25人(含チーム1)

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

資料番号: AA0064574159

レポート番号: JAXA-SP-09-008E

収録刊行物

• 宇宙航空研究開発機構特別資料: = JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H

  宇宙航空研究開発機構特別資料: = JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H JAXA-SP-09-008E 414-415, 2010-02-26

  宇宙航空研究開発機構

キーワード

• instrumentation: detectors - methods: data analysis - X-ray CCDs

詳細情報

• CRID: 1050855511172143744
• NII論文ID: 120006828561
• NII書誌ID: AA11984031
• ISSN: 1349113X
• Web Site: http://id.nii.ac.jp/1696/00005085/
• 本文言語コード: en
• 資料種別: conference paper
• データソース種別:
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