SPICA Mid-infrared Instrument Calibration plan

Material type: 文書・図像類

Author: 山岸, 光義ほか

Publisher: 宇宙航空研究開発機構(JAXA)

Publication date: 2022-02-28

Material Format: Digital

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Note (General)：: Preparatory works for the calibration of SPICA Mid-infrared Instrument (SMI) are reported. We focus on three calibration items, flux, wavelength, and ...

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Material Type: 文書・図像類
Title: SPICA Mid-infrared Instrument Calibration plan
Author/Editor: 山岸, 光義
山村, 一誠
大薮, 進喜
大坪, 貴文
和田, 武彦
石原, 大助
中川, 貴雄
金田, 英宏
平原, 靖大
YAMAGISHI, Mitsuyoshi
YAMAMURA, Issei
OYABU, Shinki
OTSUBO, Takafumi
WADA, Takehiko
ISHIHARA, Daisuke
NAKAGAWA, Takao
KANEDA, Hidehiro
HIRAHARA, Yasuhiro
Author Heading: 山岸, 光義
山村, 一誠
大薮, 進喜
大坪, 貴文
和田, 武彦
石原, 大助
中川, 貴雄
金田, 英宏
平原, 靖大
YAMAGISHI, Mitsuyoshi
YAMAMURA, Issei
OYABU, Shinki
OTSUBO, Takafumi
WADA, Takehiko
ISHIHARA, Daisuke
NAKAGAWA, Takao
KANEDA, Hidehiro
HIRAHARA, Yasuhiro
Publication, Distribution, etc.: 宇宙航空研究開発機構(JAXA)
Publication Date: 2022-02-28
Publication Date (W3CDTF): 2022-02-28
Periodical title: 宇宙航空研究開発機構研究開発報告 = JAXA Research and Development Report
No. or year of volume/issue: JAXA-RR-21-007E
Volume: JAXA-RR-21-007E
Pages: 1-35
ISSN (Periodical Title): ISSN : 2433-2216
Text Language Code: eng
Subject Heading: space vehicles: instruments
instrumentation: spectrographs
methods: observational
techniques: spectroscopic
Target Audience: 一般
Note (General): Preparatory works for the calibration of SPICA Mid-infrared Instrument (SMI) are reported. We focus on three calibration items, flux, wavelength, and geometrical distortion, and discuss requirements, strategies, and candidates of celestial objects to be used for the calibration. Information of previous and ongoing space infrared astronomical missions is compiled as a reference. We confirm that the standard stars for the flux calibration used in other missions are also applicable for SMI. We investigate objects for wavelength calibration, and conclude that both planetary nebulae and Be stars are needed. In addition, we discuss possible use of molecular lines in red-giant stars for the high-resolution mode. Globular clusters are only the objects that provide a sufficient number of position references for the correction of the geometrical distortion, but further investigation is needed to establish the correction method. The total amount of the observing time for the calibration of SPICA/SMI well fits the allocation plan of the observing time. Information and consideration made so far shall also be useful for future space infrared astronomical missions.
形態: カラー図版あり
Physical characteristics: Original contains color illustrations
資料番号: AA2130034000
レポート番号: JAXA-RR-21-007E
DOI: 10.20637/00048398
Access Restrictions: 限定公開
Data Provider (Database): 国立情報学研究所 : 学術機関リポジトリデータベース（IRDB）（機関リポジトリ）
https://irdb.nii.ac.jp
Original Data Provider (Database): 宇宙航空研究開発機構 : 宇宙航空研究開発機構リポジトリ