タイトル(掲載誌)宇宙航空研究開発機構研究開発報告 = JAXA Research and Development Report
一般注記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
一次資料へのリンクURLhttps://jaxa.repo.nii.ac.jp/?action=repository_action_common_download&item_id=48414&item_no=1&attribute_id=31&file_no=1
連携機関・データベース国立情報学研究所 : 学術機関リポジトリデータベース(IRDB)(機関リポジトリ)
提供元機関・データベース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