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Estimation of the Confusion Limit for SPICA
https://jaxa.repo.nii.ac.jp/records/3013
https://jaxa.repo.nii.ac.jp/records/3013a28faa22-29e1-4255-95a6-d70d042b6105
名前 / ファイル | ライセンス | アクション |
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AA1730027036.pdf (362.9 kB)
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Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2018-05-01 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Estimation of the Confusion Limit for SPICA | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_5794 | |||||
資源タイプ | conference paper | |||||
著者 |
竹内, 努
× 竹内, 努× 和田, 武彦× 松原, 英雄× 土井, 靖生× 長島, 雅裕× 榎, 基宏× 石井, 貴子× Takeuchi, Tsutomu T.× Wada, Takehiko× Matsuhara, Hideo× Doi, Yasuo× Nagashima, Masahiro× Enoki, Motohiro× Ishii, Takako T. |
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著者所属 | ||||||
名古屋大学 | ||||||
著者所属 | ||||||
宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS) | ||||||
著者所属 | ||||||
宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS) | ||||||
著者所属 | ||||||
東京大学 | ||||||
著者所属 | ||||||
長崎大学 | ||||||
著者所属 | ||||||
東京経済大学 | ||||||
著者所属 | ||||||
京都大学 | ||||||
著者所属(英) | ||||||
en | ||||||
Nagoya University | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) | ||||||
著者所属(英) | ||||||
en | ||||||
The University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
Nagasaki University | ||||||
著者所属(英) | ||||||
en | ||||||
Tokyo Keizai University | ||||||
著者所属(英) | ||||||
en | ||||||
Kyoto University | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構(JAXA) | |||||
出版者(英) | ||||||
出版者 | Japan Aerospace Exploration Agency (JAXA) | |||||
書誌情報 |
宇宙航空研究開発機構特別資料 en : JAXA Special Publication: Proceedings of the SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe 巻 JAXA-SP-17-010E, p. 157-159, 発行日 2018-03-09 |
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会議概要(会議名, 開催地, 会期, 主催者等)(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe (June 18-21, 2013. Ito Hall, the University of Tokyo), Bunkyou-ku, Tokyo, Japan | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Since the most fundamental limit to detect very distant objects is the source confusion, the estimation of the source confusion limit of SPICA is very important to decide the observational strategy. We estimated the confusion limit of SPICA from 5 to 200 μm. For the mid- and far-IR (MIR and FIR) galaxy counts, we used an updated version of the empirical galaxy number count model of Takeuchi et al. (2001). At 5 μm, we used a semi-analytic galaxy evolution model “ νGC” to construct the galaxy number counts. Based on his, confusion limits for SPICA were estimated by the analytic formulation that can deal with angular clustering of the galaxies (Takeuchi & Ishii 2004). | |||||
内容記述 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 形態: カラー図版あり | |||||
内容記述(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Physical characteristics: Original contains color illustrations | |||||
ISSNONLINE | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 2433-2232 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA1730027036 | |||||
レポート番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | レポート番号: JAXA-SP-17-010E |