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SPICA Distant Cluster Survey: Unveiling the Dust-Obscured Star Formation Triggered by Young Cluster Environments
https://jaxa.repo.nii.ac.jp/records/3008
https://jaxa.repo.nii.ac.jp/records/3008dec7c701-5bd6-4f31-bd38-930aff49e314
名前 / ファイル | ライセンス | アクション |
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AA1730027031.pdf (410.1 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 | SPICA Distant Cluster Survey: Unveiling the Dust-Obscured Star Formation Triggered by Young Cluster Environments | |||||
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 |
小山, 佑世
× 小山, 佑世× 児玉, 忠恭× 林, 将央× 但木, 謙一× 田中, 壱× 嶋川, 里澄× 松原, 英雄× 和田, 武彦× Koyama, Yusei× Kodama, Tadayuki× Hayashi, Masao× Tadaki, Kenichi× Tanaka, Ichi× Shimakawa, Rhythm× Matsuhara, Hideo× Wada, Takehiko |
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著者所属 | ||||||
国立天文台 | ||||||
著者所属 | ||||||
国立天文台 | ||||||
著者所属 | ||||||
東京大学 | ||||||
著者所属 | ||||||
国立天文台 | ||||||
著者所属 | ||||||
国立天文台ハワイ観測所 | ||||||
著者所属 | ||||||
総合研究大学院大学(SOKENDAI) | ||||||
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(英) | ||||||
en | ||||||
National Astronomical Observatory of Japan | ||||||
著者所属(英) | ||||||
en | ||||||
National Astronomical Observatory of Japan | ||||||
著者所属(英) | ||||||
en | ||||||
The University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
National Astronomical Observatory of Japan | ||||||
著者所属(英) | ||||||
en | ||||||
Subaru Telescope, National Astronomical Observatory of Japan | ||||||
著者所属(英) | ||||||
en | ||||||
The Graduate University for Advanced Studies (SOKENDAI) | ||||||
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) | ||||||
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. 137-139, 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 | We present the results of our star-forming galaxy survey of distant clusters of galaxies using Subaru (H ) and AKARI (MIR). By comparing the H and MIR data, we revealed that dust-obscured star-forming galaxies are most preferentially located in the cluster outskirts at z approximately 1. We propose to extend this H - and IR-based environmental study to higher redshifts, but a problem so far is that the existing MIR-FIR surveys always suffer from their limited depths. We can overcome this problems with the wide-field mid-infrared (MIR) camera on-board SPICA (5′FoV), which will allow us an efficient, and extremely deep MIR survey of distant clusters. In particular, the expected high sensitivity of SPICA at 20-40 μm regime promotes us to extend IR galaxy survey out to z = 2-4 (i.e. the “peak epoch” of galaxy evolution) based on their rest-frame 8 μm feature. We provide a quick overview of our recent progress with the MAHALO-Subaru collaboration, and then discuss how significantly SPICA can improve our understanding of the environmental effects on galaxy evolution in the early universe. | |||||
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: AA1730027031 | |||||
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 |