WEKO3
アイテム
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Where do infrared-bright dust-obscured galaxies lie on the star formation rate-stellar mass plane?
https://jaxa.repo.nii.ac.jp/records/3103
https://jaxa.repo.nii.ac.jp/records/3103accbce80-407d-4961-8553-211525061ed2
名前 / ファイル | ライセンス | アクション |
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AA1730026029.pdf (260.5 kB)
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Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2018-05-16 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Where do infrared-bright dust-obscured galaxies lie on the star formation rate-stellar mass plane? | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | catalogs | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | galaxies: active | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | galaxies: star formation | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | infrared: galaxies | |||||
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 |
鳥羽, 儀樹
× 鳥羽, 儀樹× 長尾, 透× Wang, Wei-Hao× 松原, 英雄× 秋山, 正幸× 後藤, 友嗣× 小山, 佑世× 大山, 陽一× 山村, 一誠× Toba, Yoshiki× Nagao, Toru× Wang, Wei-Hao× Matsuhara, Hideo× Akiyama, Masayuki× Goto, Tomotsugu× Koyama, Yusei× Oyama, Yoichi× Yamamura, Issei |
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著者所属 | ||||||
台湾中央研究院天文及天文物理研究所 : 愛媛大学宇宙進化研究センター | ||||||
著者所属 | ||||||
愛媛大学宇宙進化研究センター | ||||||
著者所属 | ||||||
台湾中央研究院天文及天文物理研究所 | ||||||
著者所属 | ||||||
宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS) : 総合研究大学院大学(SOKENDAI) | ||||||
著者所属 | ||||||
東北大学天文学教室 | ||||||
著者所属 | ||||||
国立清華大学 | ||||||
著者所属 | ||||||
国立天文台ハワイ観測所 : 総合研究大学院大学(SOKENDAI) | ||||||
著者所属 | ||||||
台湾中央研究院天文及天文物理研究所 | ||||||
著者所属 | ||||||
宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS) : 総合研究大学院大学(SOKENDAI) | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Astronomy and Astrophysics, Academia Sinica, Taiwan : Research Center for Space and Cosmic Evolution, Ehime University | ||||||
著者所属(英) | ||||||
en | ||||||
Research Center for Space and Cosmic Evolution, Ehime University | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Astronomy and Astrophysics, Academia Sinica, Taiwan | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) : The Graduate University for Advanced Studies (SOKENDAI) | ||||||
著者所属(英) | ||||||
en | ||||||
Astronomical Institute, Tohoku University | ||||||
著者所属(英) | ||||||
en | ||||||
National Tsing Hua University | ||||||
著者所属(英) | ||||||
en | ||||||
Subaru Telescope, National Astronomical Observatory of Japan : The Graduate University for Advanced Studies (SOKENDAI) | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Astronomy and Astrophysics, Academia Sinica, Taiwan | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) : The Graduate University for Advanced Studies (SOKENDAI) | ||||||
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: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life 巻 JAXA-SP-17-009E, p. 181-184, 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) | ||||||
内容記述タイプ | Other | |||||
内容記述 | 第4回「あかり」国際会議 (2017年10月17-20日. 東京大学), 文京区, 東京 | |||||
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 | The 4th AKARI International Conference: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life (October 17-20, 2017. The University of Tokyo), Bunkyo-ku, Tokyo, Japan | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | We present the relation between stellar mass and star formation rate (SFR) of a sample of infrared (IR)-bright dust-obscured galaxies (DOGs) that are defined by (i - brackets 22 brackets)(sub AB) greater than 7.0 and flux density at 22 micrometers greater than 3.8 mJy. Combining the Sloan Digital Sky Survey (SDSS), TwoMicron All Sky Survey (TWOMASS), Wide-field Infrared Survey Explorer (WISE), Infrared Astronomical Satellite (IRAS), and AKARI catalogs, we selected 7 IR-bright DOG at Z(sub spec) is greater than 0 and less than 1. We estimated their stellar mass and SFR based on a spectral energy distribution fitting technique, and compared them with main sequence of star-forming galaxies at z is greater than 0 and less than 2 and local ULIRGs. As a result, we found that most of IR-bright DOGs lie significantly above the main sequence of star-forming galaxies at similar redshifts. We conclude that the majority of IRAS- and/or AKARI-detected IR-bright DOGs are starburst galaxies. | |||||
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: AA1730026029 | |||||
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-17-009E |