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"pubdate": {"attribute_name": "公開日", "attribute_value": "2018-05-18"}, "publish_date": "2018-05-18", "publish_status": "0", "recid": "3147", "relation": {}, "relation_version_is_last": true, "title": ["Herschel 250 micrometers detected star-forming (SF) galaxies over the North Ecliptic Pole (NEP) Wide field of AKARI"], "weko_shared_id": 1}
Herschel 250 micrometers detected star-forming (SF) galaxies over the North Ecliptic Pole (NEP) Wide field of AKARI
https://jaxa.repo.nii.ac.jp/records/3147
https://jaxa.repo.nii.ac.jp/records/3147e766c801-413e-4eb5-8ffd-2811dc3d6f24
名前 / ファイル | ライセンス | アクション |
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AA1730026073.pdf (1.0 MB)
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Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2018-05-18 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Herschel 250 micrometers detected star-forming (SF) galaxies over the North Ecliptic Pole (NEP) Wide field of AKARI | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | infrared | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | star-forming galaxies | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | galaxy evolution | |||||
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 |
Kim, Seong Jin
× Kim, Seong Jin× Jeong, Woong-Seob× Lee, Hyung Mok× 後藤, 友嗣× Pearson, Chris× Shim, Hyunjin× 松原, 英雄× The AKARI NEP Team× Kim, Seong Jin× Jeong, Woong-Seob× Lee, Hyung Mok× Goto, Tomotsugu× Pearson, Chris× Shim, Hyunjin× Matsuhara, Hideo× The AKARI NEP Team |
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著者所属 | ||||||
Korea Astronomy and Space Science Institute : 国立清華大学 | ||||||
著者所属 | ||||||
Korea Astronomy and Space Science Institute | ||||||
著者所属 | ||||||
Seoul National University | ||||||
著者所属 | ||||||
国立清華大学 | ||||||
著者所属 | ||||||
RAL Space, Rutherford Appleton Laboratory : The Open University : University of Oxford | ||||||
著者所属 | ||||||
Kyungpook National University | ||||||
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 | ||||||
Korea Astronomy and Space Science Institute : National Tsing Hua University | ||||||
著者所属(英) | ||||||
en | ||||||
Korea Astronomy and Space Science Institute | ||||||
著者所属(英) | ||||||
en | ||||||
Seoul National University | ||||||
著者所属(英) | ||||||
en | ||||||
National Tsing Hua University | ||||||
著者所属(英) | ||||||
en | ||||||
RAL Space, Rutherford Appleton Laboratory : The Open University : University of Oxford | ||||||
著者所属(英) | ||||||
en | ||||||
Kyungpook National University | ||||||
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: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life 巻 JAXA-SP-17-009E, p. 363-365, 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 study infrared properties of star-forming (SF) galaxies selected by 250 micrometers band detection of the Herschel/SPIRE survey on the entire North Ecliptic Pole (NEP) field of AKARI. We matched SPIRE sources with the spectroscopic survey data and combined with those in the AKARI NEP-Wide catalogue covering from optical to 24 micrometers band. We selected around 250 star-forming galaxies and carried out spectral energy distribution (SED) fit analysis to derive physical quantities. Our SED-fit is based on the continuous near- to mid-IR coverage by 9 photometric bands as well as reliable constraint on far-IR peak by Herschel. Our sample galaxies have prominent mid-IR PAH features and majority of them are LIRG type population in the low-z (less than 0.9). Although they do not seem to form a tight concentration along the galaxy main-sequence due to a wide range of redshift (z is greater than 0.0 and less than 0.9) and various morphological types, they show the downsizing evolutionary pattern toward the present epoch. | |||||
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: AA1730026073 | |||||
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 |