WEKO3
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DEIMOS Spectroscopy of Star-Forming Galaxies in the AKARI North Ecliptic Pole-Deep Field
https://jaxa.repo.nii.ac.jp/records/3149
https://jaxa.repo.nii.ac.jp/records/3149d651ac42-e006-4ed0-9fad-28cfee820689
名前 / ファイル | ライセンス | アクション |
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AA1730026075.pdf (364.3 kB)
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Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2018-05-18 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | DEIMOS Spectroscopy of Star-Forming Galaxies in the AKARI North Ecliptic Pole-Deep Field | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | techniques: spectroscopic | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | galaxies: evolution | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | galaxies: distances and redshifts | |||||
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 |
Kim, Helen K.
× Kim, Helen K.× Malkan, Matthew A.× 大井, 渚× Burgarella, Denis× Buat, Veronique× 高木, 俊暢× 松原, 英雄× Kim, Helen K.× Malkan, Matthew A.× Oi, Nagisa× Burgarella, Denis× Buat, Veronique× Takagi, Toshinobu× Matsuhara, Hideo |
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著者所属 | ||||||
University of California, Los Angeles | ||||||
著者所属 | ||||||
University of California, Los Angeles | ||||||
著者所属 | ||||||
東京理科大学 | ||||||
著者所属 | ||||||
Aix-Marseille Universite | ||||||
著者所属 | ||||||
Aix-Marseille Universite | ||||||
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 | ||||||
University of California, Los Angeles | ||||||
著者所属(英) | ||||||
en | ||||||
University of California, Los Angeles | ||||||
著者所属(英) | ||||||
en | ||||||
Tokyo University of Science | ||||||
著者所属(英) | ||||||
en | ||||||
Aix-Marseille Universite | ||||||
著者所属(英) | ||||||
en | ||||||
Aix-Marseille Universite | ||||||
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: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life 巻 JAXA-SP-17-009E, p. 371-374, 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 follow-up optical DEIMOS/Keck-II spectra of in the order of 180 galaxies (median z in the order of 0.7) in the AKARI NEP-Deep field. The spectroscopic redshifts (z(sub spec)) agree well with photometric redshifts (z(sub phot)) at z less than 1, with mean absolute value of z approximately equal to 0.07, but the photometric redshifts are systematically too high at z greater than 1. One Seyfert 1.9 and one Seyfert 2 were identified from their emission lines, but no LINERs were found, in contrast to Kartaltepe et al. (2015), 84% of our objects are classified to be along the star-forming, HII sequence. At a given stellar mass, gas phase metallicities were found to be 0.1-0.2 dex lower than the local SDSS relation, but consistent with the relation found by Zahid et al. (2011) at z in the order of 0.8. Gas reddenings were derived from Balmer emission line ratios. In the majority of cases, the corresponding extinction at H alpha is in the order of 1 mag, typical of normal spiral galaxies. Star formation rates (SFRs) were estimated from the luminosities of either brackets O II brackets lambda 3727 or H alpha, and agreed reasonably (50% scatter). In galaxies with equivalent width EW(H alpha) of 10 angstroms or less, the broadband spectral energy distribution (SED) fitting significantly overestimates the SFR. | |||||
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: AA1730026075 | |||||
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 |