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AKARI sheds light on the red side of active galactic nuclei at z = 0 to z = 6
https://jaxa.repo.nii.ac.jp/records/3109
https://jaxa.repo.nii.ac.jp/records/31099a189d57-fe2a-44f5-ad79-6a3e71788f72
名前 / ファイル | ライセンス | アクション |
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AA1730026035.pdf (2.6 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 | AKARI sheds light on the red side of active galactic nuclei at z = 0 to z = 6 | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | Active galactic nuclei | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | Quasars | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | Galaxy evolution | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | High redshift universe | |||||
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 |
Im, Myungshin
× Im, Myungshin |
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著者所属(英) | ||||||
en | ||||||
Seoul National 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: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life 巻 JAXA-SP-17-009E, p. 209-216, 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 | This paper presents highlights from AKARI studies of active galactic nuclei (AGNs). Using its unique spectroscopic capability at 2.5 to 5.0 micrometers, AKARI revealed for the first time the redshifted H alpha lines and the rest-frame optical spectra of AGNs at z is greater than 4 and less than 6, establishing the luminosity scaling relations in the optical at high redshift and tracing the black hole mass growth history in the early universe based on black hole (BH) mass estimators in the optical. The AKARI's NIR spectroscopy also helped researchers detect the Brackett lines and 3.3 micrometers PAH features and traced the hot/warm dust emission of nearby AGNs and luminous infrared galaxies, showing promises of these spectral features to examine the host galaxy star formation rate and the black hole masses. The NIR spectroscopy of low redshift AGNs also revealed a rather cooler nature of the hot dust emission with T approximately 1100K than previously discussed. AKARI also produced other interesting scientific results utilizing its pan-chromatic mid-infrared (MIR) imaging capability. AKARI made pioneering contributions to the MIR selection of obscured/unobscured AGNs, two-sided nature of AGN feedback in the galaxy evolution, and the AGN contribution in luminous infrared galaxies. These results pave ways for infrared studies of AGN by post-AKARI/future facilities and we expect that studies of the data gained by AKARI will continue to make valuable contributions to our understanding of AGNs. | |||||
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: AA1730026035 | |||||
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 |