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Far-IR dust properties of highly dust obscured AGNs from the AKARI and WISE all-sky surveys
https://jaxa.repo.nii.ac.jp/records/3141
https://jaxa.repo.nii.ac.jp/records/3141bccb31ad-4480-4e04-a35e-4da8a7d51ec5
名前 / ファイル | ライセンス | アクション |
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AA1730026067.pdf (451.2 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 | Far-IR dust properties of highly dust obscured AGNs from the AKARI and WISE all-sky surveys | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | infrared: galaxies | |||||
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 | catalogs | |||||
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 |
Lam, Anson
× Lam, Anson× Malkan, Matthew× Wright, Edward |
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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 | ||||||
University of California, Los Angeles | ||||||
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. 341-344, 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 | The combination of the AKARI and WISE infrared all-sky surveys provides an unique opportunity to identify and characterize the most highly dust obscured AGNs in the universe. Dust-obscured AGNs are not easily detectable and potentially underrepresented in extragalactic surveys due to their high optical extinction, but are readily found in the WISE catalog due to their very red mid-IR colors. Combining these surveys with photometry from Herschel SPIRE and SDSS, we use SED modeling to characterize the extinction and dust properties of these mid-IR selected AGNs. We show that we can estimate bolometric corrections for dusty AGNs using WISE colors. Using AKARI's far-IR wavelength photometry and broadband AGN/galaxy spectral templates, we also estimate the mass and temperature properties of our AGN sample. | |||||
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: AA1730026067 | |||||
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 |