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Extragalactic survey with MAXI
https://jaxa.repo.nii.ac.jp/records/5272
https://jaxa.repo.nii.ac.jp/records/527217763326-3b2f-467f-bf74-9c28f4225894
名前 / ファイル | ライセンス | アクション |
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64306033.pdf (215.6 kB)
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Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2015-03-26 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Extragalactic survey with MAXI | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | catalogs - galaxies : active - X-rays : galaxies - X-rays : general | |||||
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 |
上田, 佳宏
× 上田, 佳宏× 廣井, 和雄× 江口, 智士× Ueda, Yoshihiro× Hiroi, Kazuo× Eguchi, Satoshi |
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著者所属 | ||||||
京都大学理学研究科宇宙物理学教室 | ||||||
著者所属 | ||||||
京都大学理学研究科宇宙物理学教室 | ||||||
著者所属 | ||||||
京都大学理学研究科宇宙物理学教室 | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Astronomy, Kyoto University | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Astronomy, Kyoto University | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Astronomy, Kyoto University | ||||||
著者所属(英) | ||||||
en | ||||||
MAXI Team | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構 | |||||
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: Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop 巻 JAXA-SP-08-014E, p. 166-167, 発行日 2009-02-27 |
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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 | Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop (RIKEN, 10-12 June 2008) | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | We summarize the prospects for extragalactic survey with the MAXI mission. By integrating all the data taken for > 1.5 years, we estimate that about 1,300 Active Galactic Nuclei (AGNs) will be detected in the 3-20 keV band with the Gas Slit Cameras from extragalactic sky at Galactic latitudes higher than 15 deg. The MAXI survey will achieve the best sensitivity for populations of moderately absorbed AGNs among any all sky X-ray missions, and is complementary to ROSAT all sky survey and hard X-ray (> 10 keV) surveys by the Swift and INTEGRAL satellites. Many "transient" AGNs could be newly detected with MAXI. In this paper, we discuss the scientific significance of the MAXI survey. | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 1349-113X | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA11984031 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0064306033 | |||||
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-08-014E |