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J-GLOBAL ID：202002267282774715   整理番号：20A1641191

ALMA 26 1ミリメートル(ASAGAO)におけるGOODS-Sのアークミンボーイング2調査【JST・京大機械翻訳】

ALMA twenty-six arcmin² survey of GOODS-S at one millimeter (ASAGAO)

著者 (46件)： Hatsukade B. (Institute of Astronomy, Graduate School of Science, The University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo, Japan email: [e-mail]) ,  Kohno K. (Institute of Astronomy, Graduate School of Science, The University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo, Japan email: [e-mail]) ,  Kohno K. (Research Center for the Early Universe, The University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo, Japan) ,  Yamaguchi Y. (Institute of Astronomy, Graduate School of Science, The University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo, Japan email: [e-mail]) ,  Umehata H. (Institute of Astronomy, Graduate School of Science, The University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo, Japan email: [e-mail]) ,  Umehata H. (RIKEN Cluster for Pioneering Research, 2-1 Hirosawa, Wako-shi, Saitama, Japan) ,  Ao Y. (Purple Mountain Observatory & Key Laboratory for Radio Astronomy, Chinese Academy of Sciences, 8 Yuanhua Road, Nanjing, China) ,  Aretxaga I. (Instituto Nacional de Astrofsica, Optica y Electronica (INAOE), Luis Enrique Erro 1, Sta. Ma. Tonantzintla, Puebla, Mexico) ,  Caputi K. I. (Kapteyn Astronomical Institute, University of Groningen, P.O. Box 800, 9700AV Groningen, The Netherlands) ,  Dunlop J. S. (Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh EH9 3HJ UK) ,  Egami E. (Steward Observatory, University of Arizona, 933 N. Cherry Ave, Tucson, AZ, USA) ,  Espada D. (National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo, Japan) ,  Espada D. (SOKENDAI (The Graduate University for Advanced Studies), 2-21-1 Osawa, Mitaka, Tokyo, Japan) ,  Fujimoto S. (Institute for Cosmic Ray Research, The University of Tokyo, Kashiwa, Chiba, Japan) ,  Hayatsu N. (Department of Physics, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo, Japan) ,  Hayatsu N. (European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748 Garching, Germany) ,  Hughes D. H. (Instituto Nacional de Astrofsica, Optica y Electronica (INAOE), Luis Enrique Erro 1, Sta. Ma. Tonantzintla, Puebla, Mexico) ,  Ikarashi S. (Kapteyn Astronomical Institute, University of Groningen, P.O. Box 800, 9700AV Groningen, The Netherlands) ,  Iono D. (National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo, Japan) ,  Iono D. (SOKENDAI (The Graduate University for Advanced Studies), 2-21-1 Osawa, Mitaka, Tokyo, Japan) ,  Ivison R. J. (European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748 Garching, Germany) ,  Ivison R. J. (Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh EH9 3HJ UK) ,  Kawabe R. (National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo, Japan) ,  Kawabe R. (SOKENDAI (The Graduate University for Advanced Studies), 2-21-1 Osawa, Mitaka, Tokyo, Japan) ,  Kodama T. (Astronomical Institute, Tohoku University, Aramaki, Aoba-ku, Sendai, Miyagi, Japan) ,  Lee M. (Department of Physics, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Japan) ,  Matsuda Y. (National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo, Japan) ,  Matsuda Y. (SOKENDAI (The Graduate University for Advanced Studies), 2-21-1 Osawa, Mitaka, Tokyo, Japan) ,  Nakanishi K. (National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo, Japan) ,  Nakanishi K. (SOKENDAI (The Graduate University for Advanced Studies), 2-21-1 Osawa, Mitaka, Tokyo, Japan) ,  Ohta K. (Department of Astronomy, Kyoto University, Kyoto, Japan) ,  Ouchi M. (Institute for Cosmic Ray Research, The University of Tokyo, Kashiwa, Chiba, Japan) ,  Ouchi M. (Kavli Institute for the Physics and Mathematics of the Universe, Todai Institutes for Advanced Study, the University of Tokyo, Kashiwa, Japan (Kavli IPMU, WPI)) ,  Rujopakarn W. (Kavli Institute for the Physics and Mathematics of the Universe, Todai Institutes for Advanced Study, the University of Tokyo, Kashiwa, Japan (Kavli IPMU, WPI)) ,  Rujopakarn W. (Department of Physics, Faculty of Science, Chulalongkorn University, 254 Phayathai Road, Pathumwan, Bangkok, Thailand) ,  Rujopakarn W. (National Astronomical Research Institute of Thailand (Public Organization), Don Kaeo, Mae Rim, Chiang Mai, Thailand) ,  Suzuki T. (National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo, Japan) ,  Tamura Y. (Department of Physics, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Japan) ,  Ueda Y. (Department of Astronomy, Kyoto University, Kyoto, Japan) ,  Wang T. (Institute of Astronomy, Graduate School of Science, The University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo, Japan email: [e-mail]) ,  Wang T. (National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo, Japan) ,  Wang W.-H. (Institute of Astronomy and Astrophysics, Academia Sinica, Taipei, Taiwan) ,  Wilson G. W. (Department of astronomy, University of Massachusetts, Amherst, MA, USA) ,  Yoshimura Y. (Institute of Astronomy, Graduate School of Science, The University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo, Japan email: [e-mail]) ,  Yun M. S. (Department of astronomy, University of Massachusetts, Amherst, MA, USA) ,  ASAGAO team
資料名： Proceedings of the International Astronomical Union  (Proceedings of the International Astronomical Union)
巻： 15  号： S352  ページ： 239-240  発行年： 2019年 
JST資料番号： W5499A  ISSN： 1743-9213  資料種別： 逐次刊行物 (A)
記事区分： 原著論文  発行国： イギリス (GBR)  言語： 英語 (EN)

抄録/ポイント： 1mm(ASAGAO)でのGOODS-SのALMA26arcmin2調査は,1.2mmの隣接場での深い(1σ~61μJy/ビーム)と広い面積(26arcmin2)の調査である。アーカイブデータと組み合わせることにより,同じ領域(1σ~30μJy/ビーム-1,合成ビームサイズ0.59′′×0.53′′)でより深いマップを得て,ALMAブランク場調査の中で,発生源の最大試料(5σで25源,4.5σで45源)を得た。4.5σ源の中央値赤方偏移は2.4であった。数カウントは,1.2mmの銀河外バックグラウンド光の52%が離散源に分解されることを示した。z=1-3でIR光度関数(LFs)を作成し,2

シソーラス用語： 赤方偏移 ,  *光度 ,  ブランク
準シソーラス用語： 発生源 ,  光度関数 ,  弱光 , 【Automatic Indexing@JST】

著者キーワード (3件)： 宇宙論:観測 ,  銀河:進化 ,  銀河:形成

分類 (1件)： 星雲  (DB06000W)

タイトルに関連する用語 (2件)： ALMA ,  調査