{"id":5736,"date":"2017-05-03T12:40:19","date_gmt":"2017-05-03T03:40:19","guid":{"rendered":"http:\/\/www-v2.icrr.u-tokyo.ac.jp\/prwps\/?post_type=news&#038;p=5736"},"modified":"2019-11-21T12:40:35","modified_gmt":"2019-11-21T03:40:35","slug":"%e8%ab%96%e6%96%87%e6%83%85%e5%a0%b1%e8%a6%b3%e6%b8%ac%e7%9a%84%e5%ae%87%e5%ae%99%e8%ab%96%e3%82%b0%e3%83%ab%e3%83%bc%e3%83%97%e3%80%8csilverrush-iv-ly%ce%b1-luminosity-functions-at-z5-7-and-6-6-2","status":"publish","type":"news","link":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/news\/5736\/","title":{"rendered":"\u8ad6\u6587\u60c5\u5831[\u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30b0\u30eb\u30fc\u30d7]\u300cSILVERRUSH. IV. Ly\u03b1 Luminosity Functions at z=5.7 and 6.6 Studied with ? 2,000 LAEs on the 14\uff0d21 deg2 Sky\u300d"},"content":{"rendered":"\n<p class=\"wp-block-paragraph\">Akira Konno, Masami Ouchi, Takatoshi Shibuya, Yoshiaki Ono, Kazuhiro Shimasaku, Yoshiaki Taniguchi, Tohru Nagao, Masakazu A. R. Kobayashi, Masaru Kajisawa, Nubunari Kashikawa, Akio K. Inoue, Masamune Oguri, Hisanori Furusawa, Tomotsugu Goto, Yuichi Harikane, Ryo Higuchi, Yutaka Komiyama, Haruka Kusakabe, Satoshi Miyazaki, Kimihiko Nakajima, Shiang-Yu Wang,<br>&#8220;SILVERRUSH. IV. Ly\u03b1 Luminosity Functions at z=5.7 and 6.6 Studied with ? 2,000 LAEs on the 14\uff0d21 deg2 Sky&#8221;,<br>19 pages, 12 figures, submitted to PASJ special issue,<br><a href=\"https:\/\/arxiv.org\/pdf\/1705.01222\" target=\"_blank\" rel=\"noreferrer noopener\" aria-label=\" (\u65b0\u3057\u3044\u30bf\u30d6\u3067\u958b\u304f)\">e-Print: ArXiv: 1705.01222[astro-ph.GA]<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Akira Konno, Masami Ouchi, Takatoshi Shibuya, Yoshiaki Ono, Kazuhiro Shimasaku, Yoshiaki Taniguchi, Tohru Naga&#8230;<\/p>\n","protected":false},"featured_media":0,"parent":0,"template":"","taxo_news":[51],"tag_news":[],"class_list":["post-5736","news","type-news","status-publish","hentry","taxo_news-books-and-papers","en-US"],"aioseo_notices":[],"aioseo_head":"\n\t\t<!-- All in One SEO 5.0.2 - aioseo.com -->\n\t<meta name=\"robots\" content=\"max-image-preview:large\" \/>\n\t<link rel=\"canonical\" href=\"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/news\/5736\/\" \/>\n\t<meta name=\"generator\" content=\"All in One SEO (AIOSEO) 5.0.2\" \/>\n\t\t<meta property=\"og:locale\" content=\"en_US\" \/>\n\t\t<meta property=\"og:site_name\" content=\"ICRR | Institute for Cosmic Ray Research University of Tokyo | \u30de\u30eb\u30c1\u30e1\u30c3\u30bb\u30f3\u30b8\u30e3\u30fc\u306e\u89b3\u6e2c\u3092\u901a\u3058\u3001\u5b87\u5b99\u306e\u8b0e\u306b\u8feb\u308a\u307e\u3059\" \/>\n\t\t<meta property=\"og:type\" content=\"article\" \/>\n\t\t<meta property=\"og:title\" content=\"\u8ad6\u6587\u60c5\u5831[\u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30b0\u30eb\u30fc\u30d7]\u300cSILVERRUSH. IV. Ly\u03b1 Luminosity Functions at z=5.7 and 6.6 Studied with ? 2,000 LAEs on the 14\uff0d21 deg2 Sky\u300d | ICRR | Institute for Cosmic Ray Research University of Tokyo\" \/>\n\t\t<meta property=\"og:url\" content=\"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/news\/5736\/\" \/>\n\t\t<meta property=\"article:published_time\" content=\"2017-05-03T03:40:19+00:00\" \/>\n\t\t<meta property=\"article:modified_time\" content=\"2019-11-21T03:40:35+00:00\" \/>\n\t\t<meta name=\"twitter:card\" content=\"summary\" \/>\n\t\t<meta name=\"twitter:title\" content=\"\u8ad6\u6587\u60c5\u5831[\u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30b0\u30eb\u30fc\u30d7]\u300cSILVERRUSH. IV. 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IV. Ly\u03b1 Luminosity Functions at z=5.7 and 6.6 Studied with ? 2,000 LAEs on the 14\uff0d21 deg2 Sky\u300d | ICRR | Institute for Cosmic Ray Research University of Tokyo","og:url":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/news\/5736\/","article:published_time":"2017-05-03T03:40:19+00:00","article:modified_time":"2019-11-21T03:40:35+00:00","twitter:card":"summary","twitter:title":"\u8ad6\u6587\u60c5\u5831[\u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30b0\u30eb\u30fc\u30d7]\u300cSILVERRUSH. IV. 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