{"id":5694,"date":"2018-02-15T12:26:36","date_gmt":"2018-02-15T03:26:36","guid":{"rendered":"http:\/\/www-v2.icrr.u-tokyo.ac.jp\/prwps\/?post_type=news&#038;p=5694"},"modified":"2019-11-21T12:26:53","modified_gmt":"2019-11-21T03:26:53","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%8csubaru-high-z-exploration-of-low-luminosity-quasars-shellqs-i-2","status":"publish","type":"news","link":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/news\/5694\/","title":{"rendered":"\u8ad6\u6587\u60c5\u5831[\u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30b0\u30eb\u30fc\u30d7]\u300cSubaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) III. Star formation properties of the host galaxies at z>6 studied with ALMA\u300d"},"content":{"rendered":"\n<p>Takuma Izumi, Masafusa Onoue, Hikari Shirakata, Tohru Nagao, Kotaro Kohno, Yoshiki Matsuoka, Masatoshi Imanishi, Michael A. Strauss, Nobunari Kashikawa, Andreas Shulze, John D. Silverman, Seiji Fujimoto, Yuichi Harikane, Yoshiki Toba, Hideki Umehata, Kouichiro Nakanishi, Jenny E. Greene, Yoichi Tamura, Akio Taniguchi, Yuki Yamaguchi, Tomotsugu Goto, Yasuhiro Hashimoto, Soh Ikarashi, Daisuke Iono, Kazushi Iwasawa, Chien-Hsiu Lee, Ryu Makiya, Takeo Minezaki, Ji-Jia Tang,<br>&#8220;Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) III. Star formation properties of the host galaxies at z&gt;6 studied with ALMA&#8221;,<br>Accepted for publication in PASJ,<br><a href=\"https:\/\/arxiv.org\/pdf\/1802.05742\">e-Print: ArXiv: 1802.05742[astro-ph.CO]<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Takuma Izumi, Masafusa Onoue, Hikari Shirakata, Tohru Nagao, Kotaro Kohno, Yoshiki Matsuoka, Masatoshi Imanish&#8230;<\/p>\n","protected":false},"featured_media":0,"parent":0,"template":"","taxo_news":[51],"tag_news":[],"class_list":["post-5694","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\/5694\/\" \/>\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]\u300cSubaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) III. Star formation properties of the host galaxies at z&gt;6 studied with ALMA\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\/5694\/\" \/>\n\t\t<meta property=\"article:published_time\" content=\"2018-02-15T03:26:36+00:00\" \/>\n\t\t<meta property=\"article:modified_time\" content=\"2019-11-21T03:26:53+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]\u300cSubaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) III. Star formation properties of the host galaxies at z&gt;6 studied with ALMA\u300d | ICRR | Institute for Cosmic Ray Research University of Tokyo\" \/>\n\t\t<script type=\"application\/ld+json\" class=\"aioseo-schema\">\n\t\t\t{\"@context\":\"https:\\\/\\\/schema.org\",\"@graph\":[{\"@type\":\"BreadcrumbList\",\"@id\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/en\\\/news\\\/5694\\\/#breadcrumblist\",\"itemListElement\":[{\"@type\":\"ListItem\",\"@id\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/#listItem\",\"position\":1,\"name\":\"\\u30db\\u30fc\\u30e0\",\"item\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/\",\"nextItem\":{\"@type\":\"ListItem\",\"@id\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/en\\\/news\\\/#listItem\",\"name\":\"\\u30cb\\u30e5\\u30fc\\u30b9\"}},{\"@type\":\"ListItem\",\"@id\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/en\\\/news\\\/#listItem\",\"position\":2,\"name\":\"\\u30cb\\u30e5\\u30fc\\u30b9\",\"item\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/en\\\/news\\\/\",\"nextItem\":{\"@type\":\"ListItem\",\"@id\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/en\\\/taxo_news\\\/books-and-papers\\\/#listItem\",\"name\":\"\\u66f8\\u7c4d\\\/\\u8ad6\\u6587\"},\"previousItem\":{\"@type\":\"ListItem\",\"@id\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/#listItem\",\"name\":\"\\u30db\\u30fc\\u30e0\"}},{\"@type\":\"ListItem\",\"@id\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/en\\\/taxo_news\\\/books-and-papers\\\/#listItem\",\"position\":3,\"name\":\"\\u66f8\\u7c4d\\\/\\u8ad6\\u6587\",\"item\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/en\\\/taxo_news\\\/books-and-papers\\\/\",\"nextItem\":{\"@type\":\"ListItem\",\"@id\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/en\\\/news\\\/5694\\\/#listItem\",\"name\":\"\\u8ad6\\u6587\\u60c5\\u5831[\\u89b3\\u6e2c\\u7684\\u5b87\\u5b99\\u8ad6\\u30b0\\u30eb\\u30fc\\u30d7]\\u300cSubaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) III. Star formation properties of the host galaxies at z>6 studied with ALMA\\u300d\"},\"previousItem\":{\"@type\":\"ListItem\",\"@id\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/en\\\/news\\\/#listItem\",\"name\":\"\\u30cb\\u30e5\\u30fc\\u30b9\"}},{\"@type\":\"ListItem\",\"@id\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/en\\\/news\\\/5694\\\/#listItem\",\"position\":4,\"name\":\"\\u8ad6\\u6587\\u60c5\\u5831[\\u89b3\\u6e2c\\u7684\\u5b87\\u5b99\\u8ad6\\u30b0\\u30eb\\u30fc\\u30d7]\\u300cSubaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) III. Star formation properties of the host galaxies at z>6 studied with ALMA\\u300d\",\"previousItem\":{\"@type\":\"ListItem\",\"@id\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/en\\\/taxo_news\\\/books-and-papers\\\/#listItem\",\"name\":\"\\u66f8\\u7c4d\\\/\\u8ad6\\u6587\"}}]},{\"@type\":\"Organization\",\"@id\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/#organization\",\"name\":\"\\u6771\\u4eac\\u5927\\u5b66\\u5b87\\u5b99\\u7dda\\u7814\\u7a76\\u6240\",\"description\":\"\\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\",\"url\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/\",\"logo\":{\"@type\":\"ImageObject\",\"url\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/prwps\\\/wp-content\\\/uploads\\\/logo_w-1.jpeg\",\"@id\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/en\\\/news\\\/5694\\\/#organizationLogo\",\"width\":340,\"height\":180},\"image\":{\"@id\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/en\\\/news\\\/5694\\\/#organizationLogo\"}},{\"@type\":\"WebPage\",\"@id\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/en\\\/news\\\/5694\\\/#webpage\",\"url\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/en\\\/news\\\/5694\\\/\",\"name\":\"\\u8ad6\\u6587\\u60c5\\u5831[\\u89b3\\u6e2c\\u7684\\u5b87\\u5b99\\u8ad6\\u30b0\\u30eb\\u30fc\\u30d7]\\u300cSubaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) III. Star formation properties of the host galaxies at z>6 studied with ALMA\\u300d | ICRR | Institute for Cosmic Ray Research University of Tokyo\",\"inLanguage\":\"en-US\",\"isPartOf\":{\"@id\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/#website\"},\"breadcrumb\":{\"@id\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/en\\\/news\\\/5694\\\/#breadcrumblist\"},\"datePublished\":\"2018-02-15T12:26:36+09:00\",\"dateModified\":\"2019-11-21T12:26:53+09:00\"},{\"@type\":\"WebSite\",\"@id\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/#website\",\"url\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/\",\"name\":\"ICRR | Institute for Cosmic Ray Research University of Tokyo\",\"description\":\"\\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\",\"inLanguage\":\"en-US\",\"publisher\":{\"@id\":\"https:\\\/\\\/www.icrr.u-tokyo.ac.jp\\\/#organization\"}}]}\n\t\t<\/script>\n\t\t<!-- All in One SEO -->\n\n","aioseo_head_json":{"title":"\u8ad6\u6587\u60c5\u5831[\u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30b0\u30eb\u30fc\u30d7]\u300cSubaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) III. Star formation properties of the host galaxies at z>6 studied with ALMA\u300d | ICRR | Institute for Cosmic Ray Research University of Tokyo","description":"","canonical_url":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/news\/5694\/","robots":"max-image-preview:large","keywords":"","webmasterTools":{"miscellaneous":""},"schema":{"@context":"https:\/\/schema.org","@graph":[{"@type":"BreadcrumbList","@id":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/news\/5694\/#breadcrumblist","itemListElement":[{"@type":"ListItem","@id":"https:\/\/www.icrr.u-tokyo.ac.jp\/#listItem","position":1,"name":"\u30db\u30fc\u30e0","item":"https:\/\/www.icrr.u-tokyo.ac.jp\/","nextItem":{"@type":"ListItem","@id":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/news\/#listItem","name":"\u30cb\u30e5\u30fc\u30b9"}},{"@type":"ListItem","@id":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/news\/#listItem","position":2,"name":"\u30cb\u30e5\u30fc\u30b9","item":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/news\/","nextItem":{"@type":"ListItem","@id":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/taxo_news\/books-and-papers\/#listItem","name":"\u66f8\u7c4d\/\u8ad6\u6587"},"previousItem":{"@type":"ListItem","@id":"https:\/\/www.icrr.u-tokyo.ac.jp\/#listItem","name":"\u30db\u30fc\u30e0"}},{"@type":"ListItem","@id":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/taxo_news\/books-and-papers\/#listItem","position":3,"name":"\u66f8\u7c4d\/\u8ad6\u6587","item":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/taxo_news\/books-and-papers\/","nextItem":{"@type":"ListItem","@id":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/news\/5694\/#listItem","name":"\u8ad6\u6587\u60c5\u5831[\u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30b0\u30eb\u30fc\u30d7]\u300cSubaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) III. Star formation properties of the host galaxies at z>6 studied with ALMA\u300d"},"previousItem":{"@type":"ListItem","@id":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/news\/#listItem","name":"\u30cb\u30e5\u30fc\u30b9"}},{"@type":"ListItem","@id":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/news\/5694\/#listItem","position":4,"name":"\u8ad6\u6587\u60c5\u5831[\u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30b0\u30eb\u30fc\u30d7]\u300cSubaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) III. Star formation properties of the host galaxies at z>6 studied with ALMA\u300d","previousItem":{"@type":"ListItem","@id":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/taxo_news\/books-and-papers\/#listItem","name":"\u66f8\u7c4d\/\u8ad6\u6587"}}]},{"@type":"Organization","@id":"https:\/\/www.icrr.u-tokyo.ac.jp\/#organization","name":"\u6771\u4eac\u5927\u5b66\u5b87\u5b99\u7dda\u7814\u7a76\u6240","description":"\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","url":"https:\/\/www.icrr.u-tokyo.ac.jp\/","logo":{"@type":"ImageObject","url":"https:\/\/www.icrr.u-tokyo.ac.jp\/prwps\/wp-content\/uploads\/logo_w-1.jpeg","@id":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/news\/5694\/#organizationLogo","width":340,"height":180},"image":{"@id":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/news\/5694\/#organizationLogo"}},{"@type":"WebPage","@id":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/news\/5694\/#webpage","url":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/news\/5694\/","name":"\u8ad6\u6587\u60c5\u5831[\u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30b0\u30eb\u30fc\u30d7]\u300cSubaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) III. Star formation properties of the host galaxies at z>6 studied with ALMA\u300d | ICRR | Institute for Cosmic Ray Research University of Tokyo","inLanguage":"en-US","isPartOf":{"@id":"https:\/\/www.icrr.u-tokyo.ac.jp\/#website"},"breadcrumb":{"@id":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/news\/5694\/#breadcrumblist"},"datePublished":"2018-02-15T12:26:36+09:00","dateModified":"2019-11-21T12:26:53+09:00"},{"@type":"WebSite","@id":"https:\/\/www.icrr.u-tokyo.ac.jp\/#website","url":"https:\/\/www.icrr.u-tokyo.ac.jp\/","name":"ICRR | Institute for Cosmic Ray Research University of Tokyo","description":"\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","inLanguage":"en-US","publisher":{"@id":"https:\/\/www.icrr.u-tokyo.ac.jp\/#organization"}}]},"og:locale":"en_US","og:site_name":"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","og:type":"article","og:title":"\u8ad6\u6587\u60c5\u5831[\u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30b0\u30eb\u30fc\u30d7]\u300cSubaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) III. Star formation properties of the host galaxies at z&gt;6 studied with ALMA\u300d | ICRR | Institute for Cosmic Ray Research University of Tokyo","og:url":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/news\/5694\/","article:published_time":"2018-02-15T03:26:36+00:00","article:modified_time":"2019-11-21T03:26:53+00:00","twitter:card":"summary","twitter:title":"\u8ad6\u6587\u60c5\u5831[\u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30b0\u30eb\u30fc\u30d7]\u300cSubaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) III. Star formation properties of the host galaxies at z&gt;6 studied with ALMA\u300d | ICRR | Institute for Cosmic Ray Research University of Tokyo"},"aioseo_meta_data":{"post_id":"5694","title":null,"description":null,"keywords":null,"keyphrases":null,"primary_term":null,"canonical_url":null,"og_title":null,"og_description":null,"og_object_type":"default","og_image_type":"default","og_image_url":null,"og_image_width":null,"og_image_height":null,"og_image_custom_url":null,"og_image_custom_fields":null,"og_video":null,"og_custom_url":null,"og_article_section":null,"og_article_tags":null,"twitter_use_og":false,"twitter_card":"default","twitter_image_type":"default","twitter_image_url":null,"twitter_image_custom_url":null,"twitter_image_custom_fields":null,"twitter_title":null,"twitter_description":null,"schema":{"blockGraphs":[],"customGraphs":[],"default":{"data":{"Article":[],"Course":[],"Dataset":[],"FAQPage":[],"Movie":[],"Person":[],"Product":[],"ProductReview":[],"Car":[],"Recipe":[],"Service":[],"SoftwareApplication":[],"WebPage":[]},"graphName":"","isEnabled":true},"graphs":[]},"schema_type":null,"schema_type_options":null,"pillar_content":false,"robots_default":true,"robots_noindex":false,"robots_noarchive":false,"robots_nosnippet":false,"robots_nofollow":false,"robots_noimageindex":false,"robots_noodp":false,"robots_notranslate":false,"robots_max_snippet":null,"robots_max_videopreview":null,"robots_max_imagepreview":"large","priority":null,"frequency":null,"local_seo":null,"breadcrumb_settings":null,"limit_modified_date":false,"ai":null,"created":"2021-04-19 12:01:02","updated":"2025-09-19 22:30:28","focus_keyword":null,"additional_keywords":null,"truseo_locale":null,"seo_analyzer_scan_date":null},"aioseo_breadcrumb":"<div class=\"aioseo-breadcrumbs\"><span class=\"aioseo-breadcrumb\">\n\t\t\t<a href=\"https:\/\/www.icrr.u-tokyo.ac.jp\/\" title=\"\u30db\u30fc\u30e0\">\u30db\u30fc\u30e0<\/a>\n\t\t<\/span><span class=\"aioseo-breadcrumb-separator\">\u00bb<\/span><span class=\"aioseo-breadcrumb\">\n\t\t\t<a href=\"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/news\/\" title=\"\u30cb\u30e5\u30fc\u30b9\">\u30cb\u30e5\u30fc\u30b9<\/a>\n\t\t<\/span><span class=\"aioseo-breadcrumb-separator\">\u00bb<\/span><span class=\"aioseo-breadcrumb\">\n\t\t\t<a href=\"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/taxo_news\/books-and-papers\/\" title=\"\u66f8\u7c4d\/\u8ad6\u6587\">\u66f8\u7c4d\/\u8ad6\u6587<\/a>\n\t\t<\/span><span class=\"aioseo-breadcrumb-separator\">\u00bb<\/span><span class=\"aioseo-breadcrumb\">\n\t\t\t\u8ad6\u6587\u60c5\u5831[\u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30b0\u30eb\u30fc\u30d7]\u300cSubaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) III. Star formation properties of the host galaxies at z&gt;6 studied with ALMA\u300d\n\t\t<\/span><\/div>","aioseo_breadcrumb_json":[{"label":"\u30db\u30fc\u30e0","link":"https:\/\/www.icrr.u-tokyo.ac.jp\/"},{"label":"\u30cb\u30e5\u30fc\u30b9","link":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/news\/"},{"label":"\u66f8\u7c4d\/\u8ad6\u6587","link":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/taxo_news\/books-and-papers\/"},{"label":"\u8ad6\u6587\u60c5\u5831[\u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30b0\u30eb\u30fc\u30d7]\u300cSubaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) III. Star formation properties of the host galaxies at z>6 studied with ALMA\u300d","link":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/news\/5694\/"}],"_links":{"self":[{"href":"https:\/\/www.icrr.u-tokyo.ac.jp\/wp-json\/wp\/v2\/news\/5694","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.icrr.u-tokyo.ac.jp\/wp-json\/wp\/v2\/news"}],"about":[{"href":"https:\/\/www.icrr.u-tokyo.ac.jp\/wp-json\/wp\/v2\/types\/news"}],"wp:attachment":[{"href":"https:\/\/www.icrr.u-tokyo.ac.jp\/wp-json\/wp\/v2\/media?parent=5694"}],"wp:term":[{"taxonomy":"taxo_news","embeddable":true,"href":"https:\/\/www.icrr.u-tokyo.ac.jp\/wp-json\/wp\/v2\/taxo_news?post=5694"},{"taxonomy":"tag_news","embeddable":true,"href":"https:\/\/www.icrr.u-tokyo.ac.jp\/wp-json\/wp\/v2\/tag_news?post=5694"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}