{"id":832,"date":"2018-02-01T11:58:19","date_gmt":"2018-02-01T02:58:19","guid":{"rendered":"http:\/\/guas-astronomy.jp\/weblog\/?p=832"},"modified":"2018-02-01T11:58:19","modified_gmt":"2018-02-01T02:58:19","slug":"a-start-to-understand-the-relation-between-galaxies-and-igm-in-the-most-over-dense-regions-exploration-of-the-cosmic-dawn-with-high-redshift-quasars-detecting-brightest-cluster-galaxies-at-z4-by","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=832","title":{"rendered":"A start to understand the relation between galaxies and IGM in the most over-dense regions \/ Exploration of the Cosmic Dawn with High-Redshift Quasars \/ Detecting Brightest Cluster Galaxies at z~4 by using Hyper Suprime-Cam"},"content":{"rendered":"<p>[Speaker 1]<br \/>\nLiang, Yongming, SOKENDAI 1st year (M1)(Supervisor: Kashikawa, Nobunari,,)<br \/>\n[Title]<br \/>\nA start to understand the relation between galaxies and IGM in the most over-dense regions<\/p>\n<p>[Speaker 2]<br \/>\nMasafusa Onoue, SOKENDAI 5th year (D3)(Supervisor: Nobunari Kashikawa,,)<br \/>\n[Title]<br \/>\nExploration of the Cosmic Dawn with High-Redshift Quasars<\/p>\n<p>[Speaker 3]<br \/>\nKei Ito, SOKENDAI 1st year (M1)(Supervisor: Nobunari Kashikawa,Yuichi Matsuda,Yusei Koyama)<br \/>\n[Title]<br \/>\nDetecting Brightest Cluster Galaxies at z~4 by using Hyper Suprime-Cam<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker 1] Liang, Yongming, SOKENDAI 1st year (M1)(Supervisor: Kashikawa, Nobunari,,) [Title] A start to unde [&hellip;]<\/p>\n","protected":false},"author":2,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[6,5],"tags":[],"class_list":["post-832","post","type-post","status-publish","format-standard","hentry","category-6","category-5"],"_links":{"self":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/832","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=832"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/832\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=832"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=832"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=832"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}