{"id":604,"date":"2016-06-15T14:10:16","date_gmt":"2016-06-15T05:10:16","guid":{"rendered":"http:\/\/guas-astronomy.jp\/weblog\/?p=604"},"modified":"2016-06-16T11:32:40","modified_gmt":"2016-06-16T02:32:40","slug":"deep-nir-spectroscopy-for-oiii-emission-line-galaxies-at-z3-the-accelerated-build-up-of-the-red-sequence-in-high-redshift-galaxy-clusters-the-review-of-cerulo16","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=604","title":{"rendered":"Deep NIR spectroscopy for [OIII] emission line galaxies at z>3 \/ The accelerated build-up of the red sequence in high-redshift galaxy clusters (The review of Cerulo+16)"},"content":{"rendered":"<p>[Speaker 1]<br \/>\nTomoko Suzuki, D3, SOKENDAI (Supervisor; Tadayuki Kodama)<br \/>\n[Title]<br \/>\nDeep NIR spectroscopy for [OIII] emission line galaxies at z>3<br \/>\n[Abstract]<br \/>\nI will show our preliminary results obtained by recent near-infrared spectroscopy for narrow-band-selected star-forming galaxies at z>3 with Keck\/MOSFIRE.<\/p>\n<p>[Speaker 2]<br \/>\nMoegi Yamamoto, D1, SOKENDAI (Supervisor; Tadayuki Kodama)<br \/>\n[Title]<br \/>\nThe accelerated build-up of the red sequence in high-redshift galaxy clusters (The review of Cerulo+16)<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker 1] Tomoko Suzuki, D3, SOKENDAI (Supervisor; Tadayuki Kodama) [Title] Deep NIR spectroscopy for [OIII] [&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-604","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\/604","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=604"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/604\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=604"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=604"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=604"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}