{"id":505,"date":"2015-11-05T15:37:54","date_gmt":"2015-11-05T06:37:54","guid":{"rendered":"http:\/\/guas-astronomy.jp\/weblog\/?p=505"},"modified":"2016-06-16T11:32:41","modified_gmt":"2016-06-16T02:32:41","slug":"the-morphologies-and-stellar-population-of-high-z-galaxies-at-0-5","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=505","title":{"rendered":"The morphologies and stellar population of high-z galaxies at 0.5\uff1cz\uff1c2.5; star-forming main sequence, clumpy galaxies and passive galaxies \/ Star Forming Molecular Gas in Merging Galaxies ~ASTE Observation~"},"content":{"rendered":"<p>[Speaker 1]<br \/>\nSumire Tatehora, D3, SOKENDAI (supervisor: Nobuo Arimoto)<br \/>\n[Title]<br \/>\nThe morphologies and stellar population of high-z galaxies at 0.5\uff1cz\uff1c2.5; star-forming main sequence, clumpy galaxies and passive galaxies<\/p>\n<p>[Speaker 2]<br \/>\nTomonari Michiyama, M2, SOKENDAI (supervisor: D. Iono)<br \/>\n[Title]<br \/>\nStar Forming Molecular Gas in Merging Galaxies ~ASTE Observation~ <\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker 1] Sumire Tatehora, D3, SOKENDAI (supervisor: Nobuo Arimoto) [Title] The morphologies and stellar pop [&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-505","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\/505","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=505"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/505\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=505"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=505"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=505"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}