{"id":868,"date":"2018-04-27T09:11:57","date_gmt":"2018-04-27T00:11:57","guid":{"rendered":"http:\/\/guas-astronomy.jp\/weblog\/?p=868"},"modified":"2018-04-27T09:11:57","modified_gmt":"2018-04-27T00:11:57","slug":"detecting-proto-bcg-candidates-at-z4-by-using-hsc-ssp-gas-inflow-and-outflow-of-star-forming-galaxies-at-redshift-1-4-as-revealed-by-chemical-evolution","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=868","title":{"rendered":"Detecting proto-BCG candidates at z~4 by using HSC-SSP \/ Gas inflow and outflow of star forming galaxies at redshift 1.4 as revealed by chemical evolution"},"content":{"rendered":"<p>[Speaker1]<br \/>\nKei Ito, SOKENDAI 2nd year (M2)(Supervisor: Nobunari Kashikawa,Yuichi Matsuda,Yusei Koyama)<br \/>\n[Title]<br \/>\nDetecting proto-BCG candidates at z~4 by using HSC-SSP<\/p>\n<p>[Speaker2]<br \/>\nNao Fukagawa, SOKENDAI 3rd year (D1)(Supervisor: Prof. Tadayuki Kodama,,)<br \/>\n[Title]<br \/>\nGas inflow and outflow of star forming galaxies at redshift 1.4 as revealed by chemical evolution<br \/>\n[Abstract]<br \/>\nGas inflow and outflow are processes that control star formation history of galaxies. Using chemical evolution models, we attempt to extract information about gas inflow and outflow of star forming galaxies at redshift z~1.4. In this talk, we discuss our results.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker1] Kei Ito, SOKENDAI 2nd year (M2)(Supervisor: Nobunari Kashikawa,Yuichi Matsuda,Yusei Koyama) [Title] [&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-868","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\/868","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=868"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/868\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=868"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=868"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=868"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}