{"id":1798,"date":"2022-07-20T13:18:50","date_gmt":"2022-07-20T04:18:50","guid":{"rendered":"https:\/\/guas-astronomy.jp\/weblog\/?p=1798"},"modified":"2022-07-20T13:18:50","modified_gmt":"2022-07-20T04:18:50","slug":"uncovering-the-origin-of-very-high-fe-o-in-young-star-forming-galaxies-sn2018zd-a-promising-candidate-of-electron-capture-supernova-progress-of-light-curve-modeling","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=1798","title":{"rendered":"Uncovering the Origin of Very High Fe\/O in Young Star Forming Galaxies \/  SN2018zd: a promising candidate of Electron Capture Supernova Progress of light curve modeling"},"content":{"rendered":"<p>[Speaker1]<br \/>\nKuria Watanabe<br \/>\nSOKENDAI 1st year (M1)<br \/>\n(Supervisor: Masami Ouchi, Nozomu Tominaga, Masato Onodera)<br \/>\n[Title1]<br \/>\nUncovering the Origin of Very High Fe\/O in Young Star Forming Galaxies<\/p>\n<p>[Speaker2]<br \/>\nMasato Sato<br \/>\nSOKENDAI 3rd year (D1)<br \/>\n(Supervisor: Nozomu Tominaga, Tomoya Takiwaki, Takashi Moriya)<br \/>\n[Title2]<br \/>\nSN2018zd: a promising candidate of Electron Capture Supernova Progress of light curve modeling<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker1] Kuria Watanabe SOKENDAI 1st year (M1) (Supervisor: Masami Ouchi, Nozomu Tominaga, Masato Onodera) [ [&hellip;]<\/p>\n","protected":false},"author":2,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[6,2],"tags":[],"class_list":["post-1798","post","type-post","status-publish","format-standard","hentry","category-6","category-2"],"_links":{"self":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/1798","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=1798"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/1798\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=1798"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=1798"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=1798"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}