{"id":1590,"date":"2021-06-30T16:04:44","date_gmt":"2021-06-30T07:04:44","guid":{"rendered":"https:\/\/guas-astronomy.jp\/weblog\/?p=1590"},"modified":"2021-06-30T16:04:44","modified_gmt":"2021-06-30T07:04:44","slug":"towards-predicting-the-mass-range-of-core-collapse-supernovae-using-1d-simulations-development-of-a-new-concept-single-mode-fiber-high-resolution-spectrograph","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=1590","title":{"rendered":"Towards predicting the mass range of core-collapse supernovae using 1D+ simulations \/ Development of a new concept single-mode fiber high-resolution spectrograph"},"content":{"rendered":"<p>[Speaker1]<br \/>\nShunsuke Sasaki<br \/>\nSOKENDAI 2nd year (M2)<br \/>\n(Supervisor: Tomoya Takiwaki, Mami Machida, Takashi Moriya)<br \/>\n[Title1]<br \/>\nTowards predicting the mass range of core-collapse supernovae using<br \/>\n1D+ simulations<\/p>\n<p>[Speaker2]<br \/>\nShotaro Tada<br \/>\nSOKENDAI 2nd year (M2)<br \/>\n(Supervisor: Takayuki Kotani, Yutaka Hayano, Yosuke Minowa)<br \/>\n[Title2]<br \/>\nDevelopment of a new concept single-mode fiber high-resolution spectrograph<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker1] Shunsuke Sasaki SOKENDAI 2nd year (M2) (Supervisor: Tomoya Takiwaki, Mami Machida, Takashi Moriya)  [&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-1590","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\/1590","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=1590"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/1590\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=1590"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=1590"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=1590"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}