{"id":1311,"date":"2019-12-18T09:10:49","date_gmt":"2019-12-18T00:10:49","guid":{"rendered":"https:\/\/guas-astronomy.jp\/weblog\/?p=1311"},"modified":"2019-12-18T09:10:49","modified_gmt":"2019-12-18T00:10:49","slug":"the-experimental-results-of-fe-xiv-line-ratio-for-the-electron-galactic-dynamics-and-dark-matter-profile-of-ngc1380-with-alma-and-vlt-muse","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=1311","title":{"rendered":"The experimental results of Fe XIV line ratio for the electron \/ Galactic dynamics and Dark Matter Profile of NGC1380 with ALMA and VLT\/MUSE"},"content":{"rendered":"<p>[Speaker1]<br \/>\nNagaaki Kambara<br \/>\nSOKENDAI 5th year (D3)<br \/>\n(Supervisor: Izumi Murakami, Kohji Tomisaka, Hirohisa Hara, Masahito Kubo)<\/p>\n<p>[Title1]<br \/>\nThe experimental results of Fe XIV line ratio for the electron density diagnostics by using  laboratory plasmas<\/p>\n<p>[Speaker2]<br \/>\nTakafumi Tsukui<br \/>\nSOKENDAI 3rd year (D1)<br \/>\n(Supervisor: Satoru Iguchi, Hiroshi Nagai, Yuichi Matsuda)<\/p>\n<p>[Title2]<br \/>\nGalactic dynamics and Dark Matter Profile of NGC1380 with ALMA and VLT\/MUSE<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker1] Nagaaki Kambara SOKENDAI 5th year (D3) (Supervisor: Izumi Murakami, Kohji Tomisaka, Hirohisa Hara,  [&hellip;]<\/p>\n","protected":false},"author":2,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[6,2],"tags":[],"class_list":["post-1311","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\/1311","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=1311"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/1311\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=1311"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=1311"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=1311"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}