{"id":1481,"date":"2020-11-18T16:16:11","date_gmt":"2020-11-18T07:16:11","guid":{"rendered":"https:\/\/guas-astronomy.jp\/weblog\/?p=1481"},"modified":"2020-11-26T09:04:15","modified_gmt":"2020-11-26T00:04:15","slug":"morphological-dependence-of-hi-gas-fraction-across-the-star-formation-main-sequence-simulation-of-a-new-concept-single-mode-fiber-high-resolution-spectrometer","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=1481","title":{"rendered":"Morphological dependence of HI gas fraction across the star-formation main sequence \/ Simulation of a new-concept, single-mode fiber high-resolution spectrometer"},"content":{"rendered":"<p>[Speaker1]<br \/>\nShigeru Namiki<br \/>\nSOKENDAI 4th year (D2)<br \/>\n(Supervisor: Yusei Koyama , Masayuki Tanaka, Masato Onodera )<br \/>\n[Title1]<br \/>\nMorphological dependence of HI gas fraction across the star-formation main sequence<\/p>\n<p>[Speaker2]<br \/>\nShotaro Tada<br \/>\nSOKENDAI 1st year (M1)<br \/>\n(Supervisor: Takayuki Kotani, Yutaka Hayano, Yosuke Minowa)<br \/>\n[Title2]<br \/>\nSimulation of a new-concept, single-mode fiber high-resolution spectrometer<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker1] Shigeru Namiki SOKENDAI 4th year (D2) (Supervisor: Yusei Koyama , Masayuki Tanaka, 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-1481","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\/1481","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=1481"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/1481\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=1481"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=1481"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=1481"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}