{"id":1096,"date":"2019-06-12T11:00:07","date_gmt":"2019-06-12T02:00:07","guid":{"rendered":"https:\/\/guas-astronomy.jp\/weblog\/?p=1096"},"modified":"2019-07-08T15:28:19","modified_gmt":"2019-07-08T06:28:19","slug":"doppler-tomographic-analysis-for-planetary-orbital-precession-of-wasp-33b-constraint-on-the-rates-of-gas-inflow-and-outflow-of-star-forming-galaxies-at-redshift-of-1-4-based-on-chemical-evolution","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=1096","title":{"rendered":"Constraint on the rates of gas inflow and outflow of star-forming galaxies at redshift of 1.4 based on chemical evolution \/ Doppler Tomographic Analysis for Planetary Orbital Precession of WASP-33b"},"content":{"rendered":"\n<p>[Speaker1]<\/p>\n\n\n\n<p>Nao Fukagawa, <br>\nSOKENDAI 5th year (D3) <br>\n(Supervisors:Tadayuki Kodama (Tohoku university), Wako Aoki, Daisuke Iono, Masato Onodera)<\/p>\n\n\n\n<p>[Title1]<\/p>\n\n\n\n<p>Constraint on the rates of gas inflow and outflow of star-forming galaxies at redshift of 1.4 based on chemical evolution<\/p>\n\n\n\n<p>[Speaker2]<\/p>\n\n\n\n<p>Noriharu Watanabe, <br>\nSOKENDAI 4th year (D2) <br>\n(Supervisors: Norio Narita, Hideki Takami, Wako Aoki)<\/p>\n\n\n\n<p>[Title2]<\/p>\n\n\n\n<p>Doppler Tomographic Analysis for Planetary Orbital Precession of WASP-33b<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker1] Nao Fukagawa, SOKENDAI 5th year (D3) (Supervisors:Tadayuki Kodama (Tohoku university), Wako Aoki, D [&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-1096","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\/1096","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=1096"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/1096\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=1096"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=1096"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=1096"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}