{"id":871,"date":"2018-05-10T13:54:28","date_gmt":"2018-05-10T04:54:28","guid":{"rendered":"http:\/\/guas-astronomy.jp\/weblog\/?p=871"},"modified":"2018-05-10T13:54:28","modified_gmt":"2018-05-10T04:54:28","slug":"the-current-understanding-of-the-stellar-differential-rotation-doppler-tomographic-measurement-for-orbital-precession-of-wasp-33b","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=871","title":{"rendered":"The current understanding of the stellar differential rotation \/ Doppler Tomographic Measurement for Orbital Precession of WASP-33b"},"content":{"rendered":"<p>[Speaker1]<br \/>\nYoshiki Hatta, SOKENDAI: D1 (Supervisor : Takashi Sekii , Tetsuya Watanabe, Yukio Katsukawa)<br \/>\n[Title]<br \/>\nThe current understanding of the stellar differential rotation<\/p>\n<p>[Speaker2]<br \/>\nNoriharu Watanabe, SOKENDAI: D1 (Supervisor : Motohide Usuda, Norio Narita)<br \/>\n[Title]<br \/>\nDoppler Tomographic Measurement for Orbital Precession of WASP-33b<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker1] Yoshiki Hatta, SOKENDAI: D1 (Supervisor : Takashi Sekii , Tetsuya Watanabe, Yukio Katsukawa) [Title [&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-871","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\/871","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=871"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/871\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=871"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=871"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=871"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}