{"id":1807,"date":"2022-10-12T16:56:44","date_gmt":"2022-10-12T07:56:44","guid":{"rendered":"https:\/\/guas-astronomy.jp\/weblog\/?p=1807"},"modified":"2022-10-12T16:56:44","modified_gmt":"2022-10-12T07:56:44","slug":"search-for-a-planetary-mass-companion-around-a-brown-dwarf-gl-229b-playing-with-gas-kinematics-kinematical-properties-of-co-line-in-z1-5-cluster-galaxies","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=1807","title":{"rendered":"Search for a Planetary-mass Companion around a Brown Dwarf, Gl 229B \/ Playing with Gas Kinematics &#8211; Kinematical properties of CO line in z~1.5 cluster galaxies &#8211;"},"content":{"rendered":"<p>[Speaker1]<br \/>\nYuki Kasagi<br \/>\nSOKENDAI 4th year (D2)<br \/>\n(Supervisor: Takayuki Kotani, Saeko Hayashi, Wako Aoki)<br \/>\n[Title1]<br \/>\nSearch for a Planetary-mass Companion around a Brown Dwarf, Gl 229B<\/p>\n<p>[Speaker2]<br \/>\nRyota Ikeda<br \/>\nSOKENDAI 2nd year (M2)<br \/>\n(Supervisor: Daisuke Iono, Kenichi Tadaki)<br \/>\n[Title2]<br \/>\nPlaying with Gas Kinematics &#8211; Kinematical properties of CO line in z~1.5 cluster galaxies &#8211;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker1] Yuki Kasagi SOKENDAI 4th year (D2) (Supervisor: Takayuki Kotani, Saeko Hayashi, Wako Aoki) [Title1] [&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-1807","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\/1807","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=1807"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/1807\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=1807"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=1807"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=1807"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}