{"id":1041,"date":"2018-11-07T00:00:10","date_gmt":"2018-11-06T15:00:10","guid":{"rendered":"https:\/\/guas-astronomy.jp\/weblog\/?p=1041"},"modified":"2019-07-08T15:44:16","modified_gmt":"2019-07-08T06:44:16","slug":"chemical-abundances-and-kinematics-of-metal-poor-stars-study-the-correlation-between-galaxies-and-intergalactic-gas-at-tens-of-mpc-scale-at-z2-2-using-subaru-hsc","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=1041","title":{"rendered":"Chemical abundances and kinematics of metal-poor stars \/ Study the correlation between galaxies and intergalactic gas at tens of Mpc scale at z~2.2 using Subaru\/HSC"},"content":{"rendered":"<p>[Speaker1]<br \/>\nT. Matsuno,<br \/>\nSOKENDAI 4th year (D2)<br \/>\n(Supervisor: W. Aoki,T. Tsujimoto,Y. Komiyama)<\/p>\n<p>[Title1]<br \/>\nThe research for hot Jupiters around hot stars<\/p>\n<p>[Speaker2]<br \/>\nYongming Liang<br \/>\nSOKENDAI 2nd year (M2)<br \/>\n(Supervisor: Masayuki Tanaka, Yuichi Matsuda, Yutaka Komiyama)<\/p>\n<p>[Title2]<br \/>\nStudy the correlation between galaxies and intergalactic gas at tens of Mpc scale at z~2.2 using Subaru\/HSC<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker1] T. Matsuno, SOKENDAI 4th year (D2) (Supervisor: W. Aoki,T. Tsujimoto,Y. Komiyama) [Title1] The rese [&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-1041","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\/1041","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=1041"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/1041\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=1041"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=1041"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=1041"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}