{"id":1403,"date":"2020-10-21T13:00:51","date_gmt":"2020-10-21T04:00:51","guid":{"rendered":"https:\/\/guas-astronomy.jp\/weblog\/?p=1403"},"modified":"2020-10-21T10:27:42","modified_gmt":"2020-10-21T01:27:42","slug":"the-environment-of-ly%ce%b1-emitters-massive-star-forming-and-quiescent-galaxies-simulating-the-effect-of-aberrations-on-beam-patterns-for-radio-telescopes","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=1403","title":{"rendered":"The environment of Ly\u03b1 emitters, massive star forming and quiescent galaxies \/ Simulating the Effect of Aberrations on Beam Patterns for Radio Telescopes"},"content":{"rendered":"<p>[Speaker1]<br \/>\nKei Ito<br \/>\nSOKENDAI 4th year (D2)<br \/>\n(Supervisor: Masayuki Tanaka, Nobunari Kashikawa, Yuichi Matsuda, Yusei Koyama)<br \/>\n[Title1]<br \/>\nThe environment of Ly\u03b1 emitters, massive star forming and quiescent galaxies<\/p>\n<p>[Speaker2]<br \/>\nTakaho Masai<br \/>\nSOKENDAI 2nd year (M2)<br \/>\n(Supervisor: Alvaro Gonzalez, Yoshinori Uzawa, Takafumi Kojima)<br \/>\n[Title2]<br \/>\nSimulating the Effect of Aberrations on Beam Patterns for Radio Telescopes<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker1] Kei Ito SOKENDAI 4th year (D2) (Supervisor: Masayuki Tanaka, Nobunari Kashikawa, Yuichi Matsuda, Yu [&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-1403","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\/1403","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=1403"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/1403\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=1403"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=1403"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=1403"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}