[Speaker1]
\nShuichiro Tsuda, SOKENDAI 1st year (M1)(Supervisor: \u672c\u9593\u5e0c\u6a39,\u79e6\u548c\u5f18,\u67f4\u7530\u514b\u5178)
\n[Title]
\nResolved magnetic-field structure and variability near the event horizon of Sgr A* <\/p>\n
[Speaker2]
\nJungha Kim, SOKENDAI 4th year (D2)(Supervisor: \u672c\u9593\u5e0c\u6a39,\u5ee3\u7530\u667a\u4e5f,\u67f4\u7530\u514b\u5178)
\n[Title]
\nDynamics of jets\/outflows from high-mass young stellar objects revealed by KaVA and ALMA observations <\/p>\n
[Speaker3]
\nSatoshi Kikuta, SOKENDAI 3rd year (D1)(Supervisor: Masatoshi Imanishi,Yuichi Matsuda,Yutaka Komiyama)
\n[Title]
\nLyman Alpha Imaging around a Hyperluminous QSO at z=2.84
\n[Abstract]
\nLy-alpha imaging is a powerful technique to study galaxy formation at high-redshift by detecting redshifted Ly-alpha emission line with narrowband filters. I present the latest results of our Ly-alpha imaging around a hyperluminous QSO at z=2.84, namely HS1549+1919, with HSC\/Subaru. We have detected >3400 LAEs within 36 arcmin from the QSO (i.e., ~1.1 deg^2 FoV). The QSO is found to reside in the center of massive overdensity of LAEs which is embedded within a large scale (~100 cMpc) structure of LAEs. We have also detected a gigantic Ly-alpha nebula around the QSO as well as many Ly-alpha blobs. The nebula is the largest and the most luminous to date and has a peculiar morphology: bubble-like structure extending several hundred kpc. After sharing the current status I present our future plans to further reveal galaxy formation in this rich environment. Your comments and suggestions are very welcome.<\/p>\n","protected":false},"excerpt":{"rendered":"
[Speaker1] Shuichiro Tsuda, SOKENDAI 1st year (M1)(Supervisor: \u672c\u9593\u5e0c\u6a39,\u79e6\u548c\u5f18,\u67f4\u7530\u514b\u5178) [Title] Resolved magnetic-field […]<\/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-818","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\/818","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=818"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/818\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=818"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=818"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=818"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}