{"id":703,"date":"2017-01-31T14:32:06","date_gmt":"2017-01-31T05:32:06","guid":{"rendered":"http:\/\/guas-astronomy.jp\/weblog\/?p=703"},"modified":"2017-02-07T14:38:37","modified_gmt":"2017-02-07T05:38:37","slug":"the-galaxy-halo-connection-across-cosmic-history-radiation-mhd-simulation-of-clumpy-outflow-from-supercritical-accretion-flow-s-cam-and-hsc-search-of-z6-quasars","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=703","title":{"rendered":"The Galaxy-Halo Connection Across Cosmic History \/ Radiation-MHD Simulation of Clumpy Outflow from Supercritical Accretion Flow \/ S-Cam and HSC Search of z>6 Quasars"},"content":{"rendered":"<p>[Speaker1]<br \/>\nShogo Ishikawa, D3, SOKENDAI (Supervisor; Nobunari Kashikawa)<br \/>\n[Title]<br \/>\nThe Galaxy-Halo Connection Across Cosmic History<\/p>\n<p>[Speaker2]<br \/>\nHiroshi Kobayashi, D3, SOKENDAI (Supervisor: Ken Ohsuga)<br \/>\n[Title]<br \/>\nRadiation-MHD Simulation of Clumpy Outflow from Supercritical Accretion Flow<\/p>\n<p>[Speaker3]<br \/>\nMasafusa Onoue, D2, SOKENDAI (Supervisor; Nobunari Kashikawa)<br \/>\n[Title]<br \/>\nS-Cam and HSC Search of z>6 Quasars<br \/>\n[Abstract]<br \/>\nI will present several updates on our high-redshift (z>6) quasar search projects using Subaru\/S-Cam and HSC.<br \/>\nIn short, our constraints on the quasar luminosity function at z~6 suggest that quasars have only a moderate contribution on the total photons required to re-ionize the universe at z~6.<br \/>\nFrom the HSC-Wide survey, we have found ~30 low-luminosity quasars<br \/>\nat z>6 in ~100 deg^2 of the HSC-SSP coverage. Their NIR follow-up observation is<br \/>\nnow ongoing with Gemini and VLT, which is for the BH mass and metallicity measurements.<br \/>\nMoreover, the HSC-Deep survey enables us to find much fainter quasar candidates down to z~25 AB mag.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker1] Shogo Ishikawa, D3, SOKENDAI (Supervisor; Nobunari Kashikawa) [Title] The Galaxy-Halo Connection Ac [&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-703","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\/703","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=703"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/703\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=703"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=703"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=703"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}