{"id":247,"date":"2014-05-21T09:41:57","date_gmt":"2014-05-21T00:41:57","guid":{"rendered":"http:\/\/guas-astronomy.jp\/weblog\/?p=247"},"modified":"2016-06-16T11:34:31","modified_gmt":"2016-06-16T02:34:31","slug":"clustering-properties-of-z2-galaxies-by-extremely-wide-field-galaxy-survey-etc","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=247","title":{"rendered":"clustering properties of z~2 galaxies by extremely wide field galaxy survey etc."},"content":{"rendered":"<p>[Speaker1]<br \/>\nShogo Ishikawa , D1, SOKENDAI, Mitaka(supervisor: Nobunari Kashikawa)<br \/>\n[Title]<br \/>\nclustering properties of z~2 galaxies by extremely wide field galaxy survey <\/p>\n<p>[Speaker2]<br \/>\nMasafusa Onoue , M2, SOKENDAI, Mitaka(supervisor: Nobunari Kashikawa)<br \/>\n[Title]<br \/>\nThe Selection Method for Finding High-z Quasar<br \/>\n[Abstract]<br \/>\nIn this colloquium, I\u2019d like to start with explaining how to estimate redshift of unknown objects, and why it is important. Then, I will show you the progress of the development of effective quasar selection method that I have been working on.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker1] Shogo Ishikawa , D1, SOKENDAI, Mitaka(supervisor: Nobunari Kashikawa) [Title] clustering properties [&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-247","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\/247","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=247"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/247\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=247"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=247"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=247"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}