{"id":2047,"date":"2023-06-28T12:00:14","date_gmt":"2023-06-28T03:00:14","guid":{"rendered":"https:\/\/guas-astronomy.jp\/weblog\/?p=2047"},"modified":"2023-06-28T09:36:39","modified_gmt":"2023-06-28T00:36:39","slug":"the-chemical-origins-of-nitrogen-rich-galaxy-gn-z11-at-high-redshift-modeling-the-mass-metallicity-relation-with-the-dark-matter-halo-assembly-from-z0-10","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=2047","title":{"rendered":"SOKENDAI Colloquium (2023.6.28)"},"content":{"rendered":"<p>Speaker1 : Kuria Watanabe<br \/>\nAffiliation: SOKENDAI 2nd year (M2)<br \/>\n(Supervisor: Masami Ouchi, Nozomu Tominaga, Masato Onodera)<br \/>\nTitle: The Chemical Origins of Nitrogen-Rich Galaxy GN-z11 at High Redshift<\/p>\n<p>Speaker2 : Moka Nishigaki<br \/>\nAffiliation: SOKENDAI 3rd year (D1)<br \/>\n(Supervisor: Masami Ouchi, Tadafumi Takata, Kimihiko Nakajima)<br \/>\nTitle: Modeling the Mass-Metallicity Relation with the Dark Matter Halo Assembly from z = 0 \u2013 10<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Speaker1 : Kuria Watanabe Affiliation: SOKENDAI 2nd year (M2) (Supervisor: Masami Ouchi, Nozomu Tominaga, Masa [&hellip;]<\/p>\n","protected":false},"author":2,"featured_media":0,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[6,2],"tags":[],"class_list":["post-2047","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\/2047","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=2047"}],"version-history":[{"count":1,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/2047\/revisions"}],"predecessor-version":[{"id":2048,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/2047\/revisions\/2048"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=2047"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=2047"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=2047"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}