{"id":1341,"date":"2020-05-13T10:02:59","date_gmt":"2020-05-13T01:02:59","guid":{"rendered":"https:\/\/guas-astronomy.jp\/weblog\/?p=1341"},"modified":"2020-05-13T10:08:50","modified_gmt":"2020-05-13T01:08:50","slug":"verification-of-detailed-chemical-analysis-for-m-dwarfs-characterization-of-dipper-stars-by-high-dispersion-spectroscopy-and-improvement-of-the-irds-stability","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=1341","title":{"rendered":"Verification of Detailed Chemical Analysis for M Dwarfs \/ Characterization of dipper stars by high-dispersion spectroscopy and improvement of the IRD\u2019s stability"},"content":{"rendered":"<p>[Speaker1]<br \/>\nHiroyuki Tako ISHIKAWA<br \/>\nSOKENDAI 5th year (D3)<br \/>\n(Supervisor: Wako Aoki, Takayuki Kotani, Saeko Hayashi)<\/p>\n<p>[Title1]<br \/>\nVerification of Detailed Chemical Analysis for M Dwarfs<\/p>\n<p>[Speaker2]<br \/>\nYui Kasagi<br \/>\nSOKENDAI 2nd year (M2)<br \/>\n(Supervisor: Takayuki Kotani, Saeko Hayashi, Wako Aoki)<\/p>\n<p>[Title2]<br \/>\nCharacterization of dipper stars by high-dispersion spectroscopy and improvement of the IRD\u2019s stability<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker1] Hiroyuki Tako ISHIKAWA SOKENDAI 5th year (D3) (Supervisor: Wako Aoki, Takayuki Kotani, Saeko Hayash [&hellip;]<\/p>\n","protected":false},"author":2,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[6,2],"tags":[],"class_list":["post-1341","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\/1341","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=1341"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/1341\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=1341"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=1341"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=1341"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}