{"id":2,"date":"2026-04-14T21:25:30","date_gmt":"2026-04-14T12:25:30","guid":{"rendered":"http:\/\/sagadatabase.jp\/?page_id=2"},"modified":"2026-04-20T12:40:30","modified_gmt":"2026-04-20T03:40:30","slug":"sample-page","status":"publish","type":"page","link":"http:\/\/sagadatabase.jp\/index.php\/sample-page\/","title":{"rendered":"Data"},"content":{"rendered":"\n<ul class=\"wp-block-list\">\n<li><a href=\".\/List\/list.cgi\">List of Papers<\/a><\/li>\n\n\n\n<li><a href=\".\/Data\/starlist.html\">List of Objects<\/a>\n<ul class=\"wp-block-list\">\n<li>Updated on Jan 20, 2026<\/li>\n<\/ul>\n<\/li>\n\n\n\n<li><a href=\".\/Data\/txt_table_recommended.tsv\">Text data in tsv format (all the records)<\/a>\n<ul class=\"wp-block-list\">\n<li>Version Jan 20, 2026<\/li>\n\n\n\n<li>Abundances are in units of [X\/H] (including Li where we adopted A(Li) = 3.26) normalized by the solar abundances of Asplund et al. (2009).<\/li>\n\n\n\n<li>d(X) and f(X) stands for uncertainties and upper limits for element X, respectively.<\/li>\n\n\n\n<li>New columns: Facility, Resolution, SN, Solar Abundance\n<ul class=\"wp-block-list\">\n<li>Facility: observational facilities used to take spectra<\/li>\n\n\n\n<li>Resolution: the highest resolving power obtained to take spectra<\/li>\n\n\n\n<li>SN: the range of signal-to-noise ratio obtained to take spectra<\/li>\n\n\n\n<li>Solar Abundance: solar abundances adopted to derive [X\/H] or log-e(X) in the original paper<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<\/li>\n\n\n\n<li><a href=\".\/Data\/txt_table_recommended.tsv\">Text data in tsv format (recommended data set)<\/a>\n<ul class=\"wp-block-list\">\n<li>Version April 7, 2026\n<ul class=\"wp-block-list\">\n<li class=\"has-text-color has-link-color wp-elements-ccc400013b8a16896c38df7043f3bfc0\" style=\"color:#ff0000\">Some stars in the database were not correctly identified as the same objects when assigned different identifiers. This issue has been resolved in the current version.<\/li>\n<\/ul>\n<\/li>\n\n\n\n<li>Abundances are in units of [X\/H] (including Li where we adopted A(Li) = 3.26) normalized by the solar abundances of Asplund et al. (2009).<\/li>\n\n\n\n<li>Recommended list of data, provided by one record for one star, following our priority parameter. See SAGA paper series IV for the definition of the priority parameter.<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n\n\n\n<p><\/p>\n","protected":false},"excerpt":{"rendered":"","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"open","template":"","meta":{"footnotes":""},"class_list":["post-2","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"http:\/\/sagadatabase.jp\/index.php\/wp-json\/wp\/v2\/pages\/2","targetHints":{"allow":["GET"]}}],"collection":[{"href":"http:\/\/sagadatabase.jp\/index.php\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"http:\/\/sagadatabase.jp\/index.php\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"http:\/\/sagadatabase.jp\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"http:\/\/sagadatabase.jp\/index.php\/wp-json\/wp\/v2\/comments?post=2"}],"version-history":[{"count":4,"href":"http:\/\/sagadatabase.jp\/index.php\/wp-json\/wp\/v2\/pages\/2\/revisions"}],"predecessor-version":[{"id":24,"href":"http:\/\/sagadatabase.jp\/index.php\/wp-json\/wp\/v2\/pages\/2\/revisions\/24"}],"wp:attachment":[{"href":"http:\/\/sagadatabase.jp\/index.php\/wp-json\/wp\/v2\/media?parent=2"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}