{"id":43,"date":"2020-02-04T11:03:23","date_gmt":"2020-02-04T10:03:23","guid":{"rendered":"https:\/\/www.issibern.ch\/teams\/pristine\/?page_id=43"},"modified":"2020-02-04T11:03:23","modified_gmt":"2020-02-04T10:03:23","slug":"publications","status":"publish","type":"page","link":"https:\/\/www.issibern.ch\/teams\/pristine\/publications\/","title":{"rendered":"Publications"},"content":{"rendered":"<ul class=\"n8H08c UVNKR\">\n<li id=\"h.p_oEXfs1JwfmX7\" class=\"TYR86d zfr3Q\"><a class=\"dhtgD aw5Odc\" href=\"http:\/\/www.google.com\/url?q=http%3A%2F%2Fadsabs.harvard.edu%2Fabs%2F2017MNRAS.471.2587S&amp;sa=D&amp;sntz=1&amp;usg=AFQjCNHI7WSlSGU3zDImfKk0frGL3ABm5g\" target=\"_blank\" rel=\"noopener noreferrer\">The Pristine survey &#8211; I. Mining the Galaxy for the most metal-poor stars<\/a>(Starkenburg, Martin et al. 2017)<\/li>\n<li id=\"h.p_fJDHO9zgfKN6\" class=\"TYR86d zfr3Q\"><a class=\"dhtgD aw5Odc\" href=\"http:\/\/www.google.com\/url?q=http%3A%2F%2Fadsabs.harvard.edu%2Fabs%2F2017AN....338..686C&amp;sa=D&amp;sntz=1&amp;usg=AFQjCNHxeG-91fVwdJI4YsyQAiePQEx8kA\" target=\"_blank\" rel=\"noopener noreferrer\">The Pristine survey II: A sample of bright stars observed with FEROS<\/a>(Caffau et al. 2017)<\/li>\n<li id=\"h.p_uW0CzJL9fR6u\" class=\"TYR86d zfr3Q\"><a class=\"dhtgD aw5Odc\" href=\"http:\/\/www.google.com\/url?q=http%3A%2F%2Fadsabs.harvard.edu%2Fabs%2F2017MNRAS.472.2963Y&amp;sa=D&amp;sntz=1&amp;usg=AFQjCNHpkww03NNU3hLhPdThBh5F4_hDzA\" target=\"_blank\" rel=\"noopener noreferrer\">The Pristine survey &#8211; III. Spectroscopic confirmation of an efficient search for extremely metal-poor stars<\/a>(Youakim et al. 2017)<\/li>\n<li id=\"h.p_DBZbN022ffRB\" class=\"TYR86d zfr3Q\"><a class=\"dhtgD aw5Odc\" href=\"http:\/\/www.google.com\/url?q=http%3A%2F%2Fadsabs.harvard.edu%2Fabs%2F2018MNRAS.481.3838S&amp;sa=D&amp;sntz=1&amp;usg=AFQjCNF9Jz5Wl9_5rgzUPFJpsdtAxOWi2Q\" target=\"_blank\" rel=\"noopener noreferrer\">The Pristine survey IV: approaching the Galactic metallicity floor with the discovery of an ultra-metal-poor star<\/a>(Starkenburg et al. 2018)<\/li>\n<li id=\"h.p_B7Xth5BW7mQT\" class=\"TYR86d zfr3Q\"><a class=\"dhtgD aw5Odc\" href=\"https:\/\/www.google.com\/url?q=https%3A%2F%2Fui.adsabs.harvard.edu%2Fabs%2F2019MNRAS.487.3797B%2Fabstract&amp;sa=D&amp;sntz=1&amp;usg=AFQjCNE_KR9jbYkekRKpBsW53gc73b19Zw\" target=\"_blank\" rel=\"noopener noreferrer\">The Pristine survey &#8211; V. A bright star sample observed with SOPHIE<\/a>(Bonifacio et al. 2019)<\/li>\n<li id=\"h.p_7mI49FMsE3Ir\" class=\"TYR86d zfr3Q\"><a class=\"dhtgD aw5Odc\" href=\"https:\/\/www.google.com\/url?q=https%3A%2F%2Fui.adsabs.harvard.edu%2Fabs%2F2019MNRAS.490.2241A%2Fabstract&amp;sa=D&amp;sntz=1&amp;usg=AFQjCNE3MTD9NGR9cb983BH1xO5wYgp4AQ\" target=\"_blank\" rel=\"noopener noreferrer\">The Pristine survey &#8211; VI. The first three years of medium-resolution follow-up spectroscopy of Pristine EMP star candidates<\/a>(Aguado, Youakim et al. 2019)<\/li>\n<li id=\"h.p_5P_N-HsgxbtE\" class=\"TYR86d zfr3Q\"><a class=\"dhtgD aw5Odc\" href=\"https:\/\/www.google.com\/url?q=https%3A%2F%2Fui.adsabs.harvard.edu%2Fabs%2F2019MNRAS.490.5757S%2Fabstract&amp;sa=D&amp;sntz=1&amp;usg=AFQjCNGE09GS-ObzFL_SPLce8nZC4pMyqw\" target=\"_blank\" rel=\"noopener noreferrer\">The Pristine survey &#8212; VII. A cleaner view of the Galactic outer halo using blue horizontal branch stars<\/a>(Starkenburg et al. 2019)<\/li>\n<li id=\"h.p_nR0jZu5Ixb-S\" class=\"TYR86d zfr3Q\"><a class=\"dhtgD aw5Odc\" href=\"https:\/\/www.google.com\/url?q=https%3A%2F%2Fui.adsabs.harvard.edu%2Fabs%2F2020arXiv200104988Y%2Fabstract&amp;sa=D&amp;sntz=1&amp;usg=AFQjCNFxnwhOhOPAfd5qmiEcA4o7fmmRew\" target=\"_blank\" rel=\"noopener noreferrer\">The Pristine Survey &#8211; VIII. The metallicity distribution function of the Milky Way halo down to the extremely metal-poor regime<\/a>(Youakim et al. 2020)<\/li>\n<li id=\"h.p_yIrzIYp_xcKr\" class=\"TYR86d zfr3Q\"><a class=\"dhtgD aw5Odc\" href=\"https:\/\/www.google.com\/url?q=https%3A%2F%2Fui.adsabs.harvard.edu%2Fabs%2F2019MNRAS.tmp.3190V%2Fabstract&amp;sa=D&amp;sntz=1&amp;usg=AFQjCNF-Hw-_CfSgXs_48PJV2MP5V2EYYg\" target=\"_blank\" rel=\"noopener noreferrer\">The Pristine survey &#8211; IX. CFHT ESPaDOnS Spectroscopic Analysis of 115 Bright Metal-Poor Candidate Stars<\/a>(Venn et al. 2019)<\/li>\n<li id=\"h.p_F68ojM_eQmds\" class=\"TYR86d zfr3Q\"><a class=\"dhtgD aw5Odc\" href=\"https:\/\/www.google.com\/url?q=https%3A%2F%2Fui.adsabs.harvard.edu%2Fabs%2F2019arXiv191108491S%2Fabstract&amp;sa=D&amp;sntz=1&amp;usg=AFQjCNEDNQUl1TpGLxOVq_Ppey8o66OtRQ\" target=\"_blank\" rel=\"noopener noreferrer\">The Pristine survey X: a large population of low-metallicity stars permeates the Galactic disk<\/a>(Sestito et al., preprint)<\/li>\n<\/ul>\n<div class=\"CjVfdc\">\n<div class=\"PPhIP rviiZ\"><\/div>\n<\/div>\n<div class=\"CjVfdc\">Dwarf galaxy survey:<\/div>\n<ul class=\"n8H08c UVNKR\">\n<li id=\"h.p_dyUOkbdlfjjq\" class=\"TYR86d zfr3Q\"><a class=\"dhtgD aw5Odc\" href=\"http:\/\/www.google.com\/url?q=http%3A%2F%2Fadsabs.harvard.edu%2Fabs%2F2018MNRAS.480.2609L&amp;sa=D&amp;sntz=1&amp;usg=AFQjCNESzOp3F88aSKIM9b2uXCkumiOmaA\" target=\"_blank\" rel=\"noopener noreferrer\">Pristine dwarf galaxy survey &#8211; I. A detailed photometric and spectroscopic study of the very metal-poor Draco II satellite<\/a>(Longeard et al. 2018)<\/li>\n<li id=\"h.p_HhKGNSFG5VOA\" class=\"TYR86d zfr3Q\"><a class=\"dhtgD aw5Odc\" href=\"https:\/\/www.google.com\/url?q=https%3A%2F%2Fui.adsabs.harvard.edu%2Fabs%2F2020MNRAS.491..356L%2Fabstract&amp;sa=D&amp;sntz=1&amp;usg=AFQjCNH68J8AUuiUmmYNGGry3waBG-acTw\" target=\"_blank\" rel=\"noopener noreferrer\">The Pristine Dwarf-Galaxy survey &#8211; II. In-depth observational study of the faint Milky Way satellite Sagittarius II<\/a>(Longeard et al. 2019)<\/li>\n<\/ul>\n<div class=\"CjVfdc\">Pristine Inner Galaxy Survey (PIGS):<\/div>\n<ul>\n<li style=\"list-style-type: none\">\n<ul class=\"n8H08c UVNKR\">\n<li id=\"h.p_jY9iPL5DxTB_\" class=\"TYR86d zfr3Q\"><a class=\"dhtgD aw5Odc\" href=\"https:\/\/www.google.com\/url?q=https%3A%2F%2Fui.adsabs.harvard.edu%2Fabs%2F2020MNRAS.491L..11A%2Fabstract&amp;sa=D&amp;sntz=1&amp;usg=AFQjCNHOt9zs1xOOZPO4eJcDnicMHVLpfw\" target=\"_blank\" rel=\"noopener noreferrer\">The Pristine Inner Galaxy Survey (PIGS) I: Tracing the kinematics of metal-poor stars in the Galactic bulge<\/a>(Arentsen et al. 2019)<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n","protected":false},"excerpt":{"rendered":"<p>The Pristine survey &#8211; I. Mining the Galaxy for the most metal-poor stars(Starkenburg, Martin et al. 2017) The Pristine survey II: A sample of bright stars observed with FEROS(Caffau et al. 2017) The Pristine survey &#8211; III. Spectroscopic confirmation of &hellip; <a href=\"https:\/\/www.issibern.ch\/teams\/pristine\/publications\/\">Continue reading <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":2,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-43","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.issibern.ch\/teams\/pristine\/wp-json\/wp\/v2\/pages\/43","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.issibern.ch\/teams\/pristine\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.issibern.ch\/teams\/pristine\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/pristine\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/pristine\/wp-json\/wp\/v2\/comments?post=43"}],"version-history":[{"count":0,"href":"https:\/\/www.issibern.ch\/teams\/pristine\/wp-json\/wp\/v2\/pages\/43\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.issibern.ch\/teams\/pristine\/wp-json\/wp\/v2\/media?parent=43"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}