{"id":74,"date":"2019-04-19T12:07:33","date_gmt":"2019-04-19T10:07:33","guid":{"rendered":"https:\/\/www.oa-roma.inaf.it\/santini\/?page_id=74"},"modified":"2022-10-03T00:27:02","modified_gmt":"2022-10-02T22:27:02","slug":"publications","status":"publish","type":"page","link":"https:\/\/www.oa-roma.inaf.it\/santini\/publications\/","title":{"rendered":"Publications"},"content":{"rendered":"\n<p class=\"has-medium-font-size\">Main publications:<\/p>\n\n\n\n<ul class=\"wp-block-list\"><li><a rel=\"noreferrer noopener\" aria-label=\"Passive galaxies in the early Universe: ALMA confirmation of z ~ 3-5 candidates in the CANDELS GOODS-South field (si apre in una nuova scheda)\" href=\"https:\/\/www.oa-roma.inaf.it\/santini\/wp-content\/uploads\/sites\/12\/2019\/04\/santini19.pdf\" target=\"_blank\">Early results from GLASS-JWST. XI: Stellar masses and mass-to-light ratio of z &gt; 7 galaxies<\/a> (Santini et al. 2022, ApJL, in press)<\/li><li><a rel=\"noreferrer noopener\" aria-label=\"Passive galaxies in the early Universe: ALMA confirmation of z ~ 3-5 candidates in the CANDELS GOODS-South field (si apre in una nuova scheda)\" href=\"https:\/\/www.oa-roma.inaf.it\/santini\/wp-content\/uploads\/sites\/12\/2019\/04\/santini19.pdf\" target=\"_blank\">Passive galaxies in the early Universe: ALMA confirmation of z ~ 3-5 candidates in the CANDELS GOODS-South field<\/a> (Santini et al. 2019, MNRAS, 486, 560)<\/li><li><a href=\"https:\/\/www.oa-roma.inaf.it\/santini\/wp-content\/uploads\/sites\/12\/2019\/04\/santini17.pdf\">The Star Formation Main Sequence in the Hubble Space Telescope Frontier Fields<\/a>  (Santini et al. 2017, ApJ, 847, 76)<\/li><li><a rel=\"noreferrer noopener\" aria-label=\" (si apre in una nuova scheda)\" href=\"https:\/\/www.oa-roma.inaf.it\/santini\/wp-content\/uploads\/sites\/12\/2019\/04\/santini16.pdf\" target=\"_blank\">Characterizing elusive, faint dusty star-forming galaxies: a lensed, optically undetected ALMA galaxy at z \u223c 3.3<\/a> (Santini et al. 2016, A&amp;A, 596, A75)<\/li><li><a rel=\"noreferrer noopener\" aria-label=\" (si apre in una nuova scheda)\" href=\"https:\/\/www.oa-roma.inaf.it\/santini\/wp-content\/uploads\/sites\/12\/2019\/04\/santini15.pdf\" target=\"_blank\">Stellar Masses from the CANDELS Survey: The GOODS-South and UDS Fields<\/a>  (Santini et al. 2015, ApJ, 801, 97)<\/li><li><a rel=\"noreferrer noopener\" aria-label=\" (si apre in una nuova scheda)\" href=\"https:\/\/www.oa-roma.inaf.it\/santini\/wp-content\/uploads\/sites\/12\/2019\/04\/santini14.pdf\" target=\"_blank\">The evolution of the dust and gas content in galaxies<\/a> (Santini et al. 2014, A&amp;A, 562, A30)<\/li><li><a rel=\"noreferrer noopener\" aria-label=\" (si apre in una nuova scheda)\" href=\"https:\/\/www.oa-roma.inaf.it\/santini\/wp-content\/uploads\/sites\/12\/2019\/04\/santini12b.pdf\" target=\"_blank\">Enhanced star formation rates in AGN hosts with respect to inactive galaxies from PEP-Herschel observations<\/a> (Santini et al. 2012, A&amp;A, 540, A109)<\/li><li><a rel=\"noreferrer noopener\" aria-label=\" (si apre in una nuova scheda)\" href=\"https:\/\/www.oa-roma.inaf.it\/santini\/wp-content\/uploads\/sites\/12\/2019\/04\/santini12a.pdf\" target=\"_blank\">The evolving slope of the stellar mass function at 0.6 \u2264 z &lt; 4.5 from deep WFC3 data<\/a> (Santini et al. 2012, A&amp;A, 538, A33)<\/li><li><a rel=\"noreferrer noopener\" aria-label=\" (si apre in una nuova scheda)\" href=\"https:\/\/www.oa-roma.inaf.it\/santini\/wp-content\/uploads\/sites\/12\/2019\/04\/santini10.pdf\" target=\"_blank\">The dust content of high-z submillimeter galaxies revealed by Herschel<\/a> (Santini et al. 2010, A&amp;A, 518, L154)<\/li><li><a rel=\"noreferrer noopener\" aria-label=\" (si apre in una nuova scheda)\" href=\"https:\/\/www.oa-roma.inaf.it\/santini\/wp-content\/uploads\/sites\/12\/2019\/04\/santini09.pdf\" target=\"_blank\">Star formation and mass assembly in high redshift galaxies<\/a> (Santini et al. 2009, A&amp;A, 504, 751)<\/li><\/ul>\n\n\n\n<p class=\"has-medium-font-size\">The full list of my publications is available <a href=\"http:\/\/ui.adsabs.harvard.edu\/public-libraries\/qkWQYlLYQ2Cysh6SKOLSpw\" target=\"_blank\" rel=\"noreferrer noopener\" aria-label=\" (si apre in una nuova scheda)\">here<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Main publications: Early results from GLASS-JWST. XI: Stellar masses and mass-to-light ratio of z &gt; 7 galaxies (Santini et al. 2022, ApJL, in press) Passive galaxies in the early Universe: ALMA confirmation of z ~ 3-5 candidates in the CANDELS &hellip; <a href=\"https:\/\/www.oa-roma.inaf.it\/santini\/publications\/\">Continua a leggere<span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":113,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"_acf_changed":false,"footnotes":""},"class_list":["post-74","page","type-page","status-publish","hentry"],"acf":[],"_links":{"self":[{"href":"https:\/\/www.oa-roma.inaf.it\/santini\/wp-json\/wp\/v2\/pages\/74","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.oa-roma.inaf.it\/santini\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.oa-roma.inaf.it\/santini\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.oa-roma.inaf.it\/santini\/wp-json\/wp\/v2\/users\/113"}],"replies":[{"embeddable":true,"href":"https:\/\/www.oa-roma.inaf.it\/santini\/wp-json\/wp\/v2\/comments?post=74"}],"version-history":[{"count":14,"href":"https:\/\/www.oa-roma.inaf.it\/santini\/wp-json\/wp\/v2\/pages\/74\/revisions"}],"predecessor-version":[{"id":267,"href":"https:\/\/www.oa-roma.inaf.it\/santini\/wp-json\/wp\/v2\/pages\/74\/revisions\/267"}],"wp:attachment":[{"href":"https:\/\/www.oa-roma.inaf.it\/santini\/wp-json\/wp\/v2\/media?parent=74"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}