{"id":78,"date":"2019-04-19T16:22:47","date_gmt":"2019-04-19T14:22:47","guid":{"rendered":"https:\/\/www.oa-roma.inaf.it\/santini\/?page_id=78"},"modified":"2022-10-03T00:51:05","modified_gmt":"2022-10-02T22:51:05","slug":"collaborations","status":"publish","type":"page","link":"https:\/\/www.oa-roma.inaf.it\/santini\/collaborations\/","title":{"rendered":"Main collaborations"},"content":{"rendered":"\n<p class=\"has-text-align-left has-medium-font-size\">I am or have been involved in the following collaborations:<\/p>\n\n\n\n<ul class=\"wp-block-list\"><li><strong><a href=\"https:\/\/glass.astro.ucla.edu\/ers\/\">GLASS<\/a><\/strong>: JWST-ERS program (PI T. Treu) aimed at studying the early Universe with the NIRCam, NIRSpec and NIRISS instruments; it is the deepest extragalactic ERS program with NIRCam.<\/li><li><strong><a href=\"https:\/\/ceers.github.io\/\">CEERS<\/a><\/strong>: JWST-ERS program (PI S. Finkelstein) observing 100 sq. arcmin with JWST imaging and spectroscopy using NIRCam, MIRI, and NIRSpec.<\/li><li><strong><a href=\"https:\/\/primer-jwst.github.io\/\">PRIMER<\/a><\/strong>: JWST Cycle 1 public Treasury Program (PI J. Dunlop) designed to provide the astronomical community with an early, large-area, homogenous, deep JWST NIRCam+MIRI imaging survey.<\/li><li><strong><a rel=\"noreferrer noopener\" aria-label=\" (si apre in una nuova scheda)\" href=\"http:\/\/www.astrodeep.eu\/\" target=\"_blank\">ASTRODEEP<\/a><\/strong>: FP7-SPACE project (PI A. Fontana) aimed at building consistent multiwavelength catalogues (from X-ray to far-IR) in the major extragalactic fields with the most advanced techniques and exploit them for studying galaxy evolution.<\/li><li><strong>SPICA Galaxy Evolution Working Group<\/strong>: <a rel=\"noreferrer noopener\" href=\"https:\/\/spica-mission.org\/\" target=\"_blank\">SPICA<\/a> (an infrared space observatory with a 2.5m actively cooled mirror) was a joint European-Japanese project that had been selected as one of three candidates for the ESA Cosmic Vision M5 mission. <\/li><li><strong><a rel=\"noreferrer noopener\" href=\"http:\/\/candels.ucolick.org\/\" target=\"_blank\">CANDELS<\/a><\/strong>: the Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey (PIs S. Faber and H. Ferguson) is the widest HST program (902 orbits) ever approved, mostly finalised to study the distant Universe.<\/li><li><strong><a rel=\"noreferrer noopener\" href=\"http:\/\/www.mpe.mpg.de\/ir\/Research\/PEP\/index.html\" target=\"_blank\">PEP<\/a><\/strong>: PACS Evolutionary Probe (PI D. Lutz) is a Herschel guaranteed time key program survey of the extragalactic sky with the PACS instrument, aimed at studying the rest-frame far-IR emission of galaxies up to redshift ~3.<\/li><li><a rel=\"noreferrer noopener\" href=\"http:\/\/oberon.roma1.infn.it\/boomerang\/b2k\/\" target=\"_blank\"><strong>BOOMERanG<\/strong><\/a>: a microwave telescope on board of a stratospheric balloon to map the intensity and polarization of the CMB (PIs P. de Bernardis and A. Lange).<\/li><\/ul>\n\n\n\n<div class=\"wp-block-image\"><figure class=\"alignright size-large is-resized\"><img decoding=\"async\" src=\"https:\/\/www.oa-roma.inaf.it\/santini\/wp-content\/uploads\/sites\/12\/2022\/10\/primer_v6_trimmed-edited.png\" alt=\"\" class=\"wp-image-275\" width=\"169\" srcset=\"https:\/\/www.oa-roma.inaf.it\/santini\/wp-content\/uploads\/sites\/12\/2022\/10\/primer_v6_trimmed-edited.png 1190w, https:\/\/www.oa-roma.inaf.it\/santini\/wp-content\/uploads\/sites\/12\/2022\/10\/primer_v6_trimmed-edited-203x300.png 203w, https:\/\/www.oa-roma.inaf.it\/santini\/wp-content\/uploads\/sites\/12\/2022\/10\/primer_v6_trimmed-edited-693x1024.png 693w, https:\/\/www.oa-roma.inaf.it\/santini\/wp-content\/uploads\/sites\/12\/2022\/10\/primer_v6_trimmed-edited-768x1135.png 768w, https:\/\/www.oa-roma.inaf.it\/santini\/wp-content\/uploads\/sites\/12\/2022\/10\/primer_v6_trimmed-edited-1040x1536.png 1040w\" sizes=\"(max-width: 1190px) 100vw, 1190px\" \/><\/figure><\/div>\n\n\n\n<div class=\"wp-block-image\"><figure class=\"aligncenter size-full is-resized\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/www.oa-roma.inaf.it\/santini\/wp-content\/uploads\/sites\/12\/2022\/10\/ceers_logo.jpeg\" alt=\"\" class=\"wp-image-273\" width=\"185\" height=\"188\" \/><\/figure><\/div>\n\n\n\n<div class=\"wp-block-image\"><figure class=\"alignleft is-resized\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/www.oa-roma.inaf.it\/santini\/wp-content\/uploads\/sites\/12\/2019\/04\/LogoAD-300x179.jpg\" alt=\"\" class=\"wp-image-119\" width=\"197\" height=\"118\" \/><\/figure><\/div>\n\n\n\n<figure class=\"wp-block-image is-resized\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/www.oa-roma.inaf.it\/santini\/wp-content\/uploads\/sites\/12\/2019\/04\/candels.jpg\" alt=\"\" class=\"wp-image-118\" width=\"164\" height=\"150\" \/><\/figure>\n\n\n\n<div class=\"wp-block-image\"><figure class=\"alignright\"><img loading=\"lazy\" decoding=\"async\" width=\"136\" height=\"137\" src=\"https:\/\/www.oa-roma.inaf.it\/santini\/wp-content\/uploads\/sites\/12\/2019\/04\/pep.jpg\" alt=\"\" class=\"wp-image-120\" \/><\/figure><\/div>\n\n\n\n<div class=\"wp-block-image\"><figure class=\"alignright is-resized\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/www.oa-roma.inaf.it\/santini\/wp-content\/uploads\/sites\/12\/2019\/04\/SPICA.logo_.gif\" alt=\"\" class=\"wp-image-164\" width=\"242\" height=\"40\" \/><\/figure><\/div>\n\n\n\n<div class=\"wp-block-image\"><figure class=\"alignright is-resized\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/www.oa-roma.inaf.it\/santini\/wp-content\/uploads\/sites\/12\/2019\/04\/BmLogo_Col.jpg\" alt=\"\" class=\"wp-image-122\" width=\"168\" height=\"152\" \/><\/figure><\/div>\n\n\n\n<p><\/p>\n","protected":false},"excerpt":{"rendered":"<p>I am or have been involved in the following collaborations: GLASS: JWST-ERS program (PI T. Treu) aimed at studying the early Universe with the NIRCam, NIRSpec and NIRISS instruments; it is the deepest extragalactic ERS program with NIRCam. CEERS: JWST-ERS &hellip; <a href=\"https:\/\/www.oa-roma.inaf.it\/santini\/collaborations\/\">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-78","page","type-page","status-publish","hentry"],"acf":[],"_links":{"self":[{"href":"https:\/\/www.oa-roma.inaf.it\/santini\/wp-json\/wp\/v2\/pages\/78","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=78"}],"version-history":[{"count":55,"href":"https:\/\/www.oa-roma.inaf.it\/santini\/wp-json\/wp\/v2\/pages\/78\/revisions"}],"predecessor-version":[{"id":276,"href":"https:\/\/www.oa-roma.inaf.it\/santini\/wp-json\/wp\/v2\/pages\/78\/revisions\/276"}],"wp:attachment":[{"href":"https:\/\/www.oa-roma.inaf.it\/santini\/wp-json\/wp\/v2\/media?parent=78"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}