{"id":94,"date":"2019-03-21T14:00:48","date_gmt":"2019-03-21T14:00:48","guid":{"rendered":"https:\/\/www.oato.inaf.it\/blazars\/webt\/?page_id=94"},"modified":"2019-03-21T14:00:49","modified_gmt":"2019-03-21T14:00:49","slug":"perugia-university-astronomical-observatory-italy","status":"publish","type":"page","link":"https:\/\/www.oato.inaf.it\/blazars\/webt\/perugia-university-astronomical-observatory-italy\/","title":{"rendered":"Perugia University Astronomical Observatory (Italy)"},"content":{"rendered":"<div class=\"pdfprnt-buttons pdfprnt-buttons-page pdfprnt-top-right\"><a href=\"https:\/\/www.oato.inaf.it\/blazars\/webt\/wp-json\/wp\/v2\/pages\/94?print=pdf\" class=\"pdfprnt-button pdfprnt-button-pdf\" target=\"_blank\"><\/a><a href=\"https:\/\/www.oato.inaf.it\/blazars\/webt\/wp-json\/wp\/v2\/pages\/94?print=print\" class=\"pdfprnt-button pdfprnt-button-print\" target=\"_blank\"><img decoding=\"async\" src=\"https:\/\/www.oato.inaf.it\/blazars\/webt\/wp-content\/plugins\/pdf-print\/images\/print.png\" alt=\"image_print\" title=\"Print Content\" \/><\/a><\/div>\n<p style=\"font-size:17px\">WEBT observations are made at the&nbsp;<a href=\"http:\/\/astro.fisica.unipg.it\/\">Perugia Observatory<\/a>&nbsp;by Gino Tosti with the Automatic Imaging Telescope (AIT).<\/p>\n\n\n\n<p style=\"font-size:17px\"><strong>Telescope parameters:<\/strong> Long= +12.3916 deg, Lat= +43.1122 deg, Alt=451 m<\/p>\n\n\n\n<p style=\"font-size:17px\"><strong>Optical configuration:<\/strong> Newtonian, D= 0.4 m, f\/D= 5; Seeing_typical= 2&#8243;.5 &#8211; 3&#8243;, Skybrightness_typical= V=18.5 mag\/arcsec^2;<\/p>\n\n\n\n<p style=\"font-size:17px\"><strong>CCD camera:<\/strong> Spectrasource Ins. Ltd., Peltier cooled 50 deg C wrt ambient, CCD chip: TI TC211, 192&#215;165 pixels, 13.5&#215;16.5 um pixel width;<\/p>\n\n\n\n<p style=\"font-size:17px\"><strong>Filters:<\/strong> diameter = 1in, Johnson B (BG12 (2mm) + GG385 (1mm) + BG39 (1mm)), Johnson V (GG495 (2mm) + BG39 (2mm)); Cousins R_c (OG570 (2mm) + KG3 (2mm)); Cousins I_c (RG9 (3mm)); absolute photometry to 0.06 magnitudes accuracy, differential photometry to 0.02 magnitudes.\u00a0<\/p>\n","protected":false},"excerpt":{"rendered":"<p>WEBT observations are made at the&nbsp;Perugia Observatory&nbsp;by Gino Tosti with the Automatic Imaging Telescope (AIT). Telescope parameters: Long= +12.3916 deg,&hellip;<\/p>\n","protected":false},"author":4,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-94","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.oato.inaf.it\/blazars\/webt\/wp-json\/wp\/v2\/pages\/94","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.oato.inaf.it\/blazars\/webt\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.oato.inaf.it\/blazars\/webt\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.oato.inaf.it\/blazars\/webt\/wp-json\/wp\/v2\/users\/4"}],"replies":[{"embeddable":true,"href":"https:\/\/www.oato.inaf.it\/blazars\/webt\/wp-json\/wp\/v2\/comments?post=94"}],"version-history":[{"count":1,"href":"https:\/\/www.oato.inaf.it\/blazars\/webt\/wp-json\/wp\/v2\/pages\/94\/revisions"}],"predecessor-version":[{"id":95,"href":"https:\/\/www.oato.inaf.it\/blazars\/webt\/wp-json\/wp\/v2\/pages\/94\/revisions\/95"}],"wp:attachment":[{"href":"https:\/\/www.oato.inaf.it\/blazars\/webt\/wp-json\/wp\/v2\/media?parent=94"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}