{"id":3561,"date":"2024-05-24T09:53:12","date_gmt":"2024-05-24T07:53:12","guid":{"rendered":"http:\/\/brera.inaf.it\/progetti_ricerca\/cora\/"},"modified":"2024-10-16T16:29:03","modified_gmt":"2024-10-16T14:29:03","slug":"cora","status":"publish","type":"progetti_ricerca","link":"https:\/\/brera.inaf.it\/en\/progetti_ricerca\/cora\/","title":{"rendered":"CORA"},"content":{"rendered":"\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-995f960e wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\" style=\"flex-basis:33.33%\">\n<figure class=\"wp-block-image size-full\"><img loading=\"lazy\" decoding=\"async\" width=\"800\" height=\"800\" src=\"http:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/06\/Progetti-OAB-800x800-cora.png\" alt=\"\" class=\"wp-image-980\"\/><\/figure>\n<\/div>\n\n\n\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\" style=\"flex-basis:66.66%\">\n<h5 class=\"wp-block-heading\">CORA<\/h5>\n\n\n\n<p class=\"wp-block-paragraph\"><strong>C<\/strong>ompact <strong>O<\/strong>bjects &amp; <strong>R<\/strong>elativistic <strong>A<\/strong>strophysics<\/p>\n\n\n\n<h6 class=\"wp-block-heading\">SHORT DESCRIPTION<\/h6>\n\n\n\n<p class=\"wp-block-paragraph\"><em>CORA<\/em>&nbsp;(Compact Objects &amp; Relativistic Astrophysics) is a research group at INAF OAB mainly aimed at studying&nbsp;compact objects&nbsp;(black holes, neutron stars), their relativistic jets, their close environment, and their cosmological evolution and distribution on large scale in the Universe.<br>Currently we are continuing the study of a specific class of&nbsp;jetted active galactic nuclei&nbsp;(AGN), named&nbsp;Narrow-Line Seyfert 1 Galaxies with gamma ray emission.<br>The latest efforts were dedicated to find&nbsp;new objects&nbsp;of this class and to understand the discovery space that will be available with the beginning of the operations of the Cherenkov Telescope Array (CTAO).<\/p>\n\n\n\n<h6 class=\"wp-block-heading\">OBSERVATORY STAFF INVOLVED<\/h6>\n\n\n\n<ul class=\"wp-block-list\">\n<li>Patrizia Romano: researcher<\/li>\n\n\n\n<li>Stefano Vercellone: researcher<\/li>\n<\/ul>\n\n\n\n<p class=\"wp-block-paragraph\"><strong>Other fields of research<\/strong>: X-ray binaries named Supergiant Fast X-ray Transients, a peculiar class of Galactic binaries (an accreting neutron star coupled with a supergiant young star) characterised by strong and fast outburst (Patrizia Romano).<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">Multi-wavelength studies of gamma-ray loud blazars with AGILE\/GRID and Fermi\/LAT (Stefano Vercellone)<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">Service activities within large collaborations (Patrizia Romano, Stefano Vercellone):&nbsp;<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">Patrizia Romano, former coordinator of the CTA extragalactic working group; ALTO\/COMET Multi-wavelength Coordinator. Swift\/XRT Team Member.<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">Stefano Vercellone, former CTA Science Coordinator; INAF coordinator Science work package for CTA; ASTRI Mini-Array science coordinator; ALTO\/COMET Science Coordinator.<\/p>\n\n\n\n<div class=\"wp-block-group is-layout-constrained wp-block-group-is-layout-constrained\">\n<h6 class=\"wp-block-heading\"><strong>CONTACTS<\/strong><\/h6>\n<\/div>\n\n\n\n<p class=\"wp-block-paragraph\">patrizia.romano AT inaf.it <\/p>\n\n\n\n<p class=\"wp-block-paragraph\">stefano.vercellone AT inaf.it<\/p>\n\n\n\n<h6 class=\"wp-block-heading\"><strong>CREDITS<\/strong><\/h6>\n\n\n\n<p class=\"wp-block-paragraph\">Web page content: P. Romano e S. Vercellone per CORA Team.<\/p>\n<\/div>\n<\/div>\n\n\n\n<p class=\"wp-block-paragraph\"><\/p>\n","protected":false},"excerpt":{"rendered":"<p>CORA Compact Objects &amp; Relativistic Astrophysics SHORT DESCRIPTION CORA&nbsp;(Compact Objects &amp; Relativistic Astrophysics) is a research group at INAF OAB mainly aimed at studying&nbsp;compact objects&nbsp;(black holes, neutron stars), their relativistic jets, their close environment, and their cosmological evolution and distribution on large scale in the Universe.Currently we are continuing the study of a specific class [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":1194,"parent":0,"menu_order":0,"comment_status":"open","ping_status":"closed","template":"","format":"standard","meta":{"footnotes":""},"categories":[25],"tags":[],"class_list":["post-3561","progetti_ricerca","type-progetti_ricerca","status-publish","format-standard","has-post-thumbnail","hentry","category-research-project"],"blocksy_meta":[],"featured_image_urls":{"full":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/06\/Progetti-OAB-800x800-cora.png",800,800,false],"thumbnail":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/06\/Progetti-OAB-800x800-cora.png",150,150,false],"medium":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/06\/Progetti-OAB-800x800-cora.png",300,300,false],"medium_large":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/06\/Progetti-OAB-800x800-cora.png",768,768,false],"large":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/06\/Progetti-OAB-800x800-cora.png",800,800,false],"1536x1536":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/06\/Progetti-OAB-800x800-cora.png",800,800,false],"2048x2048":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/06\/Progetti-OAB-800x800-cora.png",800,800,false]},"post_excerpt_stackable":"<p>CORA Compact Objects &amp; Relativistic Astrophysics SHORT DESCRIPTION CORA&nbsp;(Compact Objects &amp; Relativistic Astrophysics) is a research group at INAF OAB mainly aimed at studying&nbsp;compact objects&nbsp;(black holes, neutron stars), their relativistic jets, their close environment, and their cosmological evolution and distribution on large scale in the Universe.Currently we are continuing the study of a specific class of&nbsp;jetted active galactic nuclei&nbsp;(AGN), named&nbsp;Narrow-Line Seyfert 1 Galaxies with gamma ray emission.The latest efforts were dedicated to find&nbsp;new objects&nbsp;of this class and to understand the discovery space that will be available with the beginning of the operations of the Cherenkov Telescope Array (CTAO). OBSERVATORY STAFF&hellip;<\/p>\n","category_list":"<a href=\"https:\/\/brera.inaf.it\/en\/category\/research-project\/\" rel=\"category tag\">Research project<\/a>","author_info":{"name":"Maria Rosa Panzera","url":"https:\/\/brera.inaf.it\/en\/author\/maria-rosa-panzera\/"},"comments_num":"0 comments","_links":{"self":[{"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/progetti_ricerca\/3561","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/progetti_ricerca"}],"about":[{"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/types\/progetti_ricerca"}],"author":[{"embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/comments?post=3561"}],"version-history":[{"count":2,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/progetti_ricerca\/3561\/revisions"}],"predecessor-version":[{"id":3588,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/progetti_ricerca\/3561\/revisions\/3588"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/media\/1194"}],"wp:attachment":[{"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/media?parent=3561"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/categories?post=3561"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/tags?post=3561"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}