{"id":40,"date":"2021-05-04T22:26:20","date_gmt":"2021-05-04T20:26:20","guid":{"rendered":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/arianna.jpeg"},"modified":"2021-10-28T19:42:38","modified_gmt":"2021-10-28T17:42:38","slug":"arianna","status":"inherit","type":"attachment","link":"https:\/\/www.oa-roma.inaf.it\/heag\/arianna\/","title":{"rendered":"Arianna Miraval Zanon"},"author":67,"featured_media":0,"comment_status":"open","ping_status":"closed","template":"","meta":{"_acf_changed":false},"class_list":["post-40","attachment","type-attachment","status-inherit","hentry"],"acf":[],"jetpack_sharing_enabled":true,"description":{"rendered":"<p class=\"attachment\"><a href='https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/arianna.jpeg'><img loading=\"lazy\" decoding=\"async\" width=\"270\" height=\"300\" src=\"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/arianna-270x300.jpeg\" class=\"attachment-medium size-medium\" alt=\"\" srcset=\"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/arianna-270x300.jpeg 270w, https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/arianna-921x1024.jpeg 921w, https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/arianna-768x854.jpeg 768w, https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/arianna.jpeg 1047w\" sizes=\"auto, 100vw\" \/><\/a><\/p>\n<p>I am a postdoctoral researcher at the Observatory of Rome and I am working to develop new timing algorithms within Stingray. I obtained my MSc in Astronomy at the University of Padua in September 2017, doing my thesis at the Observatory of Cagliari. I obtained my PhD in Physics and Astrophysics in 2021 at the University of Insubria working in collaboration with the Observatory of Brera. My research activity is focused on the study of the X-ray, UV, optical and radio properties of Neutron Star Low Mass X-ray binaries, from the accretion phase to the radio pulsar state. <\/p>\n<p><a href=\"https:\/\/ui.adsabs.harvard.edu\/search\/q=orcid%3A%200000-0002-0943-4484&amp;sort=date%20desc%2C%20bibcode%20desc&amp;p_=0\">List of publications<\/a><\/p>\n"},"caption":{"rendered":"<p style=\"font-size:0.8vw\"> Arianna: I am a postdoctoral researcher at the Observatory of Rome. I obtained my MSc in Astronomy at the University of Padua in September 2017, doing my thesis at the Observatory of Cagliari. I obtained my PhD in Physics and Astrophysics in 2021 at the University of Insubria working in collaboration with the Observatory of Brera. My research activity is focused on the study of the X-ray, UV, optical and radio properties of Neutron Star Low Mass X-ray binaries, from the accretion phase to the radio pulsar state. <\/p>\n"},"alt_text":"","media_type":"image","mime_type":"image\/jpeg","media_details":{"width":1047,"height":1164,"file":"2021\/05\/arianna.jpeg","sizes":{"medium":{"file":"arianna-270x300.jpeg","width":270,"height":300,"mime_type":"image\/jpeg","source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/arianna-270x300.jpeg"},"large":{"file":"arianna-921x1024.jpeg","width":921,"height":1024,"mime_type":"image\/jpeg","source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/arianna-921x1024.jpeg"},"thumbnail":{"file":"arianna-150x150.jpeg","width":150,"height":150,"mime_type":"image\/jpeg","source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/arianna-150x150.jpeg"},"medium_large":{"file":"arianna-768x854.jpeg","width":768,"height":854,"mime_type":"image\/jpeg","source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/arianna-768x854.jpeg"},"post-thumbnail":{"file":"arianna-1000x288.jpeg","width":1000,"height":288,"mime_type":"image\/jpeg","source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/arianna-1000x288.jpeg"},"large-feature":{"file":"arianna-1000x288.jpeg","width":1000,"height":288,"mime_type":"image\/jpeg","source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/arianna-1000x288.jpeg"},"small-feature":{"file":"arianna-270x300.jpeg","width":270,"height":300,"mime_type":"image\/jpeg","source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/arianna-270x300.jpeg"},"inspiro-loop":{"file":"arianna-950x320.jpeg","width":950,"height":320,"filesize":53124,"mime_type":"image\/jpeg","source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/arianna-950x320.jpeg"},"inspiro-loop@2x":{"file":"arianna-1047x640.jpeg","width":1047,"height":640,"filesize":131805,"mime_type":"image\/jpeg","source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/arianna-1047x640.jpeg"},"full":{"file":"arianna.jpeg","width":1047,"height":1164,"mime_type":"image\/jpeg","source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/arianna.jpeg"}},"image_meta":{"aperture":"0","credit":"","camera":"","caption":"","created_timestamp":"0","copyright":"","focal_length":"0","iso":"0","shutter_speed":"0","title":"","orientation":"0","keywords":[]}},"post":null,"source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/arianna.jpeg","_links":{"self":[{"href":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-json\/wp\/v2\/media\/40","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-json\/wp\/v2\/media"}],"about":[{"href":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-json\/wp\/v2\/types\/attachment"}],"author":[{"embeddable":true,"href":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-json\/wp\/v2\/users\/67"}],"replies":[{"embeddable":true,"href":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-json\/wp\/v2\/comments?post=40"}]}}