{"id":6544,"date":"2021-10-28T19:30:59","date_gmt":"2021-10-28T17:30:59","guid":{"rendered":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/10\/arianna_photo.jpeg"},"modified":"2026-02-19T08:55:22","modified_gmt":"2026-02-19T07:55:22","slug":"arianna_photo","status":"inherit","type":"attachment","link":"https:\/\/www.oa-roma.inaf.it\/heag\/arianna_photo\/","title":{"rendered":"Arianna Miraval Zanon"},"author":276,"featured_media":0,"comment_status":"open","ping_status":"closed","template":"","meta":{"_acf_changed":false},"class_list":["post-6544","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\/10\/arianna_photo.jpeg'><img loading=\"lazy\" decoding=\"async\" width=\"270\" height=\"300\" src=\"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/10\/arianna_photo-270x300.jpeg\" class=\"attachment-medium size-medium\" alt=\"\" srcset=\"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/10\/arianna_photo-270x300.jpeg 270w, https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/10\/arianna_photo-921x1024.jpeg 921w, https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/10\/arianna_photo-768x854.jpeg 768w, https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/10\/arianna_photo.jpeg 1047w\" sizes=\"auto, 100vw\" \/><\/a><\/p>\n<p>I have been working as a Technologist at the Italian Space Agency since February 2023. Prior to this position, I spent two years working as a Post-Doc in the High Energy Astrophysics Group at the INAF-Observatory of Rome, and I continue to collaborate with them. My primary focus has been the study of magnetized neutron stars with rotation periods of a few milliseconds, commonly known as millisecond pulsars. My interest in pulsar research began during my time as an Astronomy student at the University of Padova, where I conducted optical timing analyses of an isolated pulsar for my Bachelor\u2019s thesis. For my Master\u2019s thesis, I engaged in research at the INAF-Observatory of Cagliari, focusing on binary millisecond pulsars in the radio band. In April 2021, I completed my PhD at Insubria University. The title of my thesis was &#8216;Multi-wavelength Study of Binary Millisecond Pulsars,&#8217; supervised by Dr. Campana and Dr. D\u2019Avanzo.<\/p>\n<p>Throughout my career, I have cultivated expertise in time-domain astronomy and have developed codes for timing analysis across various wavelength bands, including X-ray, UV, optical, and radio. Additionally, I have acquired proficiency in spectroscopic observational techniques in both the X-ray and optical bands, applying them to transient systems. Utilizing multi-wavelength observations, my goal has been to identify and interpret the mechanisms responsible for pulsed emission in different evolutionary states of binary pulsars across the entire electromagnetic spectrum.<\/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>Arianna Miraval Zanon &#8211; ASI Staff<\/p>\n"},"alt_text":"","media_type":"image","mime_type":"image\/jpeg","media_details":{"width":1047,"height":1164,"file":"2021\/10\/arianna_photo.jpeg","sizes":{"medium":{"file":"arianna_photo-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\/10\/arianna_photo-270x300.jpeg"},"large":{"file":"arianna_photo-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\/10\/arianna_photo-921x1024.jpeg"},"thumbnail":{"file":"arianna_photo-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\/10\/arianna_photo-150x150.jpeg"},"medium_large":{"file":"arianna_photo-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\/10\/arianna_photo-768x854.jpeg"},"inspiro-loop":{"file":"arianna_photo-950x320.jpeg","width":950,"height":320,"mime_type":"image\/jpeg","source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/10\/arianna_photo-950x320.jpeg"},"inspiro-loop@2x":{"file":"arianna_photo-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\/10\/arianna_photo-1047x640.jpeg"},"full":{"file":"arianna_photo.jpeg","width":1047,"height":1164,"mime_type":"image\/jpeg","source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/10\/arianna_photo.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\/10\/arianna_photo.jpeg","_links":{"self":[{"href":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-json\/wp\/v2\/media\/6544","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\/276"}],"replies":[{"embeddable":true,"href":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-json\/wp\/v2\/comments?post=6544"}]}}