{"id":6159,"date":"2021-05-27T11:19:04","date_gmt":"2021-05-27T09:19:04","guid":{"rendered":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/20170807_104835.jpg"},"modified":"2021-10-28T19:42:16","modified_gmt":"2021-10-28T17:42:16","slug":"20170807_104835","status":"inherit","type":"attachment","link":"https:\/\/www.oa-roma.inaf.it\/heag\/20170807_104835\/","title":{"rendered":"Gianluca (Giallo)"},"author":67,"featured_media":0,"comment_status":"open","ping_status":"closed","template":"","meta":{"_acf_changed":false},"class_list":["post-6159","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\/20170807_104835-rotated.jpg'><img loading=\"lazy\" decoding=\"async\" width=\"225\" height=\"300\" src=\"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/20170807_104835-225x300.jpg\" class=\"attachment-medium size-medium\" alt=\"GianLuca (Giallo) Israel\" srcset=\"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/20170807_104835-225x300.jpg 225w, https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/20170807_104835-768x1024.jpg 768w, https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/20170807_104835-1152x1536.jpg 1152w, https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/20170807_104835-rotated.jpg 1200w\" sizes=\"auto, 100vw\" \/><\/a><\/p>\n<p>I am currently Research Director and I am working at the HEAG in Rome since 1997.<br \/>\nI had several (scientific) travel mates during all these years. I have started (and still working on) with the development of timing techniques to search for coherent signals in X-ray sources and their application to the astronomical archives of X-ray missions (CATS@BAT and EXTraS recent projects). I am involved in Magnetar (the strongest magnets in the Universe) studies since 1993 when I first discovered pulsations in one of the source prototype 4U0142+614. I have been involved since 1999 in the study of an extreme X-ray binary hosting two white dwarfs  when I discovered the shortest orbital period currently known (HM Cnc; Porb=5.4minutes). More recently, I am focusing onto Ultraluminous X-ray Sources hosting neutron stars accreting at super-Eddington rates (with the discovery of the most distant and luminous X-ray pulsars in NGC5907). Other topics of interest are GWs, GRBs, FRBs, search of the optical counterpart of new X-ray pulsators, time domain astronomy. I am teaching at &#8220;Tor Vergata&#8221; University since many years (&#8220;High Energy Astrophysics&#8221; course).<\/p>\n<p><a href=\"https:\/\/ui.adsabs.harvard.edu\/search\/q=orcid%3A%200000-0001-5480-6438&amp;sort=date%20desc%2C%20bibcode%20desc&amp;p_=0\">List of publications<\/a><\/p>\n"},"caption":{"rendered":"<p style=\"font-size:0.8vw\"> Gianluca (aka Giallo): I am currently Research Director and I am working at the HEAG in Rome since 1997.<br \/>\nI had several (scientific) travel mates during all these years. I  have started (and still working on) with the development of timing techniques to search for coherent signals in X-ray sources and their application to the astronomical archives of X-ray missions. I am involved in Magnetar studies since 1993 when I discovered pulsations in 4U0142+614. More recently, I moved to Ultraluminous X-ray Sources hosting neutron stars (with the discovery of the most distant and luminous X-ray pulsars in NGC5907). Other topics of interest are GWs, GRBs, FRBs, search of the optical counterpart of new X-ray pulsators, time domain astronomy. I am teaching at &#8220;Tor Vergata&#8221; University since many years. <\/p>\n"},"alt_text":"GianLuca (Giallo) Israel","media_type":"image","mime_type":"image\/jpeg","media_details":{"width":1200,"height":1600,"file":"2021\/05\/20170807_104835-rotated.jpg","sizes":{"medium":{"file":"20170807_104835-225x300.jpg","width":225,"height":300,"mime_type":"image\/jpeg","source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/20170807_104835-225x300.jpg"},"large":{"file":"20170807_104835-768x1024.jpg","width":768,"height":1024,"mime_type":"image\/jpeg","source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/20170807_104835-768x1024.jpg"},"thumbnail":{"file":"20170807_104835-150x150.jpg","width":150,"height":150,"mime_type":"image\/jpeg","source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/20170807_104835-150x150.jpg"},"medium_large":{"file":"20170807_104835-768x1024.jpg","width":768,"height":1024,"mime_type":"image\/jpeg","source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/20170807_104835-768x1024.jpg"},"1536x1536":{"file":"20170807_104835-1152x1536.jpg","width":1152,"height":1536,"mime_type":"image\/jpeg","source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/20170807_104835-1152x1536.jpg"},"inspiro-recent-thumbnail":{"file":"20170807_104835-345x192.jpg","width":345,"height":192,"mime_type":"image\/jpeg","source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/20170807_104835-345x192.jpg"},"inspiro-recent-thumbnail-retina":{"file":"20170807_104835-690x384.jpg","width":690,"height":384,"mime_type":"image\/jpeg","source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/20170807_104835-690x384.jpg"},"inspiro-loop":{"file":"20170807_104835-950x320.jpg","width":950,"height":320,"mime_type":"image\/jpeg","source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/20170807_104835-950x320.jpg"},"inspiro-loop@2x":{"file":"20170807_104835-rotated-1200x640.jpg","width":1200,"height":640,"filesize":137940,"mime_type":"image\/jpeg","source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/20170807_104835-rotated-1200x640.jpg"},"full":{"file":"20170807_104835-rotated.jpg","width":1200,"height":1600,"mime_type":"image\/jpeg","source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/20170807_104835-rotated.jpg"}},"image_meta":{"aperture":"2.4","credit":"","camera":"SM-G361F","caption":"","created_timestamp":"1502102915","copyright":"","focal_length":"2.3500061035156","iso":"100","shutter_speed":"0.02","title":"","orientation":1,"keywords":[]},"original_image":"20170807_104835.jpg"},"post":null,"source_url":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-content\/uploads\/sites\/18\/2021\/05\/20170807_104835-rotated.jpg","_links":{"self":[{"href":"https:\/\/www.oa-roma.inaf.it\/heag\/wp-json\/wp\/v2\/media\/6159","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=6159"}]}}