{"id":22,"date":"2021-01-28T12:26:20","date_gmt":"2021-01-28T11:26:20","guid":{"rendered":"https:\/\/www.oa-roma.inaf.it\/caesar\/?page_id=22"},"modified":"2024-11-25T18:01:50","modified_gmt":"2024-11-25T17:01:50","slug":"who-we-are","status":"publish","type":"page","link":"https:\/\/www.oa-roma.inaf.it\/caesar\/who-we-are\/","title":{"rendered":"People"},"content":{"rendered":"\n<p>The group currently (February 2024) consists of xx members among staff, TD researchers, Post-Doc, PhD students, fellows and (Astro)Physics students, and xx group affiliates.&nbsp;<\/p>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:31% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"682\" height=\"1024\" src=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/03\/DNT_1253-682x1024.jpg\" alt=\"\" class=\"wp-image-448 size-full\" srcset=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/03\/DNT_1253-682x1024.jpg 682w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/03\/DNT_1253-200x300.jpg 200w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/03\/DNT_1253-768x1153.jpg 768w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/03\/DNT_1253-1023x1536.jpg 1023w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/03\/DNT_1253-1364x2048.jpg 1364w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/03\/DNT_1253-scaled.jpg 1705w\" sizes=\"auto, (max-width: 682px) 100vw, 682px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-large-font-size\">Federico Angeloni<\/p>\n\n\n\n<p><em><em>Univ. Sapienza &#8211; PhD Student<\/em><\/em><\/p>\n\n\n\n<p>BH\/NS merger population modelling, Galaxy Formation and Evolution&nbsp;Models,&nbsp; High Performance Computing, Waveform Modelling from Compact and Exotic Compact Objects<\/p>\n\n\n\n<p><a  href=\"javascript:smae_decode('ZmVkZXJpY28uYW5nZWxvbmlAcm9tYTEuaW5mbi5pdA==');\" target=\"_blank\"  rel=\"noreferrer noopener\">&#102;&#101;&#100;&#101;&#114;&#105;&#099;&#111;&#046;&#097;&#110;&#103;&#101;&#108;&#111;&#110;&#105;&#064;&#114;&#111;&#109;&#097;&#049;&#046;&#105;&#110;&#102;&#110;&#046;&#105;&#116;<\/a><\/p>\n\n\n\n<p><\/p>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:31% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"758\" height=\"932\" src=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/03\/foto_me.png\" alt=\"\" class=\"wp-image-446 size-full\" srcset=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/03\/foto_me.png 758w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/03\/foto_me-244x300.png 244w\" sizes=\"auto, (max-width: 706px) 89vw, (max-width: 767px) 82vw, 740px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-large-font-size\">Antonello Calabr\u00f2<\/p>\n\n\n\n<p><em>INAF-OAR &#8211; Post-Doctoral Research Assistant<\/em><\/p>\n\n\n\n<p>Galaxy evolution,&nbsp;morphology,&nbsp;optical\/NIR spectroscopy,&nbsp;emission line modelling of star-forming galaxies and AGNs,&nbsp;data analysis and machine learning<\/p>\n\n\n\n<p><span class=\"has-inline-color has-vivid-red-color\"><a  href=\"javascript:smae_decode('YW50b25lbGxvLmNhbGFicm9AaW5hZi5pdA==');\" target=\"_blank\"  rel=\"noreferrer noopener\">&#097;&#110;&#116;&#111;&#110;&#101;&#108;&#108;&#111;&#046;&#099;&#097;&#108;&#097;&#098;&#114;&#111;&#064;&#105;&#110;&#097;&#102;&#046;&#105;&#116;<\/a><\/span> | <a href=\"https:\/\/ui.adsabs.harvard.edu\/public-libraries\/9nhfuLHjSvSI-atPIRd9qA\" data-type=\"link\" data-id=\"https:\/\/ui.adsabs.harvard.edu\/public-libraries\/9nhfuLHjSvSI-atPIRd9qA\" target=\"_blank\" rel=\"noreferrer noopener\">NASA\/ADS<\/a><\/p>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:31% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"140\" height=\"140\" src=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/Screenshot-2020-01-09-at-15.01.43.png\" alt=\"\" class=\"wp-image-188 size-full\" srcset=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/Screenshot-2020-01-09-at-15.01.43.png 140w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/Screenshot-2020-01-09-at-15.01.43-100x100.png 100w\" sizes=\"auto, (max-width: 140px) 100vw, 140px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p><\/p>\n\n\n\n<p class=\"has-large-font-size\">Marco Castellano<\/p>\n\n\n\n<p><em>INAF-OAR &#8211; Ricercatore<\/em><\/p>\n\n\n\n<p>High-redshift galaxy evolution, reionization, extragalactic surveys, image and data analysis   <\/p>\n\n\n\n<p><span class=\"has-inline-color has-vivid-red-color\"><a  href=\"javascript:smae_decode('bWFyY28uY2FzdGVsbGFub0BpbmFmLml0');\" target=\"_blank\"  rel=\"noreferrer noopener\">&#109;&#097;&#114;&#099;&#111;&#046;&#099;&#097;&#115;&#116;&#101;&#108;&#108;&#097;&#110;&#111;&#064;&#105;&#110;&#097;&#102;&#046;&#105;&#116;<\/a><\/span><\/p>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:31% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"791\" height=\"1024\" src=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/Claudia-791x1024.jpg\" alt=\"\" class=\"wp-image-193 size-full\" srcset=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/Claudia-791x1024.jpg 791w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/Claudia-232x300.jpg 232w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/Claudia-768x994.jpg 768w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/Claudia-1187x1536.jpg 1187w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/Claudia.jpg 1582w\" sizes=\"auto, (max-width: 767px) 89vw, (max-width: 1000px) 54vw, (max-width: 1071px) 543px, 580px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p><\/p>\n\n\n\n<p class=\"has-large-font-size\">Claudia Di Cesare<\/p>\n\n\n\n<p>ISTA &#8211; <em><em><em>Post-Doctoral Research Assistant<\/em><\/em><\/em><\/p>\n\n\n\n<p>Galaxy evolution at high redshift (z=6-4)<\/p>\n\n\n\n<p><span class=\"has-inline-color has-vivid-red-color\"><a  href=\"javascript:smae_decode('Y2xhdWRpYS5kaWNlc2FyZUByb21hMS5pbmZuLml0');\" target=\"_blank\"  rel=\"noreferrer noopener\">&#099;&#108;&#097;&#117;&#100;&#105;&#097;&#046;&#100;&#105;&#099;&#101;&#115;&#097;&#114;&#101;&#064;&#114;&#111;&#109;&#097;&#049;&#046;&#105;&#110;&#102;&#110;&#046;&#105;&#116;<\/a><\/span><\/p>\n\n\n\n<p><\/p>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:31% auto\"><figure class=\"wp-block-media-text__media\"><a href=\"https:\/\/www.oa-roma.inaf.it\/fontana\" target=\"_blank\" rel=\"noopener\"><img loading=\"lazy\" decoding=\"async\" width=\"200\" height=\"248\" src=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/01\/PG2_0943zoom-e1611833460405.jpeg\" alt=\"\" class=\"wp-image-26 size-full\" \/><\/a><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-large-font-size\"><a href=\"https:\/\/www.oa-roma.inaf.it\/fontana\" target=\"_blank\" rel=\"noreferrer noopener\">Adriano Fontana<\/a><\/p>\n\n\n\n<p><em>INAF-OAR &#8211; Dirigente di Ricerca<\/em><\/p>\n\n\n\n<p>Evolution of high redshift galaxies, SED fitting <\/p>\n\n\n\n<p><span class=\"has-inline-color has-vivid-red-color\"><a  href=\"javascript:smae_decode('YWRyaWFuby5mb250YW5hQGluYWYuaXQ=');\" target=\"_blank\"  rel=\"noreferrer noopener\">&#097;&#100;&#114;&#105;&#097;&#110;&#111;&#046;&#102;&#111;&#110;&#116;&#097;&#110;&#097;&#064;&#105;&#110;&#097;&#102;&#046;&#105;&#116;<\/a><\/span><\/p>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:38% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"449\" height=\"450\" src=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/FFph-1.jpg\" alt=\"\" class=\"wp-image-183 size-full\" srcset=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/FFph-1.jpg 449w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/FFph-1-300x300.jpg 300w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/FFph-1-150x150.jpg 150w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/FFph-1-100x100.jpg 100w\" sizes=\"auto, (max-width: 449px) 100vw, 449px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p><\/p>\n\n\n\n<p class=\"has-large-font-size\">Flaminia Fortuni<\/p>\n\n\n\n<p><em>INAF-OAR &#8211; <em>Post-Doctoral Research Assistant<\/em><\/em><\/p>\n\n\n\n<p>Forward modeling of cosmological simulations<\/p>\n\n\n\n<p><span class=\"has-inline-color has-vivid-red-color\"><a  href=\"javascript:smae_decode('ZmxhbWluaWEuZm9ydHVuaUBpbmFmLml0');\" target=\"_blank\"  rel=\"noreferrer noopener\">&#102;&#108;&#097;&#109;&#105;&#110;&#105;&#097;&#046;&#102;&#111;&#114;&#116;&#117;&#110;&#105;&#064;&#105;&#110;&#097;&#102;&#046;&#105;&#116;<\/a><\/span><\/p>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:31% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"812\" height=\"872\" src=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/03\/lucagraziani-1.png\" alt=\"\" class=\"wp-image-228 size-full\" srcset=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/03\/lucagraziani-1.png 812w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/03\/lucagraziani-1-279x300.png 279w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/03\/lucagraziani-1-768x825.png 768w\" sizes=\"auto, (max-width: 767px) 89vw, (max-width: 1000px) 54vw, (max-width: 1071px) 543px, 580px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p><\/p>\n\n\n\n<p class=\"has-large-font-size\">Luca Graziani<\/p>\n\n\n\n<p><em>Univ. Sapienza &#8211; Ricercatore<\/em><\/p>\n\n\n\n<p>Formation and evolution of the first galaxies, metal and dust enrichment, early black holes and cosmic reionization<\/p>\n\n\n\n<p><span class=\"has-inline-color has-vivid-red-color\"><a  href=\"javascript:smae_decode('bHVjYS5ncmF6aWFuaUB1bmlyb21hMS5pdA==');\" target=\"_blank\"  rel=\"noreferrer noopener\">&#108;&#117;&#099;&#097;&#046;&#103;&#114;&#097;&#122;&#105;&#097;&#110;&#105;&#064;&#117;&#110;&#105;&#114;&#111;&#109;&#097;&#049;&#046;&#105;&#116;<\/a><\/span><\/p>\n\n\n\n<p><\/p>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:31% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"1024\" height=\"636\" src=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/01\/Abell370_HST_FF_v3-1024x636.png\" alt=\"\" class=\"wp-image-11 size-full\" srcset=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/01\/Abell370_HST_FF_v3-1024x636.png 1024w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/01\/Abell370_HST_FF_v3-300x186.png 300w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/01\/Abell370_HST_FF_v3-768x477.png 768w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/01\/Abell370_HST_FF_v3-1536x954.png 1536w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/01\/Abell370_HST_FF_v3.png 1786w\" sizes=\"auto, (max-width: 767px) 89vw, (max-width: 1000px) 54vw, (max-width: 1071px) 543px, 580px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-large-font-size\">Mario Francisco Llerena Ona<\/p>\n\n\n\n<p><em><em><em>INAF-OAR &#8211; Post-Doctoral Research Assistant<\/em><\/em><\/em><\/p>\n\n\n\n<p>&#8230;<\/p>\n\n\n\n<p><a  href=\"javascript:smae_decode('bWFyaW8ubGxlcmVuYW9uYUBpbmFmLml0');\" target=\"_blank\"  rel=\"noreferrer noopener\">&#109;&#097;&#114;&#105;&#111;&#046;&#108;&#108;&#101;&#114;&#101;&#110;&#097;&#111;&#110;&#097;&#064;&#105;&#110;&#097;&#102;&#046;&#105;&#116;<\/a><\/p>\n\n\n\n<p><\/p>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:31% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"1024\" height=\"1024\" src=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/02\/IMG_5119-1024x1024.jpeg\" alt=\"\" class=\"wp-image-391 size-full\" srcset=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/02\/IMG_5119-1024x1024.jpeg 1024w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/02\/IMG_5119-300x300.jpeg 300w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/02\/IMG_5119-150x150.jpeg 150w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/02\/IMG_5119-768x768.jpeg 768w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/02\/IMG_5119-1536x1536.jpeg 1536w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/02\/IMG_5119-2048x2048.jpeg 2048w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/02\/IMG_5119-100x100.jpeg 100w\" sizes=\"auto, (max-width: 767px) 89vw, (max-width: 1000px) 54vw, (max-width: 1071px) 543px, 580px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-large-font-size\">Sara Mascia<\/p>\n\n\n\n<p><em><em>INAF OAR &#8211; PhD Student<\/em><\/em><\/p>\n\n\n\n<p>High-redshift galaxy evolution, reionization, optical\/NIR spectroscopy, data analysis <\/p>\n\n\n\n<p><a  href=\"javascript:smae_decode('c2FyYS5tYXNjaWFAaW5hZi5pdA==');\" target=\"_blank\"  rel=\"noreferrer noopener\">&#115;&#097;&#114;&#097;&#046;&#109;&#097;&#115;&#099;&#105;&#097;&#064;&#105;&#110;&#097;&#102;&#046;&#105;&#116;<\/a> | <a href=\"https:\/\/ui.adsabs.harvard.edu\/public-libraries\/AIIEnqyGS56eycCfy6G3SQ\" data-type=\"link\" data-id=\"https:\/\/ui.adsabs.harvard.edu\/public-libraries\/AIIEnqyGS56eycCfy6G3SQ\" target=\"_blank\" rel=\"noreferrer noopener\">NASA\/ADS<\/a><\/p>\n\n\n\n<p><\/p>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:30% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"947\" height=\"1024\" src=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/Screenshot-2021-02-08-at-17.00.07-947x1024.png\" alt=\"\" class=\"wp-image-154 size-full\" srcset=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/Screenshot-2021-02-08-at-17.00.07-947x1024.png 947w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/Screenshot-2021-02-08-at-17.00.07-278x300.png 278w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/Screenshot-2021-02-08-at-17.00.07-768x830.png 768w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/Screenshot-2021-02-08-at-17.00.07.png 1088w\" sizes=\"auto, (max-width: 767px) 89vw, (max-width: 1000px) 54vw, (max-width: 1071px) 543px, 580px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-large-font-size\"><a href=\"https:\/\/www.oa-roma.inaf.it\/merlin\/\" target=\"_blank\" rel=\"noreferrer noopener\">Emiliano Merlin<\/a><\/p>\n\n\n\n<p><em>INAF-OAR &#8211; Ricercatore<\/em><\/p>\n\n\n\n<p>Galaxy evolution, SED fitting, astronomical software development<\/p>\n\n\n\n<p><span class=\"has-inline-color has-vivid-red-color\"><a  href=\"javascript:smae_decode('ZW1pbGlhbm8ubWVybGluQGluYWYuaXQ=');\" target=\"_blank\"  rel=\"noreferrer noopener\">&#101;&#109;&#105;&#108;&#105;&#097;&#110;&#111;&#046;&#109;&#101;&#114;&#108;&#105;&#110;&#064;&#105;&#110;&#097;&#102;&#046;&#105;&#116;<\/a><\/span><\/p>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:33% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"856\" height=\"1024\" src=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/02\/WhatsApp-Image-2024-02-29-at-09.07.38-856x1024.jpeg\" alt=\"\" class=\"wp-image-424 size-full\" srcset=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/02\/WhatsApp-Image-2024-02-29-at-09.07.38-856x1024.jpeg 856w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/02\/WhatsApp-Image-2024-02-29-at-09.07.38-251x300.jpeg 251w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/02\/WhatsApp-Image-2024-02-29-at-09.07.38-768x918.jpeg 768w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/02\/WhatsApp-Image-2024-02-29-at-09.07.38-1285x1536.jpeg 1285w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/02\/WhatsApp-Image-2024-02-29-at-09.07.38.jpeg 1380w\" sizes=\"auto, (max-width: 767px) 89vw, (max-width: 1000px) 54vw, (max-width: 1071px) 543px, 580px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p><\/p>\n\n\n\n<p class=\"has-large-font-size\">Lorenzo Napolitano<\/p>\n\n\n\n<p><em>INAF OAR &#8211; PhD Student<\/em><\/p>\n\n\n\n<p>High-redshift galaxy evolution, reionization, optical\/NIR spectroscopy data analysis, JWST\/NIRSpec data reduction and machine learning applications in scientific cases<\/p>\n\n\n\n<p><span class=\"has-inline-color has-vivid-red-color\"><a  href=\"javascript:smae_decode('cm9zYS52YWxpYW50ZUBpbmFmLml0');\" target=\"_blank\"  rel=\"noreferrer noopener\">&#108;&#111;&#114;&#101;&#110;&#122;&#111;&#046;&#110;&#097;&#112;&#111;&#108;&#105;&#116;&#097;&#110;&#111;&#064;&#105;&#110;&#097;&#102;&#046;&#105;&#116;<\/a><\/span><\/p>\n\n\n\n<p><\/p>\n\n\n\n<p><\/p>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:31% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"512\" height=\"512\" src=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/faccetta.png\" alt=\"\" class=\"wp-image-111 size-full\" srcset=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/faccetta.png 512w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/faccetta-300x300.png 300w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/faccetta-150x150.png 150w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/faccetta-100x100.png 100w\" sizes=\"auto, (max-width: 512px) 100vw, 512px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-large-font-size\">Laura Pentericci<\/p>\n\n\n\n<p><em>INAF-OAR &#8211; Dirigente di Ricerca <\/em><\/p>\n\n\n\n<p>High redshift galaxies, Epoch of Reionization, Lyman alpha and Lyman Continuum emitters, spectroscopic surveys<\/p>\n\n\n\n<p><\/p>\n\n\n\n<p><span class=\"has-inline-color has-vivid-red-color\"><a  href=\"javascript:smae_decode('bGF1cmEucGVudGVyaWNjaUBpbmFmLml0');\" target=\"_blank\"  rel=\"noreferrer noopener\">&#108;&#097;&#117;&#114;&#097;&#046;&#112;&#101;&#110;&#116;&#101;&#114;&#105;&#099;&#099;&#105;&#064;&#105;&#110;&#097;&#102;&#046;&#105;&#116;<\/a><\/span><\/p>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:31% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"386\" height=\"388\" src=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/01\/Screenshot-2021-01-28-at-12.33.35-1.png\" alt=\"\" class=\"wp-image-38 size-full\" srcset=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/01\/Screenshot-2021-01-28-at-12.33.35-1.png 386w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/01\/Screenshot-2021-01-28-at-12.33.35-1-298x300.png 298w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/01\/Screenshot-2021-01-28-at-12.33.35-1-150x150.png 150w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/01\/Screenshot-2021-01-28-at-12.33.35-1-100x100.png 100w\" sizes=\"auto, (max-width: 386px) 100vw, 386px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-large-font-size\">Paola Santini<\/p>\n\n\n\n<p><em>INAF-OAR &#8211; Ricercatrice<\/em><\/p>\n\n\n\n<p>Galaxy evolution, SED fitting, far-IR ALMA <\/p>\n\n\n\n<p><span class=\"has-inline-color has-vivid-red-color\"><a  href=\"javascript:smae_decode('cGFvbGEuc2FudGluaUBpbmFmLml0');\" target=\"_blank\"  rel=\"noreferrer noopener\">&#112;&#097;&#111;&#108;&#097;&#046;&#115;&#097;&#110;&#116;&#105;&#110;&#105;&#064;&#105;&#110;&#097;&#102;&#046;&#105;&#116;<\/a><\/span> | <a href=\"https:\/\/ui.adsabs.harvard.edu\/user\/libraries\/qkWQYlLYQ2Cysh6SKOLSpw\" data-type=\"link\" data-id=\"https:\/\/ui.adsabs.harvard.edu\/user\/libraries\/qkWQYlLYQ2Cysh6SKOLSpw\" target=\"_blank\" rel=\"noreferrer noopener\">NASA\/ADS<\/a><\/p>\n\n\n\n<p><\/p>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:31% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"1024\" height=\"576\" src=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/03\/RS1-1024x576.jpg\" alt=\"\" class=\"wp-image-206 size-full\" srcset=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/03\/RS1-1024x576.jpg 1024w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/03\/RS1-300x169.jpg 300w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/03\/RS1-768x432.jpg 768w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/03\/RS1.jpg 1280w\" sizes=\"auto, (max-width: 767px) 89vw, (max-width: 1000px) 54vw, (max-width: 1071px) 543px, 580px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p><\/p>\n\n\n\n<p class=\"has-large-font-size\">Raffaella Schneider<\/p>\n\n\n\n<p><em>Univ Sapienza &#8211; Professoressa Ordinari<\/em>a<\/p>\n\n\n\n<p>First stars, first galaxies and first black holes. Early star formation and chemical evolution. Gravitational wave signatures of cosmic dawn<\/p>\n\n\n\n<p><span class=\"has-inline-color has-vivid-red-color\"><a  href=\"javascript:smae_decode('cmFmZmFlbGxhLnNjaG5laWRlckB1bmlyb21hMS5pdA==');\" target=\"_blank\"  rel=\"noreferrer noopener\">&#114;&#097;&#102;&#102;&#097;&#101;&#108;&#108;&#097;&#046;&#115;&#099;&#104;&#110;&#101;&#105;&#100;&#101;&#114;&#064;&#117;&#110;&#105;&#114;&#111;&#109;&#097;&#049;&#046;&#105;&#116;<\/a><\/span> | <a href=\"https:\/\/ui.adsabs.harvard.edu\/public-libraries\/NTjiSXpxRsWWjs_MbOz2Hg\" data-type=\"link\" data-id=\"https:\/\/ui.adsabs.harvard.edu\/public-libraries\/NTjiSXpxRsWWjs_MbOz2Hg\" target=\"_blank\" rel=\"noreferrer noopener\">NASA\/ADS<\/a><\/p>\n\n\n\n<p><\/p>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:31% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"512\" height=\"512\" src=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/faccetta.png\" alt=\"\" class=\"wp-image-111 size-full\" srcset=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/faccetta.png 512w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/faccetta-300x300.png 300w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/faccetta-150x150.png 150w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/faccetta-100x100.png 100w\" sizes=\"auto, (max-width: 512px) 100vw, 512px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-large-font-size\">Alessandro Trinca<\/p>\n\n\n\n<p><em><em>INAF-OAR &#8211; Post-Doctoral Research Assistant<\/em><\/em><\/p>\n\n\n\n<p>Una linea di spiegazione&#8230; <\/p>\n\n\n\n<p><a  href=\"javascript:smae_decode('YWxlc3NhbmRyby50cmluY2FAaW5hZi5pdA==');\" target=\"_blank\"  rel=\"noreferrer noopener\">&#097;&#108;&#101;&#115;&#115;&#097;&#110;&#100;&#114;&#111;&#046;&#116;&#114;&#105;&#110;&#099;&#097;&#064;&#105;&#110;&#097;&#102;&#046;&#105;&#116;<\/a><\/p>\n\n\n\n<p><\/p>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:33% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"372\" height=\"396\" src=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/fotoRosaValiante.jpg\" alt=\"\" class=\"wp-image-195 size-full\" srcset=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/fotoRosaValiante.jpg 372w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/02\/fotoRosaValiante-282x300.jpg 282w\" sizes=\"auto, (max-width: 372px) 100vw, 372px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p><\/p>\n\n\n\n<p class=\"has-large-font-size\">Rosa Valiante<\/p>\n\n\n\n<p><em>INAF OAR &#8211; Ricercatrice<\/em><\/p>\n\n\n\n<p>High-z SMBHs\/galaxies formation and evolution; Observable EM\/GW signatures of BH seeds<\/p>\n\n\n\n<p><span class=\"has-inline-color has-vivid-red-color\"><a  href=\"javascript:smae_decode('cm9zYS52YWxpYW50ZUBpbmFmLml0');\" target=\"_blank\"  rel=\"noreferrer noopener\">&#114;&#111;&#115;&#097;&#046;&#118;&#097;&#108;&#105;&#097;&#110;&#116;&#101;&#064;&#105;&#110;&#097;&#102;&#046;&#105;&#116;<\/a><\/span><\/p>\n\n\n\n<p><\/p>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:33% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"238\" height=\"319\" src=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/03\/photo.png\" alt=\"\" class=\"wp-image-454 size-full\" srcset=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/03\/photo.png 238w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2024\/03\/photo-224x300.png 224w\" sizes=\"auto, (max-width: 238px) 100vw, 238px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p><\/p>\n\n\n\n<p class=\"has-large-font-size\">Alessandra Venditti<\/p>\n\n\n\n<p><em>Univ. Sapienza &#8211; PhD Student<\/em><\/p>\n\n\n\n<p>First stars and galaxies; low-metallicity environments at high z; cosmological simulations; photoionization and radiative transfer<\/p>\n\n\n\n<p><a  href=\"javascript:smae_decode('dmVuZGl0dGkuMTc1MTg1MEBzdHVkZW50aS51bmlyb21hMS5pdA==');\" target=\"_blank\"  rel=\"noreferrer noopener\">&#118;&#101;&#110;&#100;&#105;&#116;&#116;&#105;&#046;&#049;&#055;&#053;&#049;&#056;&#053;&#048;&#064;&#115;&#116;&#117;&#100;&#101;&#110;&#116;&#105;&#046;&#117;&#110;&#105;&#114;&#111;&#109;&#097;&#049;&#046;&#105;&#116;<\/a><\/p>\n\n\n\n<p><\/p>\n<\/div><\/div>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:33% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"1024\" height=\"636\" src=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/01\/Abell370_HST_FF_v3-1024x636.png\" alt=\"\" class=\"wp-image-11 size-full\" srcset=\"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/01\/Abell370_HST_FF_v3-1024x636.png 1024w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/01\/Abell370_HST_FF_v3-300x186.png 300w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/01\/Abell370_HST_FF_v3-768x477.png 768w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/01\/Abell370_HST_FF_v3-1536x954.png 1536w, https:\/\/www.oa-roma.inaf.it\/caesar\/wp-content\/uploads\/sites\/17\/2021\/01\/Abell370_HST_FF_v3.png 1786w\" sizes=\"auto, (max-width: 767px) 89vw, (max-width: 1000px) 54vw, (max-width: 1071px) 543px, 580px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p><\/p>\n\n\n\n<p class=\"has-large-font-size\">Tommaso Zana<\/p>\n\n\n\n<p><em>Univ. Sapienza &#8211;<\/em> <em><em>Post-Doctoral Research Assistant<\/em><\/em><\/p>\n\n\n\n<p>&#8230;<\/p>\n\n\n\n<p><a  href=\"javascript:smae_decode('dG9tbWFzby56YW5hQGluYWYuaXQ=');\" target=\"_blank\"  rel=\"noreferrer noopener\">&#116;&#111;&#109;&#109;&#097;&#115;&#111;&#046;&#122;&#097;&#110;&#097;&#064;&#105;&#110;&#097;&#102;&#046;&#105;&#116;<\/a><\/p>\n\n\n\n<p><\/p>\n<\/div><\/div>\n\n\n\n<p><\/p>\n","protected":false},"excerpt":{"rendered":"<p>The group currently (February 2024) consists of xx members among staff, TD researchers, Post-Doc, PhD students, fellows and (Astro)Physics students, and xx group affiliates.&nbsp; Federico Angeloni Univ. Sapienza &#8211; PhD Student BH\/NS merger population modelling, Galaxy Formation and Evolution&nbsp;Models,&nbsp; High Performance Computing, Waveform Modelling from Compact and Exotic Compact Objects &#102;&#101;&#100;&#101;&#114;&#105;&#099;&#111;&#046;&#097;&#110;&#103;&#101;&#108;&#111;&#110;&#105;&#064;&#114;&#111;&#109;&#097;&#049;&#046;&#105;&#110;&#102;&#110;&#046;&#105;&#116; Antonello Calabr\u00f2 INAF-OAR &#8211; &hellip; <\/p>\n<p class=\"link-more\"><a href=\"https:\/\/www.oa-roma.inaf.it\/caesar\/who-we-are\/\" class=\"more-link\">Continue reading<span class=\"screen-reader-text\"> &#8220;People&#8221;<\/span><\/a><\/p>\n","protected":false},"author":2,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"_acf_changed":false,"footnotes":""},"class_list":["post-22","page","type-page","status-publish","hentry"],"acf":[],"_links":{"self":[{"href":"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-json\/wp\/v2\/pages\/22","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-json\/wp\/v2\/comments?post=22"}],"version-history":[{"count":39,"href":"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-json\/wp\/v2\/pages\/22\/revisions"}],"predecessor-version":[{"id":484,"href":"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-json\/wp\/v2\/pages\/22\/revisions\/484"}],"wp:attachment":[{"href":"https:\/\/www.oa-roma.inaf.it\/caesar\/wp-json\/wp\/v2\/media?parent=22"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}