{"id":1370,"date":"2024-07-11T11:13:24","date_gmt":"2024-07-11T09:13:24","guid":{"rendered":"http:\/\/brera.inaf.it\/?post_type=tesi&#038;p=1370"},"modified":"2025-05-26T18:19:38","modified_gmt":"2025-05-26T16:19:38","slug":"exoplanets-high-resolution-spectroscopy-studies-of-exoplanetary-atmospheres","status":"publish","type":"tesi","link":"https:\/\/brera.inaf.it\/en\/tesi\/exoplanets-high-resolution-spectroscopy-studies-of-exoplanetary-atmospheres\/","title":{"rendered":"Exoplanets &#8211; PhD &#8211; MERATE (LC) &#8211; High resolution spectroscopy studies of exoplanetary atmospheres &#8211; Borsa, Rainer."},"content":{"rendered":"\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-28f84493 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=\"744\" height=\"500\" src=\"http:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/copertina-phd-rainer2.png\" alt=\"\" class=\"wp-image-1371\"\/><\/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\"><span style=\"color: #cf2e2e;\" class=\"stk-highlight\">Exoplanets<\/span><\/h5>\n\n\n\n<h5 class=\"wp-block-heading\">Phd Thesis<\/h5>\n\n\n\n<h5 class=\"wp-block-heading\">Site: Merate (LC)<\/h5>\n\n\n\n<h5 class=\"wp-block-heading\">Duration<\/h5>\n\n\n\n<p>3 years<\/p>\n\n\n\n<h5 class=\"wp-block-heading\">Tutors<\/h5>\n\n\n\n<p>&nbsp;Francesco Borsa, Monica Rainer<\/p>\n\n\n\n<h5 class=\"wp-block-heading\">Contact<\/h5>\n\n\n\n<p>francesco.borsa AT inaf.it<br>monica.rainer AT inaf.it<\/p>\n\n\n\n<h5 class=\"wp-block-heading\">Description<\/h5>\n\n\n\n<div class=\"wp-block-group is-layout-constrained wp-block-group-is-layout-constrained\">\n<p>The characterization of&nbsp;<strong>exoplanetary atmospheres<\/strong>&nbsp;is today one of the&nbsp;<strong>hottest<\/strong>&nbsp;topics in astrophysics.<br>Close-in exoplanets are among the most interesting targets, sculpted by&nbsp;<strong>atmospheric escape<\/strong>&nbsp;driven by the X-ray\/UV flux of their host stars.<br>As of today, high-resolution (HR, R&gt;50,000)&nbsp;<strong>transmission spectroscopy<\/strong>&nbsp;(spectral time-series obtained while a planet, as seen from Earth, transits in front of its host star) and&nbsp;<strong>emission spectroscopy<\/strong>&nbsp;(when the planet is close to secondary eclipse, showing its dayside) are the ultimate techniques to investigate&nbsp;<strong>exoplanet atmospheres<\/strong>, and to study their chemical and physical properties.<br>As part of the&nbsp;<strong>GAPS<\/strong>&nbsp;(Global Architecture of Planetary Systems) project (<a href=\"https:\/\/theglobalarchitectureofplanetarysystems.wordpress.com\/\" target=\"_blank\" rel=\"noreferrer noopener\">https:\/\/theglobalarchitectureofplanetarysystems.wordpress.com\/<\/a>), which involves a team of national and international exoplanet-interested scientists and exploits a currently ongoing five-year Large Programme at the&nbsp;<strong>Telescopio Nazionale Galileo<\/strong>&nbsp;(60+ nights\/yr), we are performing atmospheric characterization of many exoplanets exploiting the HR optical and infrared spectrographs HARPS-N and GIANO-B.<br>Lots of data are waiting to be analyzed, in order to understand the atmospheric peculiarities of the single exoplanets and to put them in the broader context of exoplanetary atmospheres at large.<\/p>\n\n\n\n<p><em>[Crediti immagine: James Webb Telescope]<\/em><\/p>\n<\/div>\n<\/div>\n<\/div>\n\n\n\n<p><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Exoplanets Phd Thesis Site: Merate (LC) Duration 3 years Tutors &nbsp;Francesco Borsa, Monica Rainer Contact francesco.borsa AT inaf.itmonica.rainer AT inaf.it Description The characterization of&nbsp;exoplanetary atmospheres&nbsp;is today one of the&nbsp;hottest&nbsp;topics in astrophysics.Close-in exoplanets are among the most interesting targets, sculpted by&nbsp;atmospheric escape&nbsp;driven by the X-ray\/UV flux of their host stars.As of today, high-resolution (HR, R&gt;50,000)&nbsp;transmission spectroscopy&nbsp;(spectral [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":1372,"parent":0,"menu_order":0,"comment_status":"open","ping_status":"closed","template":"","format":"standard","meta":{"footnotes":""},"categories":[27,26],"tags":[122,117,118,119],"class_list":["post-1370","tesi","type-tesi","status-publish","format-standard","has-post-thumbnail","hentry","category-phd-thesis","category-thesis","tag-exoplanetary-atmospheres-en","tag-francesco-borsa-en","tag-high-resolution-spectra-en","tag-monica-rainer-en"],"blocksy_meta":[],"featured_image_urls":{"full":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/copertina-phd-rainer2.png",744,500,false],"thumbnail":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/copertina-phd-rainer2.png",150,101,false],"medium":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/copertina-phd-rainer2.png",300,202,false],"medium_large":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/copertina-phd-rainer2.png",744,500,false],"large":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/copertina-phd-rainer2.png",744,500,false],"1536x1536":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/copertina-phd-rainer2.png",744,500,false],"2048x2048":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/copertina-phd-rainer2.png",744,500,false]},"post_excerpt_stackable":"<p>Exoplanets Phd Thesis Site: Merate (LC) Duration 3 years Tutors &nbsp;Francesco Borsa, Monica Rainer Contact francesco.borsa AT inaf.itmonica.rainer AT inaf.it Description The characterization of&nbsp;exoplanetary atmospheres&nbsp;is today one of the&nbsp;hottest&nbsp;topics in astrophysics.Close-in exoplanets are among the most interesting targets, sculpted by&nbsp;atmospheric escape&nbsp;driven by the X-ray\/UV flux of their host stars.As of today, high-resolution (HR, R&gt;50,000)&nbsp;transmission spectroscopy&nbsp;(spectral time-series obtained while a planet, as seen from Earth, transits in front of its host star) and&nbsp;emission spectroscopy&nbsp;(when the planet is close to secondary eclipse, showing its dayside) are the ultimate techniques to investigate&nbsp;exoplanet atmospheres, and to study their chemical and physical properties.As part of&hellip;<\/p>\n","category_list":"<a href=\"https:\/\/brera.inaf.it\/en\/category\/thesis\/phd-thesis\/\" rel=\"category tag\">PhD thesis<\/a>, <a href=\"https:\/\/brera.inaf.it\/en\/category\/thesis\/\" rel=\"category tag\">Thesis<\/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\/tesi\/1370","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/tesi"}],"about":[{"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/types\/tesi"}],"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=1370"}],"version-history":[{"count":8,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/tesi\/1370\/revisions"}],"predecessor-version":[{"id":6867,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/tesi\/1370\/revisions\/6867"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/media\/1372"}],"wp:attachment":[{"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/media?parent=1370"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/categories?post=1370"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/tags?post=1370"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}