{"id":1783,"date":"2024-07-16T16:07:48","date_gmt":"2024-07-16T14:07:48","guid":{"rendered":"http:\/\/brera.inaf.it\/?post_type=tesi&#038;p=1783"},"modified":"2025-05-26T18:06:19","modified_gmt":"2025-05-26T16:06:19","slug":"technological-thesis-tolerances-analysis-for-the-innovative-euv-grazing-incidence-hettrick-bowyer-telescope-for-the-mantis-cubesat-master-merate-lc","status":"publish","type":"tesi","link":"https:\/\/brera.inaf.it\/en\/tesi\/technological-thesis-tolerances-analysis-for-the-innovative-euv-grazing-incidence-hettrick-bowyer-telescope-for-the-mantis-cubesat-master-merate-lc\/","title":{"rendered":"\u00a0Technological thesis &#8211; Master &#8211; MERATE (LC) &#8211; Tolerances analysis for the innovative EUV grazing incidence Hettrick-Bowyer telescope for the MANTIS CubeSat &#8211; Civitani."},"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=\"440\" height=\"440\" src=\"http:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/icona-MANTIS.png\" alt=\"\" class=\"wp-image-1784\"\/><\/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\">Technological thesis<\/span><\/h5>\n\n\n\n<h5 class=\"wp-block-heading\">Master<\/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>1 year<\/p>\n\n\n\n<h5 class=\"wp-block-heading\">Tutor<\/h5>\n\n\n\n<p>Marta M. Civitani<\/p>\n\n\n\n<h5 class=\"wp-block-heading\">Contact<\/h5>\n\n\n\n<p>marta.civitani 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><strong>Description<\/strong>:<br><strong>MANTIS<\/strong> (Monitoring Activity of Nearby sTars with UV Imaging and Spectroscopy) is a 12U&nbsp;<strong>CubeSat mission<\/strong>&nbsp;submitted by the University of Colorado at Boulder to the NASA APRA call (December 2022). The MANTIS CubeSat is designed to measure the ultraviolet (UV) irradiance and variability of low-mass stars in order to better understand the&nbsp;<strong>environment for habitable-zone exoplanets<\/strong>. As part of this collaboration, the INAF is committed to provide scientific expertise in high-energy astrophysics, and a&nbsp;<strong>novel extreme EUV (10 -80 nm) grazing incidence Hettrick-Bowyer telescope<\/strong>.<\/p>\n\n\n\n<p>This thesis work aims at the&nbsp;<strong>tolerances analysi<\/strong>&nbsp;for the innovative grazing incidence optical system. This analysis will be the basis for the realization process definition and for the alignment procedure set-up. The activity will be carried out with&nbsp;<strong>ray-tracing numerical simulations<\/strong>&nbsp;(Matlab\/Python).<\/p>\n\n\n\n<p><em>[Image Credit: MANTIS CubeSat Mission]<\/em><\/p>\n<\/div>\n<\/div>\n<\/div>\n\n\n\n<p><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Technological thesis Master Site: Merate (LC) Duration 1 year Tutor Marta M. Civitani Contact marta.civitani AT inaf.it Description Description:MANTIS (Monitoring Activity of Nearby sTars with UV Imaging and Spectroscopy) is a 12U&nbsp;CubeSat mission&nbsp;submitted by the University of Colorado at Boulder to the NASA APRA call (December 2022). The MANTIS CubeSat is designed to measure the [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":1785,"parent":0,"menu_order":0,"comment_status":"open","ping_status":"closed","template":"","format":"standard","meta":{"footnotes":""},"categories":[28,26],"tags":[305,306,277,307,308,309],"class_list":["post-1783","tesi","type-tesi","status-publish","format-standard","has-post-thumbnail","hentry","category-master-thesis","category-thesis","tag-habitable-zone-exoplanets-en","tag-mantis-cubesat-mission-en","tag-marta-civitani-en","tag-ray-tracing-numerical-simulations-en","tag-tolerance-analysis-en","tag-ultraviolet-en"],"blocksy_meta":[],"featured_image_urls":{"full":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/icona-MANTIS.png",440,440,false],"thumbnail":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/icona-MANTIS.png",150,150,false],"medium":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/icona-MANTIS.png",300,300,false],"medium_large":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/icona-MANTIS.png",440,440,false],"large":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/icona-MANTIS.png",440,440,false],"1536x1536":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/icona-MANTIS.png",440,440,false],"2048x2048":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/icona-MANTIS.png",440,440,false]},"post_excerpt_stackable":"<p>Technological thesis Master Site: Merate (LC) Duration 1 year Tutor Marta M. Civitani Contact marta.civitani AT inaf.it Description Description:MANTIS (Monitoring Activity of Nearby sTars with UV Imaging and Spectroscopy) is a 12U&nbsp;CubeSat mission&nbsp;submitted by the University of Colorado at Boulder to the NASA APRA call (December 2022). The MANTIS CubeSat is designed to measure the ultraviolet (UV) irradiance and variability of low-mass stars in order to better understand the&nbsp;environment for habitable-zone exoplanets. As part of this collaboration, the INAF is committed to provide scientific expertise in high-energy astrophysics, and a&nbsp;novel extreme EUV (10 -80 nm) grazing incidence Hettrick-Bowyer telescope. This&hellip;<\/p>\n","category_list":"<a href=\"https:\/\/brera.inaf.it\/en\/category\/thesis\/master-thesis\/\" rel=\"category tag\">Master 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\/1783","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=1783"}],"version-history":[{"count":5,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/tesi\/1783\/revisions"}],"predecessor-version":[{"id":6853,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/tesi\/1783\/revisions\/6853"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/media\/1785"}],"wp:attachment":[{"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/media?parent=1783"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/categories?post=1783"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/tags?post=1783"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}