{"id":1625,"date":"2024-07-15T11:29:37","date_gmt":"2024-07-15T09:29:37","guid":{"rendered":"http:\/\/brera.inaf.it\/?post_type=tesi&p=1625"},"modified":"2025-05-26T18:01:20","modified_gmt":"2025-05-26T16:01:20","slug":"time-variable-phenomena-in-astrophysics-bachelor-master-merate-lc","status":"publish","type":"tesi","link":"https:\/\/brera.inaf.it\/en\/tesi\/time-variable-phenomena-in-astrophysics-bachelor-master-merate-lc\/","title":{"rendered":"\u00a0Time variable phenomena in astrophysics – Bachelor\/Master – MERATE (LC) – Covino, Landoni."},"content":{"rendered":"\n
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\u00a0Time variable phenomena in astrophysics<\/span><\/h5>\n\n\n\n
Bachelor\/Master<\/h5>\n\n\n\n
Site: Merate (LC)<\/h5>\n\n\n\n
Duration<\/h5>\n\n\n\n

3 months (bachelor) – 1 year (master)<\/p>\n\n\n\n

Tutor<\/h5>\n\n\n\n

Stefano Covino, Marco Landoni<\/p>\n\n\n\n

Contact<\/h5>\n\n\n\n

stefano.covino AT inaf.it
marco.landoni AT inaf.it<\/p>\n\n\n\n

Description<\/h5>\n\n\n\n
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Triennial Thesis<\/strong> (first level): Analysis of astrophysical time-series to identify possible periodicities and estimate power spectral densities.<\/p>\n\n\n\n

Master Thesis<\/strong> (second level): Analysis of astrophysical time-series to identify possible periodicities and estimate power spectral densities. In particular we are going to apply advanced statistical tools such as Gaussian Processes or neural networks to carry out proper inferences.<\/p>\n\n\n\n[Credit image: web]<\/em><\/p>\n<\/div>\n<\/div>\n<\/div>\n\n\n\n

<\/p>\n","protected":false},"excerpt":{"rendered":"

\u00a0Time variable phenomena in astrophysics Bachelor\/Master Site: Merate (LC) Duration 3 months (bachelor) – 1 year (master) Tutor Stefano Covino, Marco Landoni Contact stefano.covino AT inaf.itmarco.landoni AT inaf.it Description Triennial Thesis (first level): Analysis of astrophysical time-series to identify possible periodicities and estimate power spectral densities. Master Thesis (second level): Analysis of astrophysical time-series to identify possible […]<\/p>\n","protected":false},"author":1,"featured_media":1629,"parent":0,"menu_order":0,"comment_status":"open","ping_status":"closed","template":"","format":"standard","meta":{"footnotes":""},"categories":[29,28,26],"tags":[241,48,242,243,244,234,245],"class_list":["post-1625","tesi","type-tesi","status-publish","format-standard","has-post-thumbnail","hentry","category-bachelor-thesis","category-master-thesis","category-thesis","tag-gaussian-processes-en","tag-marco-landoni-en","tag-neural-networks-en","tag-periodicities-en","tag-power-spectral-densities-en","tag-stefano-covino-en","tag-time-series-en"],"blocksy_meta":[],"featured_image_urls":{"full":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/copertina-tesi-triennale-magistrale-Covino.png",546,356,false],"thumbnail":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/copertina-tesi-triennale-magistrale-Covino.png",150,98,false],"medium":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/copertina-tesi-triennale-magistrale-Covino.png",300,196,false],"medium_large":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/copertina-tesi-triennale-magistrale-Covino.png",546,356,false],"large":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/copertina-tesi-triennale-magistrale-Covino.png",546,356,false],"1536x1536":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/copertina-tesi-triennale-magistrale-Covino.png",546,356,false],"2048x2048":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/07\/copertina-tesi-triennale-magistrale-Covino.png",546,356,false]},"post_excerpt_stackable":"

\u00a0Time variable phenomena in astrophysics Bachelor\/Master Site: Merate (LC) Duration 3 months (bachelor) – 1 year (master) Tutor Stefano Covino, Marco Landoni Contact stefano.covino AT inaf.itmarco.landoni AT inaf.it Description Triennial Thesis (first level): Analysis of astrophysical time-series to identify possible periodicities and estimate power spectral densities. Master Thesis (second level): Analysis of astrophysical time-series to identify possible periodicities and estimate power spectral densities. In particular we are going to apply advanced statistical tools such as Gaussian Processes or neural networks to carry out proper inferences. [Credit image: web]<\/p>\n","category_list":"Bachelor thesis<\/a>, Master thesis<\/a>, 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\/1625","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=1625"}],"version-history":[{"count":9,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/tesi\/1625\/revisions"}],"predecessor-version":[{"id":6847,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/tesi\/1625\/revisions\/6847"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/media\/1629"}],"wp:attachment":[{"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/media?parent=1625"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/categories?post=1625"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/tags?post=1625"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}