{"id":1201,"date":"2023-09-14T19:07:47","date_gmt":"2023-09-14T19:07:47","guid":{"rendered":"https:\/\/astronomia.bedigital.cl\/?post_type=researcher&p=1201"},"modified":"2025-08-21T03:23:28","modified_gmt":"2025-08-21T03:23:28","slug":"pedro-henrique-soares-da-silva-de-pinho-nogueira","status":"publish","type":"researcher","link":"https:\/\/astronomia.udp.cl\/en\/researcher\/pedro-henrique-soares-da-silva-de-pinho-nogueira\/","title":{"rendered":"Pedro Henrique Soares da Silva de Pinho Nogueira"},"content":{"rendered":"\n
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Pedro Henrique Soares da Silva de Pinho Nogueira<\/h2>\n\n\n\n

Former PhD student<\/h4>\n\n\n\n

I am a former PhD student, graduated in 2024. I am interested in studying exoplanets, mainly with high-contrast imaging using near-infrared data.<\/p>\n\n\n\n

Projects<\/h5>\n\n\n\n

My current project focuses on an interesting system (Eta Telescopii) consisting of a giant star and a brown dwarf (BD). With several years of data, we are setting possible orbits of the BD around the star and also performing a search around the BD, aiming to test the limits of searching satellites around it, which we call exomoons. For the time we have only one candidate of exomoon, DH Tauri Bb, published by Lazzoni+ 2020. We are performing similar searches around other objects, including Eta Telescopii B, the BD. My objectives, apart from this publication, are to continue performing high-contrast imaging in systems, trying to discover and characterize planets and exomoons.<\/p>\n\n\n\n

Publications<\/h5>\n\n\n\n

NASA ADS<\/strong><\/a><\/p>\n\n\n\n

My PhD thesis titled “A mm and Near-IR study of YSOS : from outbursting protostars to satellite<\/strong>s” can be found here<\/a>.<\/p>\n\n\n\n

Extracurricular activities<\/h5>\n\n\n\n

Table tennis training and a weekly futsal match with UDP astronomy students.<\/p>\n<\/div>\n<\/div>\n","protected":false},"excerpt":{"rendered":"

Former PhD student, interested in the discovery and characterization of exoplanets and exomoons, mainly with high-contrast imaging using near-infrared data.<\/p>\n","protected":false},"author":2,"featured_media":4790,"menu_order":0,"template":"","meta":{"_monsterinsights_skip_tracking":false,"_monsterinsights_sitenote_active":false,"_monsterinsights_sitenote_note":"","_monsterinsights_sitenote_category":0,"site-sidebar-layout":"default","site-content-layout":"default","ast-global-header-display":"","ast-banner-title-visibility":"","ast-main-header-display":"","ast-hfb-above-header-display":"","ast-hfb-below-header-display":"","ast-hfb-mobile-header-display":"","site-post-title":"disabled","ast-breadcrumbs-content":"","ast-featured-img":"disabled","footer-sml-layout":"","theme-transparent-header-meta":"","adv-header-id-meta":"","stick-header-meta":"","header-above-stick-meta":"","header-main-stick-meta":"","header-below-stick-meta":""},"researcher-category":[259],"acf":[],"_links":{"self":[{"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/researcher\/1201"}],"collection":[{"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/researcher"}],"about":[{"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/types\/researcher"}],"author":[{"embeddable":true,"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/users\/2"}],"version-history":[{"count":8,"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/researcher\/1201\/revisions"}],"predecessor-version":[{"id":7879,"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/researcher\/1201\/revisions\/7879"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/media\/4790"}],"wp:attachment":[{"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/media?parent=1201"}],"wp:term":[{"taxonomy":"researcher-category","embeddable":true,"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/researcher-category?post=1201"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}