{"id":6466,"date":"2022-11-01T16:00:08","date_gmt":"2022-11-01T16:00:08","guid":{"rendered":"https:\/\/raege-az.pt\/?p=6466"},"modified":"2022-12-12T16:26:57","modified_gmt":"2022-12-12T16:26:57","slug":"instalacao-do-novo-recetor-vgos","status":"publish","type":"post","link":"https:\/\/raege-az.pt\/en\/instalacao-do-novo-recetor-vgos\/","title":{"rendered":"Installation of the new VGOS receiver"},"content":{"rendered":"
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The RAEGE Station of Santa Maria (RAEGSMAR) was recently equipped with a new high-tech VGOS receiver. The radio telescope of this station, with a 13.2m diameter paraboloid, was previously equipped with a tri-band receiver (S\/X\/Ka) until last October, which allowed us to participate in IVS R1\/R4 sessions since May 2021.<\/p>

During the month of October, the RAEGE Santa Maria station was the stage for intense and exciting integration work on the VGOS network, with the installation of this new receiver (represented on the right). The installation of this high-tech equipment allows the station to improve the VLBI data and thus walk alongside the most prestigious institutions, observatories, and stations in the pursuit of the Community of Space Geodesy's goal of 1 mm precision and 0.1 mm\/year accuracy.<\/p>

Over the course of two weeks, a team of 5 engineers from Yebes Observatory, together with the local 10-person team from RAEGE Santa Maria (see figure below) successfully installed the new receiver and backend equipment: one DBBC3, two MARK6, baseband down-converters, and a new cable delay measurement system (CDMS).<\/p>\t\t\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/div>\n\t\t\t\t

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\n\t\t\t\t\t\n\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\tBack to news page<\/span>\n\t\t\t\t\t<\/span>\n\t\t\t\t\t<\/a>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/section>\n\t\t\t\t<\/div>","protected":false},"excerpt":{"rendered":"

A Esta\u00e7\u00e3o RAEGE de Santa Maria (RAEGSMAR) foi equipada recentemente com um novo recetor VGOS de alta tecnologia. O radiotelesc\u00f3pio desta esta\u00e7\u00e3o, com um paraboloide de 13,2m de di\u00e2metro, estava equipado anteriormente com um recetor tri-banda (S\/X\/Ka) at\u00e9 outubro passado e que nos permitia participar nas sess\u00f5es IVS R1\/R4 desde maio de 2021. Durante o […]<\/p>","protected":false},"author":1,"featured_media":6468,"comment_status":"closed","ping_status":"open","sticky":false,"template":"elementor_theme","format":"standard","meta":{"site-sidebar-layout":"default","site-content-layout":"default","ast-site-content-layout":"","site-content-style":"default","site-sidebar-style":"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":"","ast-breadcrumbs-content":"","ast-featured-img":"","footer-sml-layout":"","theme-transparent-header-meta":"default","adv-header-id-meta":"","stick-header-meta":"","header-above-stick-meta":"","header-main-stick-meta":"","header-below-stick-meta":"","astra-migrate-meta-layouts":"default","ast-page-background-enabled":"default","ast-page-background-meta":{"desktop":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"tablet":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"mobile":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""}},"ast-content-background-meta":{"desktop":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"tablet":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"mobile":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""}},"footnotes":""},"categories":[19],"tags":[],"class_list":["post-6466","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-noticias"],"yoast_head":"\nInstala\u00e7\u00e3o do novo recetor VGOS - RAEGE-Az<\/title>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/raege-az.pt\/en\/instalacao-do-novo-recetor-vgos\/\" \/>\n<meta property=\"og:locale\" content=\"en_GB\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Instala\u00e7\u00e3o do novo recetor VGOS - RAEGE-Az\" \/>\n<meta property=\"og:description\" content=\"A Esta\u00e7\u00e3o RAEGE de Santa Maria (RAEGSMAR) foi equipada recentemente com um novo recetor VGOS de alta tecnologia. O radiotelesc\u00f3pio desta esta\u00e7\u00e3o, com um paraboloide de 13,2m de di\u00e2metro, estava equipado anteriormente com um recetor tri-banda (S\/X\/Ka) at\u00e9 outubro passado e que nos permitia participar nas sess\u00f5es IVS R1\/R4 desde maio de 2021. 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