{"id":6658,"date":"2019-06-14T12:00:00","date_gmt":"2019-06-14T10:00:00","guid":{"rendered":"https:\/\/www.ieec.cat\/global-high-precision-phase-delay-astrometry-at-mm-wavelengths-state-of-the-art-and-technical-limits\/"},"modified":"2023-01-17T15:06:54","modified_gmt":"2023-01-17T14:06:54","slug":"global-high-precision-phase-delay-astrometry-at-mm-wavelengths-state-of-the-art-and-technical-limits","status":"publish","type":"post","link":"https:\/\/www.ieec.cat\/en\/global-high-precision-phase-delay-astrometry-at-mm-wavelengths-state-of-the-art-and-technical-limits\/","title":{"rendered":"Global High-Precision Phase-Delay Astrometry at mm-Wavelengths: State-of-the-Art and Technical Limits"},"content":{"rendered":"<p>[et_pb_section fb_built=&#8221;1&#8243; fullwidth=&#8221;on&#8221; _builder_version=&#8221;4.14.8&#8243; _module_preset=&#8221;default&#8221; background_image=&#8221;\/wp-content\/uploads\/2022\/04\/slider-corpo2.jpg&#8221; height=&#8221;114px&#8221; global_colors_info=&#8221;{}&#8221;][\/et_pb_section][et_pb_section fb_built=&#8221;1&#8243; 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_builder_version=&#8221;4.14.8&#8243; _module_preset=&#8221;default&#8221; custom_margin=&#8221;0px||||false|false&#8221; custom_padding=&#8221;0px||||false|false&#8221; top_divider_color=&#8221;RGBA(255,255,255,0)&#8221; top_divider_height=&#8221;0px&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_row _builder_version=&#8221;4.14.8&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_column type=&#8221;4_4&#8243; _builder_version=&#8221;4.14.8&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_image src=&#8221;https:\/\/www.ieec.cat\/wp-content\/uploads\/2022\/12\/1560320134_d13e46ded0a42cfd118e0dd228d0b25e_2019_06_global_high_precision_phase_delay_astrometry.jpg&#8221; alt=&#8221;Global High-Precision Phase-Delay Astrometry at mm-Wavelengths: State-of-the-Art and Technical Limits&#8221; title_text=&#8221;Global High-Precision Phase-Delay Astrometry at mm-Wavelengths: State-of-the-Art and Technical Limits&#8221; _builder_version=&#8221;4.14.8&#8243; _module_preset=&#8221;default&#8221; width=&#8221;600px&#8221; module_alignment=&#8221;center&#8221; global_colors_info=&#8221;{}&#8221;][\/et_pb_image][et_pb_text _builder_version=&#8221;4.14.8&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;]Wide-angle high-precision differential phase-delay astrometry with VLBI at 7mm wavelength has been successfully demonstrated with state-of-the-art observations and analysis of a complete sample of 13 radio sources (Quasars and BL Lacs).<\/p>\n<p>With 20 mm wavelength observations separated by 10 years, the proper motions of the cores of the radio sources have been determined with unprecedented accuracy and with simultaneous 20\/7 mm wavelength observations the core-shift effect has been studied using three independent methods. The limits of the technique with the present instrumentation will be discussed.[\/et_pb_text][\/et_pb_column][\/et_pb_row][\/et_pb_section]<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Wide-angle high-precision differential phase-delay astrometry with VLBI at 7mm wavelength has been successfully demonstrated with state-of-the-art observations and analysis of a complete sample of 13 radio sources (Quasars and BL Lacs). With 20 mm wavelength observations separated by 10 years, the proper motions of the cores of the radio sources have been determined with unprecedented [&hellip;]<\/p>\n","protected":false},"author":0,"featured_media":6654,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_et_pb_use_builder":"on","_et_pb_old_content":"","_et_gb_content_width":"2880","footnotes":""},"categories":[72,94],"tags":[],"class_list":["post-6658","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-events","category-talk"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.5 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>Global High-Precision Phase-Delay Astrometry at mm-Wavelengths: State-of-the-Art and Technical Limits - IEEC<\/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:\/\/www.ieec.cat\/en\/global-high-precision-phase-delay-astrometry-at-mm-wavelengths-state-of-the-art-and-technical-limits\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Global High-Precision Phase-Delay Astrometry at mm-Wavelengths: State-of-the-Art and Technical Limits - IEEC\" \/>\n<meta property=\"og:description\" content=\"Wide-angle high-precision differential phase-delay astrometry with VLBI at 7mm wavelength has been successfully demonstrated with state-of-the-art observations and analysis of a complete sample of 13 radio sources (Quasars and BL Lacs). 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