Towards a Large Field of View Archive for the European VLBI Network

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dc.creatorvan Langevelde, Huib Jan
dc.creatorOlnon, Friso
dc.creatorVerkouter, Harro
dc.creatorKramer, Bauke
dc.creatorGarrett, Mike
dc.creatorSzomoru, Arpad
dc.creatorParsley, Steve
dc.creatorBos, Albert
dc.date2004-01-05
dc.date.accessioned2026-07-07T02:11:46Z
dc.date.available2026-07-07T02:11:46Z
dc.descriptionTraditionally VLBI observations focus on a small patch of sky and image typically a few 100 mas around a bright source, which is often used to self-calibrate the data. High spectral and time resolution is needed to image a larger area, in principle up to the primary beam of the individual telescopes. The EVN MkIV data processor at JIVE is being upgraded to make such high resolution data its standard product. From the archive of high resolution data it will be possible to image many sources in each field of view around the original targets.
dc.description4 pages, 1 figure, submitted to the conference proceedings of ADASS 2003, Strasbourg, ASP conference proceeding
dc.identifierhttps://arxiv.org/abs/astro-ph/0401014
dc.identifierhttp://arxiv.org/abs/astro-ph/0401014
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7216
dc.subjectAstrophysics
dc.titleTowards a Large Field of View Archive for the European VLBI Network
dc.typetext

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