2004/01/05 by Huib Jan van Langevelde, Friso Olnon, F. Olnon +16
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Radio Astronomy Observations and Technology #Superconducting and THz Device Technology #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0401014
4 pages, 1 figure, submitted to the conference proceedings of ADASS 2003, Strasbourg, ASP conference proceeding
arxiv created 2004/01/05 · openalex publication_date 2004/01/05 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Traditionally 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.