VLBI observations in Cluster-Cluster mode at 1.6 GHz

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dc.creatorRioja, M. J.
dc.creatorPorcas, R. W.
dc.creatorDesmurs, J. -F.
dc.creatorAlef, W.
dc.creatorGurvits, L. I.
dc.creatorSchilizzi, R. T.
dc.date2002-07-10
dc.date.accessioned2026-07-07T02:04:15Z
dc.date.available2026-07-07T02:04:15Z
dc.descriptionWe describe, and present preliminary results from the analysis of 1.6 GHz VLBI observations, made in Cluster-Cluster mode between subgroups of antennas from the WSRT, VLA and MERLIN arrays. We observed for two 6-hour periods on consecutive days, simultaneously monitoring 4 compact radio sources with angular separations ranging from ~1 to 9 degrees. The data were recorded in a non-standard MkIII mode using special set-ups, and correlated at the MPIfR MkIIIa correlator. The preliminary results from standard and phase reference analyses are very encouraging. The experiment has provided a useful database for investigating the potential of this new observing technique at low frequencies.
dc.descriptionProceedings of the 6th European VLBI Network Symposium (p57-60), Ros, E., Porcas, R.W., Lobanov, A.P., & Zensus, J.A. (eds.), MPIfR, Bonn, Germany (2002). 4 pages, 5 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0207210
dc.identifierhttp://arxiv.org/abs/astro-ph/0207210
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4676
dc.subjectAstrophysics
dc.titleVLBI observations in Cluster-Cluster mode at 1.6 GHz
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