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VLBI observations in Cluster-Cluster mode at 1.6 GHz

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arxiv astro-ph/0207210 v1 pith:JG2P4WYJ submitted 2002-07-10 astro-ph

classification astro-ph
keywords modecluster-clusterobservationspreliminaryresultsvlbianalysesanalysis
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We 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.

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Cited by 1 Pith paper

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  1. Serial MultiView: an efficient approach to mitigating atmospheric spatial-structure errors for VLBI astrometry

    astro-ph.IM 2025-01 conditional novelty 6.0 of 10

    Serial MultiView iteratively rotates a phase plane through time to calibrate atmospheric errors in VLBI astrometry, matching conventional MultiView at 5 GHz with reduced calibration sampling and automated phase ambigu...

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