Revisited "Cluster-Cluster" VLBI with future multi-beam low frequency radio interferometers
M. J. Rioja, R. Dodson, R. W. Porcas, D. Ferris, J. Reynolds, T., Sasao, R. T. Schilizzi

TL;DR
This paper explores the synergy of multi-beam VLBI techniques with ASKAP to enhance astrometric precision, wide-field mapping, and future high-resolution observations with the SKA by revisiting and proposing improvements to the 'Cluster-Cluster' VLBI method.
Contribution
It demonstrates how multi-view VLBI with ASKAP can improve calibration, positional accuracy, and enable wide-field mapping, contributing to future SKA observations.
Findings
Multi-view VLBI improves ionospheric calibration.
Joint ASKAP and multi-site observations increase astrometric precision.
Potential for very wide-field VLBI mapping.
Abstract
We revisit the "Cluster-Cluster" or multi-view Very-Long-Baseline-Interferometry (VLBI) technique from the perspective of its synergy with the multi-beam features inherent in the Australian Square Kilometer Array Pathfinder (ASKAP)and its potential to improve the outcomes of VLBI observations with ASKAP. We include a list of candidate VLBI sites that already support or can be upgraded to support multi-view VLBI located in Australia and overseas, and which have common visibility with ASKAP. The results of our previous "cluster-cluster" observations at 1.6 GHz demonstrated the advantages of this configuration to calibrate the ionospheric distortions responsible for the loss of positional accuracy at low frequencies, using multiple calibrators in a range between 1 to 6 degrees away from the target. Therefore, we conclude that joint observations of ASKAP with other multi-view sites using…
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Taxonomy
TopicsRadio Astronomy Observations and Technology · Astrophysics and Cosmic Phenomena · Galaxies: Formation, Evolution, Phenomena
