LBCS: the LOFAR Long-Baseline Calibrator Survey
N. Jackson, A. Tagore, A. Deller, J. Mold\'on, E. Varenius, L., Morabito, O. Wucknitz, T. Carozzi, J. Conway, A. Drabent, A. Kapinska, E., Orr\`u, M. Brentjens, R. Blaauw, G. Kuper, J. Sluman, J. Schaap, N. Vermaas,, M. Iacobelli, L. Cerrigone, A. Shulevski, S. ter Veen

TL;DR
The LBCS survey identifies suitable calibrator sources for high-resolution LOFAR observations over large sky areas, revealing the density, coherence times, and ionospheric effects impacting calibration at baselines up to 600 km.
Contribution
This work provides the first large-scale calibrator source catalog for LOFAR's long baselines, including detailed measurements of coherence times and ionospheric effects at 110-190 MHz.
Findings
Approximately 1 suitable calibrator per square degree for 200-300 km baselines.
Cal coherence times decrease with baseline length, down to about 1 minute at 600 km.
Phase transfer success is limited by ionospheric coherence patches of about 1 degree.
Abstract
(abridged). We outline LBCS (the LOFAR Long-Baseline Calibrator Survey), whose aim is to identify sources suitable for calibrating the highest-resolution observations made with the International LOFAR Telescope, which include baselines >1000 km. Suitable sources must contain significant correlated flux density (50-100mJy) at frequencies around 110--190~MHz on scales of a few hundred mas. At least for the 200--300-km international baselines, we find around 1 suitable calibrator source per square degree over a large part of the northern sky, in agreement with previous work. This should allow a randomly selected target to be successfully phase calibrated on the international baselines in over 50% of cases. Products of the survey include calibrator source lists and fringe-rate and delay maps of wide areas -- typically a few degrees -- around each source. The density of sources with…
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