Astron. J., 147, 77 (2014/April-0)
Early science with the korean VLBI network: evaluation of system performance.
LEE S.-S., PETROV L., BYUN D.-Y., KIM J., JUNG T., SONG M.-G., OH C.S., ROH D.-G., JE D.-H., WI S.-O., SOHN B.W., OH S.-J., KIM K.-T., YEOM J.-H., CHUNG M.-H., KANG J., HAN S.-T., LEE J.-W., KIM B.G., CHUNG H., KIM H.-G., KIM H.R., KANG Y.-W. and CHO S.-H.
Abstract (from CDS):
We report the very long baseline interferometry (VLBI) observing performance of the Korean VLBI Network (KVN). The KVN is the first millimeter-dedicated VLBI network in East Asia. The KVN consists of three 21 m radio telescopes with baseline lengths in a range of 305-476 km. The quasi-optical system equipped on the antennas allows simultaneous observations at 22, 43, 86, and 129 GHz. The first fringes of the KVN were obtained at 22 GHz on 2010 June 8. Test observations at 22 and 43 GHz on 2010 September 30 and 2011 April 4 confirmed that the full cycle of VLBI observations works according to specification: scheduling, antenna control system, data recording, correlation, post-correlation data processing, astrometry, geodesy, and imaging analysis. We found that decorrelation due to instability in the hardware at times up to 600 s is negligible. The atmosphere fluctuations at KVN baseline are partly coherent, which allows us to extend integration time under good winter weather conditions up to 600 s without significant loss of coherence. The post-fit residuals at KVN baselines do not exhibit systematic patterns, and the weighted rms of the residuals is 14.8 ps. The KVN is ready to image compact radio sources both in snapshot and full-track modes with residual noise in calibrated phases of less than 2 deg at 22 and 43 GHz and with dynamic ranges of ∼300 for snapshot mode and ∼1000 for full-track mode. With simultaneous multi-frequency observations, the KVN can be used to make parsec-scale spectral index maps of compact radio sources.
instrumentation: interferometers - techniques: interferometric - telescopes
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