Abstract
The calibration of Very Long Baseline Interferometry (VLBI) data has long been a time consuming process. The Korean VLBI Network (KVN) is a simple array consisting of three identical antennas. Because four frequencies are observed simultaneously, phase solutions can be transferred from lower frequencies to higher frequencies in order to improve phase coherence and hence sensitivity at higher frequencies. Due to the homogeneous nature of the array, the KVN is also well suited for automatic calibration. In this paper we describe the automatic calibration of single-polarisation KVN data using the KVN Pipeline and comparing the results against VLBI data that has been manually reduced. We find that the pipelined data using phase transfer produces better results than a manually reduced dataset not using the phase transfer. Additionally we compared the pipeline results with a manually reduced phase-transferred dataset and found the results to be identical.
Original language | English |
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Pages (from-to) | 137-144 |
Number of pages | 8 |
Journal | Journal of the Korean Astronomical Society |
Volume | 49 |
Issue number | 4 |
DOIs | |
State | Published - Aug 2016 |
Bibliographical note
Publisher Copyright:© 2016. The Korean Astronomical Society. All rights reserved.
Keywords
- KVN: pipeline: calibration