Next: Limitations on Imaging Performance
Up: PERFORMANCE OF THE VLA
Previous: Subarrays
Contents
The accuracy with which an object's position can be determined is
limited by the atmospheric phase stability, the closeness of a
suitable (astrometric) calibrator, and the calibrator-source cycle
time. Under good conditions, in A configuration, accuracies of
about 0.05 arcseconds can be obtained. Under more normal conditions,
accuracies of perhaps 0.1 arcseconds can be expected. Under
extraordinary conditions (probably attained only a few times per year
on calm winter nights in A configuration when using rapid phase
switching on a nearby astrometric calibrator - see Section
3.13.2), accuracies of 1 milliarcsecond have been
attained.
If highly accurate positions are desired, only `A' code (astrometric)
calibrators from the VLA Calibrator List should be used. The
positions of these sources are taken from lists published by the USNO.
Jim Ulvestad
2007-04-09