We have used the Very Large Array to search for compact milliarcsecond-size radio sources near methanol masers in high-mass star-forming regions. Such sources are required for Very Long Baseline Interferometry phase-referencing observations. We conducted p
parisonofCalibratorPositionErrorsDerivedfromVLAandVLBIData
SourceName
VLA-CPositionα(2000)δ(2000)
(Y/C VLBI)
(arcsec)
VLA-APositionα(2000)δ(2000)
(Y/A VLBI)
(arcsec)
VLBI
α(2000)δ(2000)
Error
(mas)
Note.—-Listedare,lefttoright,sourcename,positionderivedfromVLAC-arrayobservations,di erencebetweenthelatterandtheVLBIposition(easto setandnortho set),positionderivedfromVLAA-arrayobservations,di erencebetweenthelatterandtheVLBIposition,andtheVLBIpositionanditsuncertainties.Ofthecoordinatesforthelattertwopositionsonlysecondsoftimeandarcsecondsaregiven.
a
FromourVLBAobservations(Xuetal.2006).
bFromVCS3(Petrovetal.2005).