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
Table4—Continued
SourceName
SourcePositionα(2000)δ(2000)
1.4GHz
(mJy)
5GHz(mJy)
15GHz(mJy)
SpectralIndex
θ(′′)
Note.—The rstcolumnpresentssourcenameforthemasers(boldface)andtheextragalacticradiosources.ThenexttwocolumnslisttheirJ2000equatorialcoordinates.Forthemasersourcesthenextcolumngivesacommonname(ifavailable).Forthecalibratorsourcescolumns4to6givetheintegrated uxdensityatL-(fromNVSS),peak uxdensityatC-andU-bands,respectively.Column7isthespectralindexbetweenC-andU-bands(Sν~ν α).Column8istheupperlimitsofsourcesizes(FWHMofthemaximummajoraxesofthesourcesasdeterminedfromtheGaussian tsusingAIPStaskJMFIT).ThedatacomefromC-bandobservedwithC-con guration,exceptthosemarkedbysigns.Thelastcolumngivestheseparationbetweenmasersandcalibrators.Somesourceshavenodataduetofailureofthetelescope.
aU-bandbU-bandcU-banddSourceeSource
dataobservedwithCcon guration.dataobservedwithAcon guration.dataobservedwithBcon guration.listedinGregory&Condon(1991).
listedinVLBAcalibratorsource(Petrovetal.2005).