Processing VLBA Geodetic/Astrometric Data

Details Processing VLBA Geodetic/Astrometric Data Processing VLBA Geodetic/Astrometric Data

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..340..517g&link_type=abstract

Future Directions in High Resolution Astronomy: The 10th Anniversary of the VLBA, ASP Conference Proceedings, Vol. 340. Edited

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The GSFC VLBI group uses AIPS and Calc/Solve for geodetic and astrometric processing of VLBA correlated experiments, including the RDV, VCS1, VCS2, K/Q, and various antenna ties sessions. A VLBA vs. Mark4 correlator comparison shows group delay agreement averaging 12 psec RMS over baselines of 240 to 5000 km. Geodetic solutions for antenna axis offsets and fixed axis tilts are also presented.

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