Dual-Beam Phase Referencing with VERA

Details Dual-Beam Phase Referencing with VERA Dual-Beam Phase Referencing with VERA

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..340..569h&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

Scientific paper

We present the recent results of phase-referencing observations with VERA's dual-beam system. Since the first fringe detection with the dual-beam system in May 2002, several observations have been made to check the system performance and in particular to test how the VERA's dual-beam system works in phase-referencing observation. Among these observations, we mainly focus on the observations of a pair of strong maser sources W49N and OH43.8-0.1, and discuss the phase-referencing capability as well as potential astrometric accuracy of VERA.

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