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Sub‐Milliarcsecond Precision of Pulsar Motions: Using In‐Beam Calibrators with the VLBA

  • Authors: E. B. Fomalont, W. M. Goss, A. J. Beasley, and S. Chatterjee

Fomalont et al. 1999 The Astronomical Journal 117 3025.

  • Provider: AAS Journals

Caption: Fig. 1.

Self‐calibrator phases for in‐beam calibrator J1900−2602. Each plotted point shows the residual phase determined every five minutes averaging all eight frequency channels. Antenna 5 at Los Alamos was the reference antenna. The scatter becomes somewhat larger for MK and SC, which are the longer baselines. The continuity of the phases with time is far from random for this 7 mJy source.

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