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Structure Effects for 3417 Celestial Reference Frame Radio Sources

  • Authors: M. H. Xu, J. M. Anderson, R. Heinkelmann, S. Lunz, H. Schuh, and G. L. Wang

2019 The Astrophysical Journal Supplement Series 242 5.

  • Provider: AAS Journals

Caption: Figure 11.

Plots of closure amplitudes at the X band for source 2229+695 as a function of GMST for two quadrangles, (a) KOKEENYALES20WETTZELLTSUKUB32 and (b) BADARYKOKEEYEBES40MWETTZELL. See Figure 5 for a description of the plot design. The magnitudes of the patterns in both plots increased, and the changes of the patterns with respect to GMST became more and more rapid.

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