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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 6.

Plots of closure amplitudes at the X band of source 0016+731 as a function of GMST for three quadrangles, (a) GILCREEKKOKEEWETTZELLNRAO85_3, (b) KOKEETSUKUB32WETTZELLYEBES40M, and (c) ISHIOKAKOKEEYEBES40MWETTZELL. See Figure 5 for a description of the plot design. The structure-effect patterns in plots b and c can simply be combined because ISHIOKA and TSUKUB32 are two stations at the same site. The evolution of its structure effects is seen from the three plots.

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