Figure 20 from Structure Effects for 3417 Celestial Reference Frame Radio Sources

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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 20.

Plot of the recalculated CARMS values based on closure amplitudes from non-VLBA observations (see its definition in the text) vs. that based on closure amplitudes from VLBA observations for 863 sources, which have been observed both by IVS non-VLBA stations and the VLBA stations. VLBA observations nearly always give smaller CARMS values.

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