Figure 10 from IVS OBSERVATION OF ICRF2-GAIA TRANSFER SOURCES

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IVS OBSERVATION OF ICRF2-GAIA TRANSFER SOURCES

Authors: K. Le Bail, J. M. Gipson, D. Gordon, D. S. MacMillan, D. Behrend, C. C. Thomas, S. Bolotin, W. E. Himwich, K. D. Baver, B. E. Corey, M. Titus, G. Bourda, P. Charlot, and A. Collioud

2016 The Astronomical Journal 151 79.

Provider: AAS Journals

Caption: Figure 10.

SEFD vs. SNR. Four different cases are illustrated for sources with flux values of 0.025, 0.100, 0.220, and 0.500 Jy. Baselines T6-Ny, On-Ny, and Ft-Ny are indicated for reference. To be scheduled, a source must be above the dotted lines indicating the SNR targets used in sked (20 for X band, 15 for S band) and 600 s scans.

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