Fig. 9
VLBA detection fraction as a function of SVLA. Only the VLBA detectable sources have been considered to compute this fraction. The VLA flux densities have been separated into bins corresponding to 55μJy × 
, where N = 0, 1, 2, ... The error bars have been calculated using the Bayesian technique for binomial populations as described by Cameron (2011, 1σ confidence interval).
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