Fig. A.1.
Comparison of total flux densities of 3 GHz detections between our procedure and catalogue flux densities, both at S/N > 5 (Smolčić et al. 2017a, red dots) and at 3 < S/N < 5 (Jin et al. 2018, blue dots). Squares highlight the median ratio at various intervals. The global offset and dispersion suggest a good agreement within the uncertainties down to S/N ∼ 3.
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