Fig. 13
Detection fraction as a function of 610 MHz flux density relative to the VLA-COSMOS 3 GHz Large Project (dashed line) for the inner area (9.6 square degrees, coincident with the XMM-LSS field; top panel) and outer area (12.66 square degree) areas. Also shown is the completeness (i.e. the detection fraction in a given bin and that above the given flux bin lower limit) as a function of flux density (full line).
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