The XXL Survey - XXIX. GMRT 610 MHz continuum observations

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Table 1

Differential incompleteness measures, i.e. detection fraction as a function of 610 MHz flux density for the GMRT-XXL-N 610 MHz survey relative to the VLA-COSMOS 3 GHz Large Project source counts, and separated into two areas (inner and outer field) with different 1σ sensitivity limits.

Inner area	(9.6 deg²)	Outer area	(12.66 deg²)

S_610 MHz	Detection	S_610 MHz	Detection
[mJy]	fraction	[mJy]	fraction
1.92	0.45	0.39	0.34
2.96	0.65	0.51	0.75
4.58	0.94	0.67	0.80
		0.87	0.87
		1.24	0.87
		1.92	0.92
		2.96	0.96
		4.58	0.95

Notes. The estimated uncertainty of the detection fractions computed in this way is ~ 10%. Beyond the flux densities given here, we consider the survey complete (see text for details).

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