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The XXL Survey

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Figure

Fig. 1. Observed magnitude distribution of all optical objects present in the z Dec band catalogue within a radius of 3 00 around each radio source is shown by the black solid histogram
Fig. 2. Visual representation of the effect that produces negative val- val-ues at faint magnitudes of the expected probability distribution of the true optical counterparts
Fig. 5. Overlap between the position of the NIR sources (black tiles) and radio sources (red points)
Table 1. Results of the identification process using the likelihood ratio technique in seven different bands Band Magnitude No
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