Fig. C.1
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Chip dependent completeness plots as a function of apparent JHKs magnitudes in the original HAWK-I images and the denebulised HAWK-I images. Completeness was determined through the generation of 50 artificial sources in each of the HAWK-I J–,H– and Ks-band image chips and our ability to recover these sources using the same photometric procedure employed and described in Section 3.
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