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Fig. 2


J- and K-band completeness curves for the target galaxies. The dashed line shows the 50% completeness level. Dots delineate curves computed using stars from the central region of the galaxy, while crosses are for stars located in the outskirts of the galaxy (see text for details). We overplot the best-fitting analytic completeness functions as solid lines (Fleming et al. 1995). Even for the most crowded field (ESO269-066), the inner and outer completeness curves differ very little.

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