Fig. 4
Left: completeness as a function of the mF814W magnitude in five annuli (the inner and outer radius of each annulus, in ACS pixels, are quoted in the inset) for NGC 2298. Right: completeness contours in the radial distance versus mF814W magnitude plane. The completeness levels corresponding to the red and gray continuous lines are quoted in the figure. Dotted lines indicate differences of completeness of 0.05 ranging from 0.05 to 0.95.
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