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Fig. 2

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Photometric errors derived from the artificial star tests. The panels show the difference between output and input magnitudes as a function of the output magnitude (left panels: F814W-band; right panels: F606W-band). The vertical gray line indicates the magnitude corresponding to the 50% completeness factors, while the gray error bars show the mean magnitude difference as a function of the output magnitude.

This figure is made of several images, please see below:

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