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Fig. 14.


Detection completeness as a function of the brightness of the impact flashes in the R-band. For each magnitude bin of 0.2 mag in the R-band 50 mock flashes were placed in random positions throughout a real observation of the Moon (in both the R- and I-band images) with a color index of R-I=1 mag. The completeness is then computed by forming the ratio of the ones detected with S/N above 2.5 (σmag <  0.4), in both R- and I-bands, to the total number created (50).

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