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Fig. 4.


Top 8 panels: resulting WB (bottom 4 panels) and CRISP NB (top 4 panels) images after adding up the 74 observed images during 2 s and only compensating for relative image motion (tip and tilt) between the individual exposures and the PSF of the diffraction limited telescope. Bottom 8 panels: resulting image of the same observed images but after applying MFBD image reconstruction to compensate for the largest 100 KL modes. The wavelengths are (left to right) 525 nm, 557 nm, 630 nm, and 853 nm.

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