Fig. 4.
Comparison of star-hopping RDI vs. ADI reductions of IRDIS K1 + K2 band data injected with flat spectrum simulated planets. The inner two simulated planets are not successfully recovered in the ADI reduction, while they are clearly detected in the RDI reductions. The third simulated planet is recovered significantly better in the star-hopping RDI reduction. All real planets are masked out. The color scale is linear with intensity.
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