Recovery of simulated planets. Left: an IFS Y–H band reduced image showing simulated planets recovered with high S/N. The source recovered closest to the star indicates a contrast limit of 11.2 mag at 0.1″ projected separation. Right: an IRDIS K1 + K2 band reduced image also showing simulated planets at the same separations, all recovered with high S/N. The same contrast at 0.1″ was reached with IRDIS also. The planets were inserted into the basic calibrated data (flat-fielded, dark-subtracted, and bad pixel corrected) All real planets have been masked out. The color scale is linear with intensity.