Final detection probability map from NaCo (panel a) and the final reduced image from NEAR observations (panel b) of ϵ Ind A. The predicted position of the companion at the time of observation, along with the 1σ uncertainty in position, as inferred from the best-fit ephemerides, based on RV and astrometry data (Feng et al. 2019), is shown asan ellipse. The NaCo image was reduced using a combination of RSM and modified LOCI subtraction applied at suitable separations while the NEAR image was reduced using the circular profile subtraction technique. No companions were detected in either image.