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Aperture Masking Interferometry used in combination with Adaptive Optics, isa powerful technique that permits the detection of faint companions at smallangular separations. The precision calibration of the data achieved with thisobserving mode indeed leads to reliable results up to and beyond the formaldiffraction limit, explaining why it has, in just a few years, been ported onmost major telescopes. In this poster, we present its possible implementationon Subaru. We also discuss how the opportunity offered by the plannedExtreme-AO upgrade to HiCIAO will push further the performance of this alreadysuccessful technique, offering Subaru a unique access to a very exciting regionof the "contrast-ratio - angular separation" parameter space.

Aperture Masking Interferometry for Subaru