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In less than a year, the James Webb Space Telescope (JWST) will inherit themantle of being the world's pre-eminent infrared observatory. JWST will carrywith it an Aperture Masking Interferometer (AMI) as one of the supportedoperational modes of the Near-InfraRed Imager and Slitless Spectrograph(NIRISS) instrument. Aboard such a powerful platform, the AMI mode will deliverthe most advanced and scientifically capable interferometer ever launched intospace, exceeding anything that has gone before it by orders of magnitude insensitivity. Here we present key aspects of the design and commissioning ofthis facility: data simulations ($\texttt{ami_sim}$), the extraction ofinterferometeric observables using two different approaches($\texttt{IMPLANEIA}$ and $\texttt{AMICAL}$), an updated view of AMI's expectedperformance, and our reference star vetting programs.

The James Webb Space Telescope Aperture Masking Interferometer