We have recently begun a program of high resolution infrared imaging at Palomar Observatory. As a part of this effort, we have investigated the use of nonredundant masks both as an imaging technique and as a method of analyzing various aspects of our imaging system. In particular, we have applied the technique to a bright star and binary system using a three-hole mask. We find the method is useful for understanding certain systematic biases in our data, as well as in producing high quality

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... s despite sparse uv coverage. We find that the use of multi-r0 apertures along with a large bandwidth does not significantly hamper image, reconstruction, but provides significant extra coverage in the uv plane.