Simulations show that iterative source removal and maximum likelihood decoding can recover point-source positions and fluxes from 1.5D coded-aperture data with 5-arcmin resolution in one axis and 5-degree resolution in the other.
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Simulations of a 2 x 1.5D coded aperture camera for X-ray astronomy
Simulations show that iterative source removal and maximum likelihood decoding can recover point-source positions and fluxes from 1.5D coded-aperture data with 5-arcmin resolution in one axis and 5-degree resolution in the other.