“…The second class of telescopes utilizes the spatial multiplexing that can be obtained either from using pairs of widely separated collimator grids to form modulation patterns of the incident v-rays onto a position sensitive detector (PSD), or with one or more arrays of transparent and opaque elements, whose shadow projected along the flux direction is intercepted by a PSD. In the first case we refer to Fourier-transform imagers (Chou and Barrett, 1978;Palmer and Prince, 1987), while the multiplexing instruments of the second kind are known as 'coded mask systems', and have already been used successfully in several other fields: for monitoring confinement fusion experiments Yamanaka et al, 1984), in nuclear medicine, particularly in tomography (Cannon and Knoll et aL, 1984, Ohyama et al, 1984, in chemical spectroscopy (Harwit et aL, 1974;Plankey et al, 1974) and in optical image processing (Oliver, 1976).…”