OMP reconstructions with the pixel basis of the object a), radio emission from 3C75, simulated with measurements from a URA in b) (RE = 1.69 × 10-4), an NRA of SD = 0.14 in c) (RE = 0.763), an NRA of SD = 0.18 in d) (RE = 0.0150), the VLA-based “Y” array in e) (RE = 0.179), and the YOPP array in f) (RE = 0.0187). All pixel brightness values in the object and reconstructions are normalized by the object’s maximum pixel brightness value, to lie on [0, 1]. Image a) can be found at http://images.nrao.edu/29 (courtesy of NRAO/AUI and F.N. Owen, C.P. O’Dea, M. Inoue, and J. Eilek). Original versions of a)–c), e), and f) appeared in Fannjiang (2011).
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