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The Use of Bayesian Statistics in Image Estimation from Interferometer Data

Published online by Cambridge University Press:  12 April 2016

T. J. Cornwell
T. J. Cornwell*
Affiliation:
Nuffield Radio Astronomy Laboratories, Jodrell Bank, Macclesfield, Cheshire

Extract

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The problem of estimating radio sky brightness distributions from incomplete, and noisy, visibility measurements, such as those collected by a long baseline interferometer, has recently been attacked using nonlinear data-adaptive techniques such as the Maximum Entropy method (Abies (1974), Wernecke (1976), Wernecke and D’Addario (1977), Gull and Daniell (1978)) and the Maximum Likelihood method (Papadopoulos (1975)).

Type
Part V: Maximum Entropy Image Reconstruction
Information
International Astronomical Union Colloquium , Volume 49: Image Formation from Coherence Functions in Astronomy , 1979 , pp. 227 - 234
Copyright
Copyright © Reidel 1979

References

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