Bayesian deconvolution in optical astronomy

Details Bayesian deconvolution in optical astronomy Bayesian deconvolution in optical astronomy

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aj....103..666m&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 103, Feb. 1992, p. 666-675, 689. Research supported by British Council, SERC, DGICYT

Astronomy and Astrophysics

Astronomy

8

Bayes Theorem, Image Processing, Optical Correction Procedure, Seeing (Astronomy), Convolution Integrals, Electromagnetic Noise, Stochastic Processes

Scientific paper

Bayesian methods and spatial stochastic processes are used here in the deconvolution of images of galaxies. Under very simple but realistic prior assumptions about the true underlying image of a galaxy the Bayesian framework is put to work. The method is tested in CCD images of extragalactic objects of different morphological types and an analysis of the deconvolutions obtained is performed emphasizing the comparison with other observational results.

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