Deconvolution in Optical Astronomy. A Bayesian Approach

  • R. Molina
  • B. D. Ripley
Part of the Lecture Notes in Statistics book series (LNS, volume 74)


We describe in this work how the Bayesian paradigm can be applied to a deconvolution problem in optical astronomy. The use of robust statistics in this process is also discussed.


Prior Distribution Point Spread Function Globular Cluster Atmospheric Motion Deconvolved Image 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


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Copyright information

© Springer-Verlag Berlin Heidelberg 1992

Authors and Affiliations

  • R. Molina
    • 1
  • B. D. Ripley
    • 2
  1. 1.Departamento de Ciencias de la Computación e I.A.Universidad de GranadaGranada, EspañaSpain
  2. 2.Department of StatisticsUniversity of OxfordOxfordUK

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