Conclusions

As a result of our explorations, we can set forth several points in conclusion.

• The convolution network has proven to be a robust method for determination of an effective solution to a class of Fredholm integral equations of the first kind.

• The convolution network was originally developed to search for an efficient, data independent method of image reconstruction of Hubble Space Telescope imagery. This has proven to be highly satisfactory and work is continuing.

• The convolution network has proven successful in resolution enhancement of many imaging systems.

• The convolution network can successfully be applied for the processing of sinc apodized spectra to obtain a positive semi-definite representation of the spectra. This provides a means for obtaining a baseline for the sinc apodized spectra.