A model for data acquired with the use of a charge-coupled-device camera is given and is then used for developing a new iterative method for restoring intensities of objects observed with such a camera. The model includes the effects of point spread, photoconversion noise, readout noise, nonuniform flat-field response, nonuniform spectral response, and extraneous charge carriers resulting from bias, dark current, and both internal and external background radiation. An iterative algorithm is identified that produces a sequence of estimates converging toward a constrained maximum-likelihood estimate of the intensity distribution of an imaged object. An example is given for restoring images from data acquired with the use of the Hubble Space Telescope.
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Univ of California, Santa Cruz, CA,, USA, Univ of California, Santa Cruz, CA, USAUniv of California, Santa Cruz, CA,, USA, Univ of California, Santa Cruz, CA, USA
Robinson, L.B.
Stover, R.J.
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Univ of California, Santa Cruz, CA,, USA, Univ of California, Santa Cruz, CA, USAUniv of California, Santa Cruz, CA,, USA, Univ of California, Santa Cruz, CA, USA
Stover, R.J.
Osborne, J.
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Univ of California, Santa Cruz, CA,, USA, Univ of California, Santa Cruz, CA, USAUniv of California, Santa Cruz, CA,, USA, Univ of California, Santa Cruz, CA, USA
Osborne, J.
Miller, J.S.
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Univ of California, Santa Cruz, CA,, USA, Univ of California, Santa Cruz, CA, USAUniv of California, Santa Cruz, CA,, USA, Univ of California, Santa Cruz, CA, USA
Miller, J.S.
Vogt, S.S.
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Univ of California, Santa Cruz, CA,, USA, Univ of California, Santa Cruz, CA, USAUniv of California, Santa Cruz, CA,, USA, Univ of California, Santa Cruz, CA, USA
Vogt, S.S.
Allen, S.L.
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Univ of California, Santa Cruz, CA,, USA, Univ of California, Santa Cruz, CA, USAUniv of California, Santa Cruz, CA,, USA, Univ of California, Santa Cruz, CA, USA