We propose and simulate an iterative maximum-likelihood image reconstruction method that uses multiple images taken through the turbulent atmosphere under photon-limited conditions. The method assumes that the point-spread function corresponding to each image has been measured by a guide star or other technique. Although a guide star is still required, wave-front correction is achieved through postprocessing instead of by the mechanical methods currently used with adaptive optics. A restored image of greatly increased quality was found to be produced after only 10 iterations. Additional iterations continued to reduce the mean-square error. (C) 1998 Optical Society of America.
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Large Synopt Survey Telescope, Tucson, AZ 85719 USALarge Synopt Survey Telescope, Tucson, AZ 85719 USA
Xin, Bo
Ivezic, Zeljko
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Univ Washington, Dept Astron, Seattle, WA 98195 USALarge Synopt Survey Telescope, Tucson, AZ 85719 USA
Ivezic, Zeljko
Lupton, Robert H.
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Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USALarge Synopt Survey Telescope, Tucson, AZ 85719 USA
Lupton, Robert H.
Peterson, John R.
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Purdue Univ, Dept Phys & Astron, W Lafayette, IN 47907 USALarge Synopt Survey Telescope, Tucson, AZ 85719 USA
Peterson, John R.
Yoachim, Peter
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Univ Washington, Dept Astron, Seattle, WA 98195 USALarge Synopt Survey Telescope, Tucson, AZ 85719 USA
Yoachim, Peter
Jones, R. Lynne
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Univ Washington, Dept Astron, Seattle, WA 98195 USALarge Synopt Survey Telescope, Tucson, AZ 85719 USA
Jones, R. Lynne
Claver, Charles F.
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Large Synopt Survey Telescope, Tucson, AZ 85719 USALarge Synopt Survey Telescope, Tucson, AZ 85719 USA
Claver, Charles F.
Angeli, George
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Large Synopt Survey Telescope, Tucson, AZ 85719 USA
Giant Magellan Telescope Org, Pasadena, CA 91107 USALarge Synopt Survey Telescope, Tucson, AZ 85719 USA