DocumentCode :
1712835
Title :
Super-resolved point-spread-function calibration for astronomical imaging
Author :
Hege, E. Keith
Author_Institution :
Steward Obs., Arizona Univ., Tucson, AZ, USA
fYear :
1998
Firstpage :
477
Lastpage :
480
Abstract :
Physically constrained iterative deconvolution attempts to realize the solution of an ill-posed problem, the iterative estimation of both the object function and the corresponding set of image point-spread-functions given a set of noisy realizations of images obtained with less than perfect optical imaging systems. The conditions for achieving super-resolution, defined as recovery of some object spatial frequency components outside the optical passband, have been established by Hunt (see Int. J. Imaging Sys. and Tech. vol.6, p.297-304, 1995) and co-workers Sheppard et al. (see J. Opt. Sec. Am. A, 1998). Here results in astronomical imaging, both with and without adaptive optics correction are shown and the art of using physically constrained iterative deconvolution in astronomical imaging is discussed
Keywords :
adaptive optics; astronomy computing; calibration; deconvolution; image resolution; iterative methods; noise; optical transfer function; parameter estimation; adaptive optics correction; astronomical imaging; ill-posed problem solution; image point-spread-functions; iterative estimation; object function; object spatial frequency components recovery; optical imaging systems; optical passband; physically constrained iterative deconvolution; super-resolved point-spread-function calibration; Adaptive optics; Calibration; Deconvolution; Frequency; Optical devices; Optical imaging; Optical noise; Optimized production technology; Passband; Spatial resolution;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
Time-Frequency and Time-Scale Analysis, 1998. Proceedings of the IEEE-SP International Symposium on
Conference_Location :
Pittsburgh, PA
Print_ISBN :
0-7803-5073-1
Type :
conf
DOI :
10.1109/TFSA.1998.721465
Filename :
721465
Link To Document :
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