Analytical Approximations of Long-Exposure Point Spread Functions and their Use
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AbstractThe observed light distribution in long exposure star images (PSF) may be fitted equally well by a variety of models. But dealing with undersainpled star images, only the use of the multi-Gaussian model allows the correct model parameters estimation, taking into account integration on pixel surface, image off-centering and background behaviour. It is also shown that the convolution of a spherical source with the multi-Gaussian and Moffat’s models gives in practice the same result.
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2009 ◽
Vol 223
(1)
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pp. 1-14
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Keyword(s):
2013 ◽
Vol 11
(01)
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pp. 1350009
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