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An analytical approximation of the hubble space telescope monochromatic point spread functions
A mixture of off-center Gaussians is used to approximate the predicted monochromatic point spread functions (PSFs) of Hubble Space Telescope (HST) at long wavelengths, and also, with a reduced number of parameters, the wide-band PSFs. The usefulness of the approximation in simulation and analysis of...
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Published in: | Journal of astrophysics and astronomy 1987-12, Vol.8 (4), p.343-350 |
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Main Authors: | , , |
Format: | Article |
Language: | English |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | A mixture of off-center Gaussians is used to approximate the predicted monochromatic point spread functions (PSFs) of Hubble Space Telescope (HST) at long wavelengths, and also, with a reduced number of parameters, the wide-band PSFs. The usefulness of the approximation in simulation and analysis of HST data is shown by means of application to image centering and convolution-deconvolution problems. (Author) |
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ISSN: | 0250-6335 0973-7758 |
DOI: | 10.1007/BF02714898 |