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It is important to determine very precisely the aberrations of the Hubble Space Telescope (HST) in order to (1) design correction optics to be included in replacement instruments, (2) align the secondary mirror of the HST’s Optical Telescope Assembly (OTA) and (3) form an analytic model of the system point-spread function (PSF) that can be used for image deblurring until the telescope is repaired.
© 1991 Optical Society of America
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