Abstract
A technique for reconstructing diffraction-limited image of an object from speckle images without reference star is applied to both simulated and real data. The object spectrum is estimated by blind deconvolution using the power spectrum of the speckle images and the phase is restored from the bispectrum.
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© 1994 Springer Science+Business Media Dordrecht
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Thiebaut, E. (1994). Speckle Imaging With the Bispectrum and Without Reference Star. In: Robertson, J.G., Tango, W.J. (eds) Very High Angular Resolution Imaging. International Astronomical Union / Union Astronomique Internationale, vol 158. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0880-5_35
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DOI: https://doi.org/10.1007/978-94-011-0880-5_35
Publisher Name: Springer, Dordrecht
Print ISBN: 978-0-7923-2633-5
Online ISBN: 978-94-011-0880-5
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