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Proceedings Paper

Two-Dimensional Infrared Astronomical Speckle Interferometry
Author(s): Julian C. Christou; Jacques M. Beckers; Jonathan D Freeman; Stephen T Ridgway; Ronald G. Probst
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Paper Abstract

The infrared imager currently in use at the National Optical Astronomy Observatories (NOAO) has been adapted for use as a two-dimensional infrared speckle camera operating at wavelengths of 1μm 5μm. Data have been obtained at the Kitt Peak National Observatory (KPNO) Mayall telescope (effective aperture ti 3.8m) for a number of different sources. Diffraction-limited images are presented for two objects, the "Red Rectangle" and NML Cygnus, using the Knox-Thompson algorithm to recover the Fourier phases. A comparison of phase-relaxation techniques applied to the integrated phase differences is presented using both the Hudgin method and successive over-relaxation.

Paper Details

Date Published: 2 December 1988
PDF: 10 pages
Proc. SPIE 0976, Statistical Optics, (2 December 1988); doi: 10.1117/12.948546
Show Author Affiliations
Julian C. Christou, National Optical Astronomy Observatories (United States)
Jacques M. Beckers, European Southern Observatory (Germany)
Jonathan D Freeman, University of Arizona (United States)
Stephen T Ridgway, National Optical Astronomy Observatories (United States)
Ronald G. Probst, National Optical Astronomy Observatories (United States)


Published in SPIE Proceedings Vol. 0976:
Statistical Optics
G. Michael Morris, Editor(s)

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