Paper
2 December 1988 Two-Dimensional Infrared Astronomical Speckle Interferometry
Julian C. Christou, Jacques M. Beckers, Jonathan D Freeman, Stephen T Ridgway, Ronald G. Probst
Author Affiliations +
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.
© (1988) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Julian C. Christou, Jacques M. Beckers, Jonathan D Freeman, Stephen T Ridgway, and Ronald G. Probst "Two-Dimensional Infrared Astronomical Speckle Interferometry", Proc. SPIE 0976, Statistical Optics, (2 December 1988); https://doi.org/10.1117/12.948546
Lens.org Logo
CITATIONS
Cited by 2 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Speckle

Spatial frequencies

Infrared cameras

Phase measurement

Cameras

Statistical optics

Signal to noise ratio

Back to Top