Paper
29 January 1988 Diffraction-Limited Imaging With The Coherently Cophased Mmt
E. Keith Hege, Donald W. McCarthy Jr., J. C. Hebden, Stuart B. Shaklan, Julian C. Christou
Author Affiliations +
Abstract
The 6.86 m Multiple Mirror Telescope (MMT) has been operated as a coherently cophased interferometric imaging array since 1983. PSF observations at wavelengths from 410 to 850 nm reveal characteristics which must be controlled to achieve reliable imaging at resolutions less than 75 nanoradians (0.015 arc seconds). The MMT has been used to acquire differential speckle images of Alpha Orionis in the H-alpha line and a nearby "continuum" bandpass at 656.9 nm. Broadband images of a 12th magnitude geosynchronous communications satellite, from which shape and size measures have been obtained with 100 nm resolution, give evidence of the capability of the MMT in speckle imaging applications. We have recently extended the cophasing capability to infrared wavelengths by providing reflective pathlength compensation capability.
© (1988) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
E. Keith Hege, Donald W. McCarthy Jr., J. C. Hebden, Stuart B. Shaklan, and Julian C. Christou "Diffraction-Limited Imaging With The Coherently Cophased Mmt", Proc. SPIE 0828, Digital Image Recovery and Synthesis, (29 January 1988); https://doi.org/10.1117/12.942074
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KEYWORDS
Telescopes

Speckle

Calibration

Point spread functions

Mirrors

Image restoration

Interferometry

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