Synthetic aperture imaging at infrared wavelengths

Details Synthetic aperture imaging at infrared wavelengths Synthetic aperture imaging at infrared wavelengths

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.241p..51h&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 241, Nov. 15, 1989, p. 51P-56P. Research supported by S

Astronomy and Astrophysics

Astronomy

10

Binary Stars, Infrared Imagery, Radio Astronomy, Data Reduction, Image Reconstruction, Speckle Interferometry, Synthetic Arrays, Telescopes

Scientific paper

Observations of Eta Oph and Gamma CrB at a wavelength of 2.2 microns indicate that diffraction-limited images of high dynamic range are routinely attainable with ground-based telescopes. A simple modification of the telescope pupil permits the use of existing radio-astronomical imaging algorithms, while maintaining many of the advantages of an unapodized primary mirror.

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