Paper
13 October 1986 Diffraction-Limited 10 µm Imaging With 3 Meter Telescopes
E. E. Bloemhof, C. H. Townes, A. H. B. Vanderwyck
Author Affiliations +
Abstract
We have constructed an infrared imaging system that achieves diffraction-limited spatial resolution (about 0.8 arc seconds) at 10 um on 3 meter ground-based telescopes. The system uses a linear array of sensitive HgCdTe photodiodes, scanned in the direction perpendicular to the array axis, to form two-dimensional images. Scans are completed rapidly enough to freeze atmospheric fluctuations. Individual detectors are small compared to the diameter of the Airy disk, and images are oversampled heavily in the scan direction. This method has a number of advantages for studying small fields with very high spatial resolution, and has been applied successfully to the problem of directly imaging faint circumstellar dust shells.
© (1986) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
E. E. Bloemhof, C. H. Townes, and A. H. B. Vanderwyck "Diffraction-Limited 10 µm Imaging With 3 Meter Telescopes", Proc. SPIE 0627, Instrumentation in Astronomy VI, (13 October 1986); https://doi.org/10.1117/12.968125
Lens.org Logo
CITATIONS
Cited by 7 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Telescopes

Spatial resolution

Stars

Sensors

Diffraction

Astronomy

Mirrors

RELATED CONTENT

WIYN tip-tilt module performance
Proceedings of SPIE (February 04 2003)
All-sky 10-um cloud monitor on Mauna Kea
Proceedings of SPIE (February 04 2003)
NASA 3-Meter Infrared Telescope Facility at Mauna Kea
Proceedings of SPIE (April 03 1981)

Back to Top