Paper
20 October 1993 University of California/San Diego's mid-IR astronomical array camera
Robert K. Pina, Barbara Jones, Richard Charles Puetter
Author Affiliations +
Abstract
We have implemented an infrared array camera for high-background, ground-based astronomical imaging in the mid-infrared spectral region from 5 to 27 microns. The camera is built around a 20 X 64 element Si:As Impurity Band Conduction (IBC) device manufactured by GenCorp Aerojet Electronic Systems Division. Observations with the camera on a 1.5 meter telescope (Mt. Lemmon Observing Facility, Tucson, Arizona) yield a noise- equivalent flux density (NEFD) of 23.5 mJy min-1/2 arcsec-2 at (lambda) equals 10 micrometers , (Delta) (lambda) equals 1 micrometers , and a readout frame rate of 366 Hz. We discuss the design and implementation of the camera and operational procedures for observation in a high-background environment (e.g. background subtraction and flat-fielding). We also present sample images obtained with our camera.
© (1993) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Robert K. Pina, Barbara Jones, and Richard Charles Puetter "University of California/San Diego's mid-IR astronomical array camera", Proc. SPIE 1946, Infrared Detectors and Instrumentation, (20 October 1993); https://doi.org/10.1117/12.158719
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Digital signal processing

Telescopes

Cameras

Sensors

Data acquisition

Mirrors

Infrared detectors

RELATED CONTENT

Active THz imaging system with improved frame rate
Proceedings of SPIE (April 30 2009)
Development of the HAWC far-infrared camera for SOFIA
Proceedings of SPIE (September 30 2004)
FORCAST a facility 5 to 40 um camera...
Proceedings of SPIE (June 20 2000)
MIRAC: a mid-infrared array camera for astronomy
Proceedings of SPIE (October 20 1993)

Back to Top