Paper
20 October 1993 MIRAC: a mid-infrared array camera for astronomy
William F. Hoffmann, Giovanni G. Fazio, Kandiah Shivanandan, Joseph L. Hora, Lynne K. Deutsch
Author Affiliations +
Abstract
MIRAC is a Mid InfraRed Array Camera built for ground-based astronomy by Steward Observatory at the University of Arizona, Harvard Smithsonian Center for Astrophysics, and the Center for Advanced Space Sensing at the Naval Research Laboratory. It utilizes a Hughes Aircraft Co. 20 X 64 pixel arsenic-doped silicon impurity band conduction hybrid array with a capacitance transimpedance amplifier readout (CRC 444A) operating at 10 K in a liquid helium-cooled cryostat. It has an operating wavelength range of 2 to 26 micrometers . Using 20 parallel readout lines and frame rate of 10 KHz, the array exhibits both low noise and good linearity at high background flux, which is essential for 10 and 20 micrometers ground-based observing conditions. It has a peak quantum efficiency of 0.42 at 22 micrometers , and a well size of 120,000 electrons. MIRAC has been operated on the Steward Observatory 2.3-meter and NASA 3-meter IRTF telescopes a number of times for observing a variety of objects including infrared-luminous galaxies, planetary nebulae, star forming regions, and young stellar objects. The NEFD of MIRAC on the IRTF at 11.7 micrometers is 0.1 Jy/square-arcsec in one second of integration on-source, four seconds total time, including nodding and chopping off-source.
© (1993) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
William F. Hoffmann, Giovanni G. Fazio, Kandiah Shivanandan, Joseph L. Hora, and Lynne K. Deutsch "MIRAC: a mid-infrared array camera for astronomy", Proc. SPIE 1946, Infrared Detectors and Instrumentation, (20 October 1993); https://doi.org/10.1117/12.158697
Lens.org Logo
CITATIONS
Cited by 24 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Sensors

Signal processing

Telescopes

Cameras

Optical filters

Space telescopes

Digital signal processing

RELATED CONTENT

Infrared Camera For 10 p m Astronomy
Proceedings of SPIE (July 27 1981)
NASA IRTF tip-tilt secondary system
Proceedings of SPIE (September 18 1997)
FLITECAM a near infrared camera for test and science...
Proceedings of SPIE (June 20 2000)
CATAVIÑA: new infrared camera for OAN-SPM
Proceedings of SPIE (June 15 2006)
Long-wavelength infrared camera for the Keck Telescope
Proceedings of SPIE (July 01 1990)
TIMMI a 10 um camera for the ESO 3.6...
Proceedings of SPIE (October 20 1993)

Back to Top