Paper
20 October 1993 Ohio State Infrared Imager/Spectrometer (OSIRIS)
Author Affiliations +
Abstract
The Ohio State Infrared Imager/Spectrometer (OSIRIS) is a general purpose near infrared (0.9 to 2.5 micrometers ) instrument that can be used at a wide variety of telescope focal planes. OSIRIS currently uses a 256 X 256 HgCdTe array detector and will accommodate larger arrays when available. OSIRIS has two modes of operation: imaging and spectroscopic. This paper describes the general instrument design and sample scientific results.
© (1993) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Darren L. DePoy, Bruce Atwood, Paul Laurence Byard, J. Frogel, and Thomas P. O'Brien "Ohio State Infrared Imager/Spectrometer (OSIRIS)", Proc. SPIE 1946, Infrared Detectors and Instrumentation, (20 October 1993); https://doi.org/10.1117/12.158725
Lens.org Logo
CITATIONS
Cited by 52 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Sensors

Electronics

Cameras

Telescopes

Infrared imaging

Infrared radiation

Spectroscopes

RELATED CONTENT

SWIR at the Nordic Optical Telescope: NOTCam
Proceedings of SPIE (August 16 2000)
IR instrumentation for the ESO VLT
Proceedings of SPIE (October 20 1993)
MAGIC: a new near-infrared camera for Calar Alto
Proceedings of SPIE (October 20 1993)
System Design Of A 1 5 µm IR Camera For...
Proceedings of SPIE (October 13 1986)

Back to Top