Paper
20 October 1993 Optical design of an achromatic re-imaging lens system for a cryogenic near-infrared astronomical camera
Author Affiliations +
Abstract
This paper describes an infrared imaging system developed to match the physical pixel sizes of the near infrared arrays used in the UCLA IR camera to the typical seeing disk at the f/15 focus of the W. M. Keck telescope. A field of view of 64 arcseconds (') at 0.25' per pixel is required, no internal focussing mechanism is possible and the system must perform under vacuum at 77 K. In our design, an achromatic triplet lens of calcium and barium fluoride provides an image of the entrance pupil and collimates the beam before it passes through a dichroic beam-splitter which divides the system into two independent channels; the wavelength split occurs at approximately 2.5 micrometers . Each beam is re-imaged onto IR arrays with 30 and 40 micrometers pixels to yield 0.25'/pixel and each imager is independently optimized to be achromatic and aberration free. Spot diagrams and aberration plots will be given. We also describe the steps required to compensate for environmental changes, since these lenses are used at LN2 temperature, and we discuss AR coatings and throughput.
© (1993) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Suzanne Casement, Ian S. McLean, and Robert E. Fischer "Optical design of an achromatic re-imaging lens system for a cryogenic near-infrared astronomical camera", Proc. SPIE 1946, Infrared Detectors and Instrumentation, (20 October 1993); https://doi.org/10.1117/12.158708
Lens.org Logo
CITATIONS
Cited by 2 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Imaging systems

Telescopes

Collimators

Cameras

Infrared detectors

Optical filters

Sensors

RELATED CONTENT

Optical design of COATLI an all sky robotic optical...
Proceedings of SPIE (August 09 2016)
Status of the EMIR optical system
Proceedings of SPIE (March 07 2003)
Optical design of MOIRCS
Proceedings of SPIE (March 07 2003)

Back to Top