Paper
12 September 2007 NIRCam thermal subsystem
Author Affiliations +
Abstract
The Near Infrared Camera (NIRCam) instrument for NASA's James Webb Space Telescope (JWST) is one of the four science instruments to be installed into the Integrated Science Instrument Module (ISIM) on JWST. NIRCam's requirements include operation at 37 Kelvin to produce high resolution images in two wave bands encompassing the range from 0.6 microns to 5 microns. In addition, NIRCam is to be used as a metrology instrument during the JWST observatory commissioning on orbit, during the precise alignment of the observatory's multiple-segment primary mirror. This paper will provide an update to the NIRCam Thermal subsystem design for stable operation at 37 Kelvin.
© (2007) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Liz Osborne "NIRCam thermal subsystem", Proc. SPIE 6692, Cryogenic Optical Systems and Instruments XII, 66920J (12 September 2007); https://doi.org/10.1117/12.742097
Lens.org Logo
CITATIONS
Cited by 1 scholarly publication.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
James Webb Space Telescope

Sensors

Calibration

Staring arrays

Mirrors

Cameras

Observatories

RELATED CONTENT

NIRCam thermal subsystem
Proceedings of SPIE (August 25 2005)
NIRCam instrument overview
Proceedings of SPIE (August 25 2005)
NIRSpec: near-infrared spectrograph for the JWST
Proceedings of SPIE (October 12 2004)
Straylight considerations for NIR spectrographs
Proceedings of SPIE (July 09 2008)
Status of the NIRSpec instrument
Proceedings of SPIE (August 04 2010)

Back to Top