James Webb Space Telescope Near-Infrared Spectrograph: dark performance of the first flight candidate detector arrays

Details James Webb Space Telescope Near-Infrared Spectrograph: dark performance of the first flight candidate detector arrays James Webb Space Telescope Near-Infrared Spectrograph: dark performance of the first flight candidate detector arrays

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008spie.7021e..63r&link_type=abstract

High Energy, Optical, and Infrared Detectors for Astronomy III. Edited by Dorn, David A.; Holland, Andrew D. Proceedings of

Astronomy and Astrophysics

Astronomy

Scientific paper

The James Webb Space Telescope (JWST) Near Infrared Spectrograph (NIRSpec) incorporates two 5 μm cutoff (λco =5 μm) 2048×2048 pixel Teledyne HgCdTe HAWAII-2RG sensor chip assemblies. These detector arrays, and the two Teledyne SIDECAR application specific integrated circuits that control them, are operated in space at Τ ~ 37 K. This article focuses on the measured performance of the first flight-candidate, and near-flight candidate, detector arrays. These are the first flight-packaged detector arrays that meet NIRSpec's challenging 6 e- rms total noise requirement.

Affiliated with

Also associated with

No associations

Rating

James Webb Space Telescope Near-Infrared Spectrograph: dark performance of the first flight candidate detector arrays does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with James Webb Space Telescope Near-Infrared Spectrograph: dark performance of the first flight candidate detector arrays, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and James Webb Space Telescope Near-Infrared Spectrograph: dark performance of the first flight candidate detector arrays will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1062794