Performance of the JWST/MIRI Si:As detectors

Details Performance of the JWST/MIRI Si:As detectors Performance of the JWST/MIRI Si:As detectors

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008spie.7021e..19r&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 Mid-Infrared Instrument (MIRI) is a 5 to 28 micron imager and spectrometer that is slated to fly aboard the JWST in 2013. Each of the flight arrays is a 1024×1024 pixel Si:As impurity band conductor detector array, developed by Raytheon Vision Systems. JPL, in conjunction with the MIRI science team, has selected the three flight arrays along with their spares. We briefly summarize the development of these devices, then describe the measured performance of the flight arrays along with supplemental data from sister flight-like parts.

Affiliated with

Also associated with

No associations

Rating

Performance of the JWST/MIRI Si:As detectors 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 Performance of the JWST/MIRI Si:As detectors, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Performance of the JWST/MIRI Si:As detectors will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1061862