Translator Disclaimer
Paper
24 July 2008 Performance of the JWST/MIRI Si:As detectors
Author Affiliations +
Abstract
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.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Michael E. Ressler, Hyung Cho, Richard A. M. Lee, Kalyani G. Sukhatme, John J. Drab, George Domingo, Mark E. McKelvey, Robert E. McMurray Jr., and Jessie L. Dotson "Performance of the JWST/MIRI Si:As detectors", Proc. SPIE 7021, High Energy, Optical, and Infrared Detectors for Astronomy III, 70210O (24 July 2008); https://doi.org/10.1117/12.789606
PROCEEDINGS
12 PAGES


SHARE
Advertisement
Advertisement
RELATED CONTENT

NICMOS3 detector testing: methods and results
Proceedings of SPIE (October 20 1993)
128x128 InGaAs detector array for 1.0-1.7 um
Proceedings of SPIE (November 01 1990)
1024 x 1024 Si As IBC detector arrays for mid...
Proceedings of SPIE (June 15 2006)
Short Wavelength Infrared Hybrid Focal Plane Arrays
Proceedings of SPIE (November 30 1983)
Operation and performance of new NIR detectors from SELEX
Proceedings of SPIE (September 25 2012)
Characterization of VISTA IR detectors
Proceedings of SPIE (September 29 2004)

Back to Top