Paper
24 July 2008 Performance of the JWST/MIRI Si:As detectors
Michael E. Ressler, Hyung Cho, Richard A. M. Lee, Kalyani G. Sukhatme, John J. Drab, George Domingo, Mark E. McKelvey, Robert E. McMurray Jr., Jessie L. Dotson
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
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Cited by 20 scholarly publications.
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KEYWORDS
Sensors

Quantum efficiency

Spectroscopy

James Webb Space Telescope

Black bodies

Detector arrays

Imaging systems

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