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Development of low dark current SiGe-detector arrays for visible-NIR imaging sensor

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sword-2019-05-31T13:16:09.original.xml (130 B)
Original SWORD entry document
Author(s)
Sood, Ashok K.
•
Richwine, Robert A.
•
Puri, Yash R.
•
DiLello, Nicole Ann
•
Hoyt, Judy L.
•
Akinwande, Tayo I.
•
Dhar, Nibir
•
Horn, Stuart
•
Balcerak, Raymond S.
•
Bramhall, Thomas G.
Date Issued
April 23, 2010
Publisher
SPIE
Citation
Sood, Ashok K., Richwine, Robert A., Puri, Yash R., DiLello, Nicole, Hoyt, Judy L. et al. 2010. "Development of low dark current SiGe-detector arrays for visible-NIR imaging sensor."
Version
Final published version
Abstract
SiGe based focal plane arrays offer a low cost alternative for developing visible- near-infrared focal plane arrays that will cover the spectral band from 0.4 to 1.6 microns. The attractive features of SiGe based foal plane arrays take advantage of silicon based technology that promises small feature size, low dark current and compatibility with the low power silicon CMOS circuits for signal processing. This paper will discuss performance characteristics for the SiGe based VIS-NIR Sensors for a variety of defense and commercial applications using small unit cell size and compare performance with InGaAs, InSb, and HgCdTe IRFPA's. We will present results on the approach and device design for reducing the dark current in SiGe detector arrays. We will discuss electrical and optical properties of SiGe arrays at room temperature and as a function of temperature. We will also discuss future integration path for SiGe devices with Si-MEMS Bolometers. © 2010 Copyright SPIE - The International Society for Optical Engineering.
MIT Department
Massachusetts Institute of Technology. Microsystems Technology Laboratories
Terms of Use
Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Persistent DSpace Link
https://hdl.handle.net/1721.1/137641.2
DOI of Published Version
https://doi.org/10.1117/12.852682
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