Share Email Print
cover

Proceedings Paper

Enhancing the far-UV sensitivity of silicon CMOS imaging arrays
Format Member Price Non-Member Price
PDF $14.40 $18.00
cover GOOD NEWS! Your organization subscribes to the SPIE Digital Library. You may be able to download this paper for free. Check Access

Paper Abstract

We report our progress toward optimizing backside-illuminated silicon PIN CMOS devices developed by Teledyne Imaging Sensors (TIS) for far-UV planetary science applications. This project was motivated by initial measurements at Southwest Research Institute (SwRI) of the far-UV responsivity of backside-illuminated silicon PIN photodiode test structures described in Bai et al., SPIE, 2008, which revealed a promising QE in the 100-200 nm range as reported in Davis et al., SPIE, 2012. Our effort to advance the capabilities of thinned silicon wafers capitalizes on recent innovations in molecular beam epitaxy (MBE) doping processes. Key achievements to date include: 1) Representative silicon test wafers were fabricated by TIS, and set up for MBE processing at MIT Lincoln Laboratory (LL); 2) Preliminary far-UV detector QE simulation runs were completed to aid MBE layer design; 3) Detector fabrication was completed through the pre-MBE step; and 4) Initial testing of the MBE doping process was performed on monitoring wafers, with detailed quality assessments. Early results suggest that potential challenges in optimizing the UV-sensitivity of silicon PIN type CMOS devices, compared with similar UV enhancement methods established for CCDs, have been mitigated through our newly developed methods. We will discuss the potential advantages of our approach and briefly describe future development steps.

Paper Details

Date Published: 23 July 2014
PDF: 12 pages
Proc. SPIE 9154, High Energy, Optical, and Infrared Detectors for Astronomy VI, 915412 (23 July 2014); doi: 10.1117/12.2054840
Show Author Affiliations
K. D. Retherford, Southwest Research Institute (United States)
Yibin Bai, Teledyne Imaging Sensors (United States)
Kevin K. Ryu, MIT Lincoln Lab. (United States)
J. A. Gregory, MIT Lincoln Lab. (United States)
Paul B. Welander, MIT Lincoln Lab. (United States)
SLAC National Accelerator Lab. (United States)
Michael W. Davis, Southwest Research Institute (United States)
Thomas K. Greathouse, Southwest Research Institute (United States)
Gregory S. Winter, Southwest Research Institute (United States)
Vyshnavi Suntharalingam, MIT Lincoln Lab. (United States)
James W. Beletic, Teledyne Imaging Sensors (United States)


Published in SPIE Proceedings Vol. 9154:
High Energy, Optical, and Infrared Detectors for Astronomy VI
Andrew D. Holland; James Beletic, Editor(s)

© SPIE. Terms of Use
Back to Top