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Expected outcomes of APS developments for astrophysical instrumentation

Published online by Cambridge University Press:  11 June 2009

P. Kern  and
G. Lepage
G. Lepage*
Affiliation:
CMOSIS nv, Belgium
*
[email protected]
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Abstract

CCD technology is preferred for devices used for scientific applications, as CMOS devices were plagued by high dark current, high read noise, etc. Developments in the last 15 years have help circumventing these limitations and CMOS devices could now compete with some of their CCD counterpart.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 37: Astrophysics Detector Workshop 2008 , 2009 , pp. 297 - 300
Copyright
© EAS, EDP Sciences, 2009

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References

Bogaerts, J., Lepage, G., & Dants, D., 2005, In Disruption in space Conf., High-end CMOS Active Pixel Sensors for Space-borne Imaging Instruments
Bogaerts, J., De Munck, K., De Moor, P., et al., 2007, In International image Sensor workshop '07, Radiometric Performance Enhancement of Hybrid and Monolithic Backside Illuminated CMOS APS for Space-borne Imaging
Lepage, G., Dants, D., & Diels, W., 2006, In Proc. Electronic Imaging '06 Conf., CMOS long linear array for space application
Lepage, G., Materne, A., & Renard, C., 2007, In International image Sensor workshop '07, A CMOS image sensor for Earth observation with high efficiency snapshot shutter
Wang, X., Snoeij, M.F., Rao, P.R., Mierop, A., & Theuwissen, A.J.P., 2008, In ISSCC'08, A CMOS Image Sensor with a Buried-Channel Source Follower