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Next Generation of Light Detectors in Astronomy

Published online by Cambridge University Press:  15 February 2011

C. Turon ,
F. Meynadier ,
F. Arenou  and
R. Kohley
R. Kohley*
Affiliation:
European Space Agency, European Space Astronomy Centre (ESAC), PO Box 78, 28691 Villanueva de la Cañada, Madrid, Spain
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Abstract

The paper summarizes the current status of light detectors in astronomy with focus on space science missions. Due to the effort and time needed for the necessary space qualifications, new technologies potentially interesting for space applications are commonly developed and tested for use at on-ground observatories and flown once the technology has matured. But the space environment also requires the development of special detectors for spectral ranges only detectable beyond earth’s atmosphere or the development of features and technological enhancements, for example to mitigate space radiation effects. An overview of detector technologies from the visible to short wavelength infrared (SWIR) band together with an outlook to the challenges of a next generation of light detectors for space astronomy missions.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 45: GAIA: At the Frontiers of Astrometry , 2010 , pp. 73 - 80
Copyright
© EAS, EDP Sciences 2011

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References

Références

Janesick, J., et al., 2010, “High Energy, Optical, and Infrared Detectors for Astronomy IV”, Proc. SPIE, 7742
Finger, G., et al., 2010, “High Energy, Optical, and Infrared Detectors for Astronomy IV”, Proc. SPIE, 7742
Birkmann, S.M., et al., 2010, “Space Telescopes and Instrumentation 2010: Optical, Infrared, and Millimeter Wave”, Proc. SPIE, 7731
Mills, R.E., et al., 2009, “Astronomical and Space Optical Systems”, Proc. SPIE, Vol. 7439.
Gow, J., et al., 2009, “UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XVI”, Proc. SPIE, 7435
Lumb, D.H., et al., 2009, “Astronomical and Space Optical Systems”, Proc. SPIE, 7439
Burt, D., et al., 2009, “Astronomical and Space Optical Systems”, Proc. SPIE, 7439
Dawson, K., et al., 2008, IEEE Trans. Nuc. Sci., 55, 1725 CrossRef
Walker, A., et al., 2008, “Sensors, Systems, and Next-Generation Satellites XII”, Proc. SPIE, 106
Beletic, J.W., et al., 2008, “High Energy, Optical, and Infrared Detectors for Astronomy III”, Proc. SPIE, 7021
Boggs, K., et al., 2007, 27th International Congress on High-Speed Photography and Photonics, Proc. SPIE, 6279
Verhoeve, P., et al., 2004, Proceeding of the 5th International Conference on Space Optics (ICSO 2004), SP-554, 781
Meidinger, N., et al., 2004, “X-Ray and Gamma-Ray Instrumentation for Astronomy XIII” Proc. SPIE, 5165
Marshall, C.J., et al., 2004, “Optical and Infrared Detectors for Astronomy”, Proc. SPIE, 5499
Holland, S.E., et al., 2003, IEEE Trans. Electr. Dev., 50, 225 CrossRef