Paper
12 January 2004 Development of the CCDs for ESA GAIA cornerstone mission
Andrew D. Holland, Michael A.C. Perryman, Cyril Vetel, Roy Steward, Ian B. Hutchinson, Richard M. Ambrosi, David Ryan Smith, Steve Bowring, David J. Burt, Tim Eaton, David G. Morris, Peter Poole, Robert Davancens, Anouk Laborie, Pierre Pouny, Frederic Safa, Igor Zayer, Alexander D.T. Short
Author Affiliations +
Abstract
The ESA cornerstone mission GAIA will perform astrometric and photometric measurements on one billion objects, and is due for launch in 2010 into L2 orbit. The key astrometric focal plane will comprise over 180 large area CCDs with a focal surface of about 0.5m2. The 45x60mm2 CCDs for the focal plane will include technical features new to CCDs. This paper will discuss the characteristics of these devices, including the measures to improve the radiation hardness of the technology.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Andrew D. Holland, Michael A.C. Perryman, Cyril Vetel, Roy Steward, Ian B. Hutchinson, Richard M. Ambrosi, David Ryan Smith, Steve Bowring, David J. Burt, Tim Eaton, David G. Morris, Peter Poole, Robert Davancens, Anouk Laborie, Pierre Pouny, Frederic Safa, Igor Zayer, and Alexander D.T. Short "Development of the CCDs for ESA GAIA cornerstone mission", Proc. SPIE 5167, Focal Plane Arrays for Space Telescopes, (12 January 2004); https://doi.org/10.1117/12.515401
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KEYWORDS
Charge-coupled devices

Sensors

Telescopes

Atrial fibrillation

Space telescopes

Staring arrays

Stars

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