Paper
19 February 2004 CCDs for the rotational velocity spectrometer on GAIA
Andrew D. Holland, Mark S. Cropper, David Katz, Ian B. Hutchinson, Richard M. Ambrosi, Tim J. Stevenson, David Ryan Smith, Dave Walton, D. Burt, Peter J. Pool, David G. Morris, Torgeir Paulsen
Author Affiliations +
Abstract
The ESA cornerstone mission GAIA will perform astrometric, photometric and spectroscopic measurements and is due for launch in 2010 into L2 orbit. The astrometric telescope system will catalogue the position of over 109 objects down to 20th magnitude and perform broadband photometry. The spectroscopic telescope will provide narrow-band photometry and feed a Radial Velocity Spectrometer which will accurately determine the radial velocities of objects down to 17-18 magnitude. This paper discusses the characteristics of the detectors envisaged for the focal plane of the RVS instrument.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Andrew D. Holland, Mark S. Cropper, David Katz, Ian B. Hutchinson, Richard M. Ambrosi, Tim J. Stevenson, David Ryan Smith, Dave Walton, D. Burt, Peter J. Pool, David G. Morris, and Torgeir Paulsen "CCDs for the rotational velocity spectrometer on GAIA", Proc. SPIE 5251, Detectors and Associated Signal Processing, (19 February 2004); https://doi.org/10.1117/12.517151
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Cited by 4 scholarly publications.
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KEYWORDS
Charge-coupled devices

Sensors

Spectroscopy

Stars

Telescopes

Space telescopes

Silicon

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