Bibcode
Feautrier, Philippe; Gach, Jean-Luc; Balard, Philippe; Guillaume, Christian; Downing, Mark; Stadler, Eric; Magnard, Yves; Denney, Sandy; Suske, Wolfgang; Jorden, Paul; Wheeler, Patrick; Skegg, Michael; Pool, Peter; Bell, Ray; Burt, David; Reyes, Javier; Meyer, Manfred; Hubin, Norbert; Baade, Dietrich; Kasper, Markus; Arsenault, Robin; Fusco, Thierry; Diaz Garcia, Jose Javier
Bibliographical reference
High Energy, Optical, and Infrared Detectors for Astronomy III. Edited by Dorn, David A.; Holland, Andrew D. Proceedings of the SPIE, Volume 7021, pp. 70210C-70210C-12 (2008).
Advertised on:
8
2008
Citations
0
Refereed citations
0
Description
ESO and JRA2 OPTICON have jointly funded e2v technologies to develop a
custom CCD for Adaptive Optic Wave Front Sensor (AO WFS) applications.
The device, called CCD220, is a compact Peltier-cooled 240×240
pixel frametransfer 8-output back-illuminated sensor. Using the
electron-multiplying technology of L3Vision detectors, the device is
designed to achieve sub-electron read noise at frame rates from 25 Hz to
1,500 Hz and dark current lower than 0.01 e-/pixel/frame. The
development has many unique features. To obtain high frame rates,
multiple EMCCD gain registers and metal buttressing of row clock lines
are used. The baseline device is built in standard silicon. In addition,
two speculative variants have been built; deep depletion silicon devices
to improve red response and devices with an electronic shutter to extend
use to Rayleigh and Pulsed Laser Guide Star applications. These are all
firsts for L3Vision CCDs. These CCD220 detectors have now been
fabricated by e2v technologies. This paper describes the design of the
device, technology trade-offs, and progress to date. A Test Camera,
called "OCam", has been specially designed and built for these sensors.
Main features of the OCam camera are extensively described in this
paper, together with first light images obtained with the CCD220.