By John van Duynhoven, Peter S Belton, G A Webb, Henk van As
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Pool et al. lnallOn 1 a x 512 );;=1 -"'1\- ! Photomask / ft _ _ ... -- ~ ---... -. a. --- ~ ---( -- -- -/ 112 N N CCD42 Wafer Layout I It x 512 ...... --_- -\ ---- J ~ -... -~ / a. It au: ...... "',' 2111: I( '"2 .. Figure 1 Figure 2 :0/ 2. READ-OUT REGISTER In both series of devices separate charge detection circuits are incorporated at each end of the read-out register, which is split such that a line of charges can be transferred to either output, or split between the two. The register is provided with a drain and control gate along the outer edge of the channel for charge dump purposes.
INTRODUCTION Large-area, back-illuminated CCD imager technology has been developed at Lincoln Laboratory over the past several years to support various space surveillance programs where high search rates, high sensitivity, and low noise are essential. These same features plus deep depletion depths are required in soft-x-ray astronomy, and we have been involved in multi-chip focal-plane development for x-ray space missions that include the ASCA and AXAF satellites [1,2]. All this technology is applicable to the needs of the astronomers as well, and we are now seeking ways to bring our advanced capabilities to the service of this community as well.
Ll: the 9k Ultra-Imager (right) and a test image (left) 5. SUMMARY Lockheed Martin's CCD technology is at the cutting edge of the digital image revolution. The requirements imposed to its essential components by the need of optimum performance military systems will grant benefits to all CCD users. Lockheed Martin aims to deploy its vast technical resources to capture a large portion of the commercial imager markets. The continued technology evolution pushed by these two major users will positively affect the smaller astronomical market.