By M. M. Blouke, T. Woody, T. Dosluoglu, S. T. Elliott, J. R. Janesick, R. Reed, R. Stover (auth.), James W. Beletic, Paola Amico (eds.)
The Workshop "Optical Detectors for Astronomy" used to be held in the course of October 8-10, 1996 on the headquarters of the eu Southern Observatory in Garching, Germany. This was once the 3rd assembly of its type, prior conferences being held in 1991 and 1993, yet this can be the 1st ESO "CCD Workshop" that has released court cases. many of the prime brands and significant astronomical observatories have been represented, with the 117 attendees coming jointly from 14 various nations that spanned each continent in the world. the inducement for the ESO CCD Workshop sequence is the production of casual and open venue of knowledge trade approximately astronomical CCD detectors and structures. Judging from the response and suggestions of the contributors, the 1996 workshop was once as winning because the prior variations, that is a credits to all who attended. The Workshop was once geared up as a mix of invited talks, oral shows, poster classes and roundtable discussions, the latter used to foster a loose alternate of principles between contributors. those technical periods have been complemented via a gap reception and a congenial night in downtown Munich, which incorporated a strolling journey of the ancient zone by way of dinner on the well-known Franziskaner brewery and an after dinner speak by way of Walter Kosonocky, who reviewed the heritage of CCD technology.
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Additional info for Optical Detectors for Astronomy: Proceedings of an ESO CCD Workshop held in Garching, Germany, October 8–10, 1996
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.