You have requested a machine translation of selected content from our databases. This functionality is provided solely for your convenience and is in no way intended to replace human translation. Neither SPIE nor the owners and publishers of the content make, and they explicitly disclaim, any express or implied representations or warranties of any kind, including, without limitation, representations and warranties as to the functionality of the translation feature or the accuracy or completeness of the translations.
Translations are not retained in our system. Your use of this feature and the translations is subject to all use restrictions contained in the Terms and Conditions of Use of the SPIE website.
18 July 2000Advanced MOS CCDs for high-throughput x-ray astronomy missions
We present the latest design concepts of CCDs for the next generation of X-ray astronomical applications together with test results of new detector developments for these applications. In particular we consider ways of overcoming the fundamental limitations of these detectors, namely area coverage and low readout speeds. The manufacture of a high yielding, highly efficient CCD with a well understood response at all energies remains a high priority and we discuss our program to achieve this goal. Amongst other features: increased deep depletion and state of the art noise performance will be examined.
The alert did not successfully save. Please try again later.
Andrew D. Holland, Adam Keay, Ian Hutchinson, David J. Burt, "Advanced MOS CCDs for high-throughput x-ray astronomy missions," Proc. SPIE 4012, X-Ray Optics, Instruments, and Missions III, (18 July 2000); https://doi.org/10.1117/12.391554