A high performance 1200x400 CCD array for astronomy applications.

Details A high performance 1200x400 CCD array for astronomy applications. A high performance 1200x400 CCD array for astronomy applications.

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989spie.1071..170h&link_type=abstract

Conference on Optical Sensors and Electronic Photography in Conjunction with the Symposium on Optics, Electro-Optics and Laser A

Physics

Optics

Ccd Detectors

Scientific paper

This paper describes the design and performance of a scientific CCD array for use in astronomy applications. The device is a four-phase, buried-channel CCD structure that operates in the frametransfer mode for imaging the scenes at low light levels in the spectral regions from 450 nm to near infrared. The sensor consists of two sections of 1200x200 CCD imaging elements with 27x27 μm2 pixel size. The high full-well capacity of each pixel (>0.6 million electrons) and low readout noise (<4 electrons rms) yield a dynamic range of more than 103 dB.

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