Astronomical imaging with the Texas Instruments 3-phase CCD

Details Astronomical imaging with the Texas Instruments 3-phase CCD Astronomical imaging with the Texas Instruments 3-phase CCD

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984spie..501..339g&link_type=abstract

IN: State-of-the-art imaging arrays and their applications; Proceedings of the Meeting, San Diego, CA, August 21-23, 1984 (A86-1

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Applications

Charge Coupled Devices, Hubble Space Telescope, Imaging Techniques, Nasa Programs, Quantum Efficiency, Signal Processing

Scientific paper

A reject device from the NASA/JPL development program for the Space Telescope has been evaluated for its utility in imaging at extremely low flux levels. This thinned, backside-illuminated 800 x 800 imager is run at cryogenic temperatures, allowing long integration times on faint astronomical sources. The device has to date been successfully used for both high-dispersion echelle spectroscopy and for low-dispersion work with the Faint Object Grism Spectrograph. In both these applications the T.I. three-phase imager has shown exceptionally good performance compared to other CCDs.

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