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FRONT-ILLUMINATED CCDs

Photonics Spectra
Jul 2001
Hamamatsu CorporationRequest Info
 
iFrontHamamatsu Corp. designed its S7847 series of front-illuminated FFT-CCDs with high IR sensitivity for low-light-level detection in scientific applications, including astronomy and spectrophotometry. The CCD chip is mounted on a four-stage TE cooler with a ΔT of 100 °C. Features include a wide dynamic range, low dark current and a spectral response range of 400 to 1100 nm. Typical readout noise is 6 e2 rms and maximum is 12 e2 rms. A binning operation enhances the signal-to-noise ratio and signal processing speed, and makes the CCDs suitable for use as linear image sensors. At -70 °C, the dark signal is typically 0.03, or a maximum of 0.1 e2 pixels per second. Two sensors are available, each with a pixel size of 24 x 24 µm.


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GLOSSARY
astronomy
The scientific observation of celestial radiation that has reached the vicinity of Earth, and the interpretation of these observations to determine the characteristics of the extraterrestrial bodies and phenomena that have emitted the radiation.
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