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HgCdZnTe DETECTORS
nBroad spectral response 2 to 12 µm and
beyond
nDC to subnanosecond operation
nNo flicker noise down to 0 Hz in photovoltaic
mode
nMonolithic optical immersion
nRoom temperature and TE cooled operation
Our Mercury Cadmium Zinc Telluride Detectors
(HgCdZnTe) cover a broad spectral range, 2 to 12 µm, and
have excellent detectivity. Fig. 1 shows typical curves. They
are excellent for infrared laser characterization and
stabilization, for heterodyne detection, FT-IR, fast pyrometry,
and radiometry.
Optical immersion is a classical way to make a
physically small detector (lower noise, lower bias
requirements, lower bias current heating, etc.) look optically
larger for more sensitivity. It is particularly easy to do with
the monolithic manufacturing technique of our detectors,
see Fig. 2. Our proprietary technique ensures a perfect
optical match between lens and detector. We have
removed the transmission limits normally set by bonding
adhesives.
PHOTOVOLTAIC OPERATION
Photovoltaic operation is preferred for lower frequency
applications, to avoid the bias current created 1/f noise. It
also allows highest frequency operation, down to the 100 ps
level. Response time in the photovoltaic mode is only
limited by the carrier diffusion time through the very thin
HgCdTe layer. Two forms of photovoltaic products are
available: the magnetically (PEM) assisted ones and the
photodiffusion (PD) effect assisted ones.
The PD variety is now available even in TE cooled
versions for optimum performance throughout the
frequency spectrum.
70777 HgCdZnTe Detector.
Fig. 2 Schematic of optically immersed HgCdZnTe Detectors.
Fig. 1 Typical detectivities of HgCdZnTe Detectors.
TECHNOTE
PD type detectors offer high speed response, ideal for
applications involving short pulse lasers. Occassionally
these detectors exhibit responsivity curves with both
positive and negative wavelength response regions. We
can select spectrally well balanced units for you, if you
let us know that your application covers more than a
single laser wavelength.