HgCdTe (MCT) Photovoltaic Detector

2.3 – 3.6 µm, three-stage thermoelectrically cooled, optically immersed

PVI-3TE-3.4 is three-stage thermoelectrically cooled IR photovoltaic detector based on sophisticated HgCdTe heterostructure for the best performance and stability, optically immersed in order to improve parameters of the device. The detector is optimized for the maximum performance at λopt = 3.4 μm. Cut‑on wavelength can be optimized upon request. Reverse bias Vb may significantly increase response speed and dynamic range. It also results in improved performance at high frequencies, but 1/f noise that appears in biased devices may reduce performance at low frequencies. 3° wedged sapphire (wAl2O3) window prevents unwanted interference effects.

Spectral response (Ta = 20°C, Vb = 0 mV)

Features

  • High performance in the 2.3 - 3.6 µm spectral range
  • Three-stage thermoelectrically cooled
  • Hyperhemiimmersion microlens technology applied
  • No bias required
  • No 1/f noise

Specification (Ta = 20°C, Vb = 0 mV)

Parameter
PVI-3TE-3.4
Active element material
epitaxial HgCdTe heterostructure
Optimum wavelength λopt, µm
3.4
Detectivity D*(λpeak), cm⋅Hz1/2/W
≥7.0×1011
Detectivity D*(λopt), cm⋅Hz1/2/W
≥5.0×1011
Current responsivity Riopt), A/W
≥0.8
Time constant τ, ns
≤200
Resistance-optical area product R⋅AO, Ω⋅cm2
≥1500
Active element temperature Tdet, K
~210
Optical area AO, mm×mm
0.5×0.5, 1×1
Package
TO8, TO66
Acceptance angle, Φ
~36°
Window
wAl2O3

Mechanical layout, mm

Dedicated preamplifiers

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If you need Evaluation Units, please contact us.