Paper
9 October 2008 Enhanced broadband (11-15 µm) QWIP FPAs for space applications
Alexandru Nedelcu, Nadia Brière de l'Isle, Jean-Patrick Truffer, Eric Belhaire, Eric Costard, Philippe Bois, Patrick Merken, Olivier Saint-Pé
Author Affiliations +
Proceedings Volume 7106, Sensors, Systems, and Next-Generation Satellites XII; 71061K (2008) https://doi.org/10.1117/12.800305
Event: SPIE Remote Sensing, 2008, Cardiff, Wales, United Kingdom
Abstract
A thirty months ESA project started in March 2008, whose overall purpose is to expand and assess the performance of broadband (11-15 µm) quantum detectors for spectro-imaging applications: Dispersive Spectrometers (DS) and Fourier Transform Spectrometers (FTS). We present here the technical requirements, the development approach chosen as well as preliminary signal to noise ratio (SNR) calculations. Our approach is fully compatible with the final array format (1024x256, pitch 50-60μm). We expect the requested uniformity, operability and SNR levels to be achieved at the goal temperatures (60K for FTS applications and 50K for DS applications). The performance level will be demonstrated on 256x256, 50µm pitch arrays. Also, operability and uniformity issues will be addressed on large mechanical 1024x256 hybrid arrays.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Alexandru Nedelcu, Nadia Brière de l'Isle, Jean-Patrick Truffer, Eric Belhaire, Eric Costard, Philippe Bois, Patrick Merken, and Olivier Saint-Pé "Enhanced broadband (11-15 µm) QWIP FPAs for space applications", Proc. SPIE 7106, Sensors, Systems, and Next-Generation Satellites XII, 71061K (9 October 2008); https://doi.org/10.1117/12.800305
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Cited by 7 scholarly publications.
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KEYWORDS
Quantum well infrared photodetectors

Signal to noise ratio

Fourier transforms

Sensors

Quantum wells

Absorption

Electrons

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