Paper
5 March 2003 Development of 2k x 2k FPA InSb modules for the NGST mission
Alan W. Hoffman, Peter J. Love, Ken J. Ando, Joseph P. Rosbeck, Nancy A. Lum, Roger Holcombe, John M. Durkee, Craig W. McMurtry
Author Affiliations +
Abstract
Raytheon Infrared Operations is under contract to develop 2K x 2K InSb arrays for the NGST NIRcam instrument and 1K x 1K Si:As IBC arrays for the NGST MIRI instrument. This paper reviews the progress in the NIR, showing NGST bare mux readout noise at 30 K of 2.4 e- and InSb dark current as low as 0.02 e-/s. Detectors and readouts have been fabricated in the 2K x 2K format and, except for adding indium bumps to the readouts, are ready for hybridization. Module and FPA designs are complete, resulting in a design that has self-aligning, interchangeable modules and requires no additional cold electronics to perform the NGST mission. Analysis predicts an alignment accuracy in the focus direction of ± 12 μm and total power for a 4K x 4K focal plane of 5 mW.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Alan W. Hoffman, Peter J. Love, Ken J. Ando, Joseph P. Rosbeck, Nancy A. Lum, Roger Holcombe, John M. Durkee, and Craig W. McMurtry "Development of 2k x 2k FPA InSb modules for the NGST mission", Proc. SPIE 4850, IR Space Telescopes and Instruments, (5 March 2003); https://doi.org/10.1117/12.461131
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Cited by 3 scholarly publications.
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KEYWORDS
Sensors

Staring arrays

Astronomy

Near infrared

Quantum efficiency

Electronics

Infrared radiation

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