Translator Disclaimer
Paper
29 September 2004 2Kx2K InSb for astronomy
Author Affiliations +
Abstract
Raytheon Vision Systems is under contract to develop 2K × 2K InSb Focal Plane Arrays (FPA) for the ORION and NEWFIRM projects teaming with NOAO, NASA, and USNO. This paper reviews the progress in the ORION, NEWFIRM, and the JWST projects, showing bare mux readout noise at 30 K of 2.4 e- and InSb dark current as low as 0.01 e-/s. Several FPAs have been fabricated to date and the ongoing improvements for the fabrication of FPAs will be discussed. The FPA and packaging designs are complete, resulting in a design that has self-aligning features for ease in FPA replacement at position of the focal plane assembly with alignment accuracy in the focus direction of ± 12 μm. The ORION/NEWFIRM modules are 2-side buttable to easily form 4K × 4K mosaics while the Phoenix modules, developed under the JWST development program, are 3-side buttable for ease in forming 4K × 2NK mosaics where N can be any integer. This paper will include FPA QE, dark current and noise performance, FPA reliability, and module-to-module flatness capabilities.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Alan W. Hoffman, Elizabeth Corrales, Peter J. Love, Joseph P. Rosbeck, Michael Merrill, Albert Fowler, and Craig McMurtry "2Kx2K InSb for astronomy", Proc. SPIE 5499, Optical and Infrared Detectors for Astronomy, (29 September 2004); https://doi.org/10.1117/12.555200
PROCEEDINGS
9 PAGES


SHARE
Advertisement
Advertisement
RELATED CONTENT

Low-noise, low-power HgCdTe/Al2O3 1024 x 1024 FPAs
Proceedings of SPIE (October 21 1996)
Current and future InSb infrared arrays for astronomy
Proceedings of SPIE (October 20 1993)
1024 x 1024 Si As IBC detector arrays for mid...
Proceedings of SPIE (June 15 2006)
Focal plane detectors for the WISE 12 and 23...
Proceedings of SPIE (September 19 2007)
Evaluation Of A 256 X 256 PtSi Array For Infrared...
Proceedings of SPIE (October 11 1989)

Back to Top