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Proceedings Paper

4Kx4K format 10-micron pixel pitch H4RG-10 hybrid CMOS silicon visible focal plane array for space astronomy
Author(s): Yibin Bai; William Tennant; Selmer Anglin; Andre Wong; Mark Farris; Min Xu; Eric Holland; Donald Cooper; Joseph Hosack; Kenneth Ho; Thomas Sprafke; Robert Kopp; Brian Starr; Richard Blank; James W. Beletic; Gerard A. Luppino
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Paper Abstract

Teledyne’s silicon hybrid CMOS focal plane array technology has matured into a viable, high performance and high- TRL alternative to scientific CCD sensors for space-based applications in the UV-visible-NIR wavelengths. This paper presents the latest results from Teledyne’s low noise silicon hybrid CMOS visible focal place array produced in 4K×4K format with 10 μm pixel pitch. The H4RG-10 readout circuit retains all of the CMOS functionality (windowing, guide mode, reference pixels) and heritage of its highly successful predecessor (H2RG) developed for JWST, with additional features for improved performance. Combined with a silicon PIN detector layer, this technology is termed HyViSI™ (Hybrid Visible Silicon Imager). H4RG-10 HyViSI™ arrays achieve high pixel interconnectivity (<99.99%), low readout noise (<10 e- rms single CDS), low dark current (<0.5 e-/pixel/s at 193K), high quantum efficiency (<90% broadband), and large dynamic range (<13 bits). Pixel crosstalk and interpixel capacitance (IPC) have been predicted using detailed models of the hybrid structure and these predictions have been confirmed by measurements with Fe-55 Xray events and the single pixel reset technique. For a 100-micron thick detector, IPC of less than 3% and total pixel crosstalk of less than 7% have been achieved for the HyViSI™ H4RG-10. The H4RG-10 array is mounted on a lightweight silicon carbide (SiC) package and has been qualified to Technology Readiness Level 6 (TRL-6). As part of space qualification, the HyViSI™ H4RG-10 array passed radiation testing for low earth orbit (LEO) environment.

Paper Details

Date Published: 25 September 2012
PDF: 18 pages
Proc. SPIE 8453, High Energy, Optical, and Infrared Detectors for Astronomy V, 84530M (25 September 2012); doi: 10.1117/12.926748
Show Author Affiliations
Yibin Bai, Teledyne Imaging Sensors (United States)
William Tennant, Teledyne Imaging Sensors (United States)
Selmer Anglin, Teledyne Imaging Sensors (United States)
Andre Wong, Teledyne Imaging Sensors (United States)
Mark Farris, Teledyne Imaging Sensors (United States)
Min Xu, Teledyne Imaging Sensors (United States)
Eric Holland, Teledyne Imaging Sensors (United States)
Donald Cooper, Teledyne Imaging Sensors (United States)
Joseph Hosack, Teledyne Imaging Sensors (United States)
Kenneth Ho, Teledyne Imaging Sensors (United States)
Thomas Sprafke, Teledyne Imaging Sensors (United States)
Robert Kopp, Teledyne Imaging Sensors (United States)
Brian Starr, Teledyne Imaging Sensors (United States)
Richard Blank, Teledyne Imaging Sensors (United States)
James W. Beletic, Teledyne Imaging Sensors (United States)
Gerard A. Luppino, GL Scientific (United States)

Published in SPIE Proceedings Vol. 8453:
High Energy, Optical, and Infrared Detectors for Astronomy V
Andrew D. Holland; James W. Beletic, Editor(s)

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