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Proceedings Paper

Initial laboratory and sky testing results for the second generation H4RG-10 4k x 4k, 10 micron visible CMOS-Hybrid detector
Author(s): Bryan N. Dorland; Rachel P. Dudik; Dan Veillette; Ryan Swindle; Augustyn Waczynski; Emily Kan
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Paper Abstract

We present the initial performance test results for the H4RG-10 (A2), the second generation of the H4RG-10 visible CMOS-Hybrid Sensor Chip Assembly (SCA). The first science grade H4RG-10 (A2), delivered in 2009, is an evolution of the first generation A1, first delivered and tested in 2007. The H4RG-10 is primarily intended for ground- and space-based astronomical applications. Our evaluation focused on the performance parameters as they are related to astrometric applications. We find that the A2 SCA shows high pixel interconnect (99.6%), and low read noise (10-15 e- RMS) when operated at high speeds, consistent with A1 results. Most importantly, the H4RG-10 (A2) shows a dramatic improvement in dark current vs. the A1, with a two order of magnitude reduction in mean dark level and significantly reduced hot pixel population below 200 K.

Paper Details

Date Published: 17 September 2009
PDF: 10 pages
Proc. SPIE 7439, Astronomical and Space Optical Systems, 74390E (17 September 2009); doi: 10.1117/12.827037
Show Author Affiliations
Bryan N. Dorland, U.S. Naval Observatory (United States)
Rachel P. Dudik, U.S. Naval Observatory (United States)
Dan Veillette, U.S. Naval Observatory (United States)
Ryan Swindle, Institute for Astronomy, Univ. of Hawaii (United States)
Augustyn Waczynski, Global Science and Technology, Inc. (United States)
NASA Goddard Space Flight Ctr. (United States)
Emily Kan, Global Science and Technology, Inc. (United States)
NASA Goddard Space Flight Ctr. (United States)


Published in SPIE Proceedings Vol. 7439:
Astronomical and Space Optical Systems
Penny G. Warren; James B. Heaney; Robert K. Tyson; Michael Hart; E. Todd Kvamme; Cheryl J. Marshall, Editor(s)

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