Paper
17 September 2009 Initial laboratory and sky testing results for the second generation H4RG-10 4k x 4k, 10 micron visible CMOS-Hybrid detector
Bryan N. Dorland, Rachel P. Dudik, Dan Veillette, Ryan Swindle, Augustyn Waczynski, Emily Kan
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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.
© (2009) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Bryan N. Dorland, Rachel P. Dudik, Dan Veillette, Ryan Swindle, Augustyn Waczynski, and Emily Kan "Initial laboratory and sky testing results for the second generation H4RG-10 4k x 4k, 10 micron visible CMOS-Hybrid detector", Proc. SPIE 7439, Astronomical and Space Optical Systems, 74390E (17 September 2009); https://doi.org/10.1117/12.827037
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Cited by 3 scholarly publications.
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KEYWORDS
Sensors

Cameras

Astronomy

Readout integrated circuits

Temperature metrology

Telescopes

Observatories

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