http://arxiv.org/abs/1906.03837
We present detector characterization of a state-of-the-art near-infrared (950nm – 1650 nm) Discrete Avalanche Photodiode detector (NIRDAPD) 5×5 array. We designed an experimental setup to characterize the NIRDAPD dark count rate, photon detection efficiency (PDE), and non-linearity. The NIRDAPD array was illuminated using a 1050 nm light-emitting diode (LED) as well as 980 nm, 1310 nm, and 1550 nm laser diodes. We find a dark count rate of 3.3×10$^6$ cps, saturation at 1.2×10$^8$ photons per second, a photon detection efficiency of 14.8% at 1050 nm, and pulse detection at 1 GHz. We characterized this NIRDAPD array for a future astrophysical program that will search for technosignatures and other fast (>1 Ghz) astrophysical transients as part of the Pulsed All-sky Near-infrared Optical Search for Extraterrestrial Intelligence (PANOSETI) project. The PANOSETI program will consist of an all-sky optical (350 – 800 nm) observatory capable of observing the entire northern hemisphere instantaneously and a wide-field NIR (950 – 1650 nm) component capable of drift scanning the entire sky in 230 clear nights. PANOSETI aims to be the first wide-field fast-time response near-infrared transient search.
S. Li, J. Maire, M. Cosens, et. al.
Tue, 11 Jun 19
34/60
Comments: 8 pages, 7 figures, 1 table
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