A near-infrared SETI experiment: instrument overview
Shelley A. Wright, Dan Werthimer, Richard R. Treffers, Jerome Maire,, Geoffrey W. Marcy, Remington P.S. Stone, Frank Drake, Elliot Meyer, Patrick, Dorval, Andrew Siemion

TL;DR
This paper presents the design and development of a near-infrared SETI instrument utilizing advanced avalanche photodiodes for detecting pulsed laser signals, aiming to enhance the search for extraterrestrial communications.
Contribution
It introduces a novel near-infrared pulse search instrument with high sensitivity, low false alarms, and a versatile design based on recent optical SETI experience.
Findings
Instrument design with >1 GHz bandwidth APDs for near-infrared detection
Optimized system for high sensitivity and low false coincidence rates
Initial setup and search strategies for SETI targets described
Abstract
We are designing and constructing a new SETI (Search for Extraterrestrial Intelligence) instrument to search for direct evidence of interstellar communications via pulsed laser signals at near-infrared wavelengths. The new instrument design builds upon our past optical SETI experiences, and is the first step toward a new, more versatile and sophisticated generation of very fast optical and near-infrared pulse search devices. We present our instrumental design by giving an overview of the opto-mechanical design, detector selection and characterization, signal processing, and integration procedure. This project makes use of near-infrared (950-1650 nm) discrete amplification Avalanche Photodiodes (APD) that have greater than 1 GHz bandwidths with low noise characteristics and moderate gain (~10^4). We have investigated the use of single versus multiple detectors in our instrument (see…
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