Citation

Leeb WR, Poppe A, Hammel E, Alves J, Brunner M, Meingast S. Astrobiology 2013; 13(6): 521-535.

Affiliation

1 Institute of Telecommunications, Vienna University of Technology , Vienna, Austria .

Copyright

(Copyright © 2013, Mary Ann Liebert Publishers)

DOI

10.1089/ast.2012.0951

PMID

23980766

Abstract

To draw humankind's attention to its existence, an extraterrestrial civilization could well direct periodic laser pulses toward Earth. We developed a technique capable of detecting a quasi-periodic light signal with an average of less than one photon per pulse within a measurement time of a few tens of milliseconds in the presence of the radiation emitted by an exoplanet's host star. Each of the electronic events produced by one or more single-photon avalanche detectors is tagged with precise time-of-arrival information and stored. From this we compute a histogram displaying the frequency of event-time differences in classes with bin widths on the order of a nanosecond. The existence of periodic laser pulses manifests itself in histogram peaks regularly spaced at multiples of the-a priori unknown-pulse repetition frequency. With laser sources simulating both the pulse source and the background radiation, we tested a detection system in the laboratory at a wavelength of 850 nm. We present histograms obtained from various recorded data sequences with the number of photons per pulse, the background photons per pulse period, and the recording time as main parameters. We then simulated a periodic signal hypothetically generated on a planet orbiting a G2V-type star (distance to Earth 500 light-years) and show that the technique is capable of detecting the signal even if the received pulses carry as little as one photon on average on top of the star's background light. Key Words: Optical search for extraterrestrial intelligence-SETI-Single-photon detection-Detection of periodic laser signals. Astrobiology 13, 521-535.

Language: en