A signal detection strategy for the SETI All Sky Survey

Details A signal detection strategy for the SETI All Sky Survey A signal detection strategy for the SETI All Sky Survey

Nov 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985tdapr..83..191l&link_type=abstract

In its The Telecommunications and Data Acquisition Report p 191-208 (SEE N86-14457 05-32)

Astronomy and Astrophysics

Astronomy

Project Seti, Reconnaissance, Signal Detection, Sky Surveys (Astronomy), Beams (Radiation), Computer Programs, Fast Fourier Transformations, Narrowband, Radio Antennas, Spectra, Surveys

Scientific paper

A source detection strategy for the SETI All Sky Survey is described. The method is designed to detect continuous wave (or very narrowband) sources transitting an antenna beam. The short-time spectra of the received signal are accumulated, and candidate extraterrestrial sources are recognized by the recognized by the presence of narrowband power exceeding a threshold function. The threshold function is derived using a Neyman-pearson hypothesis test.

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