Narrow-Band Signal Localization for SETI on Noisy Synthetic Spectrogram Data
Bryan Brzycki, Andrew P. V. Siemion, Steve Croft, Daniel Czech, David, DeBoer, Julia DeMarines, Jamie Drew, Vishal Gajjar, Howard Isaacson, Brian, Lacki, Matthew Lebofsky, David H. E. MacMahon, Imke de Pater, Danny C. Price,, S. Pete Worden

TL;DR
This paper develops a CNN-based method for localizing narrow-band signals in synthetic spectrogram data, improving detection of multiple signals including dim ones amidst noise, relevant for SETI signal analysis.
Contribution
It introduces a residual CNN architecture with multiple input normalizations that outperforms simpler models in localizing signals in synthetic SETI data.
Findings
Residual CNN reduces localization error by at least 3x at high SNR.
Multiple input normalizations improve model performance.
CNNs show promise for crowded signal detection in noisy spectrograms.
Abstract
As it stands today, the search for extraterrestrial intelligence (SETI) is highly dependent on our ability to detect interesting candidate signals, or technosignatures, in radio telescope observations and distinguish these from human radio frequency interference (RFI). Current signal search pipelines look for signals in spectrograms of intensity as a function of time and frequency (which can be thought of as images), but tend to do poorly in identifying multiple signals in a single data frame. This is especially apparent when there are dim signals in the same frame as bright, high signal-to-noise ratio (SNR) signals. In this work, we approach this problem using convolutional neural networks (CNN) as a computationally efficient method for localizing signals in synthetic observations resembling data collected by Breakthrough Listen using the Green Bank Telescope. We generate two synthetic…
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