2025AJ....170...12P


Query : 2025AJ....170...12P

2025AJ....170...12P - Astron. J., 170, 12 (2025/July-0)

Using Anomaly Detection to Search for Technosignatures in Breakthrough Listen Observations.

PARDO S., POZNANSKI D., CROFT S., SIEMION A.P.V. and LEBOFSKY M.

Abstract (from CDS):

We implement a machine learning algorithm to search for extraterrestrial technosignatures in radio observations of several hundred nearby stars, obtained with the Parkes and Green Bank Telescopes by the Breakthrough Listen collaboration. Advances in detection technology have led to an exponential growth in data, necessitating innovative and efficient analysis methods. This problem is exacerbated by the large variety of possible forms an extraterrestrial signal might take, and the size of the multidimensional parameter space that must be searched. It is then made markedly worse by the fact that our best guess at the properties of such a signal is that it might resemble the signals emitted by human technology and communications, the main (yet diverse) contaminant in radio observations. We address this challenge by using a combination of simulations and machine learning methods for anomaly detection. We rank candidates by how unusual they are in frequency, and how persistent they are in time, by measuring the similarity between consecutive spectrograms of the same star. We validate that our filters significantly improve the quality of the candidates that are selected for human vetting when compared to a random selection. Of the ∼1011 spectrograms that we analyzed, we visually inspected thousands of the most promising spectrograms, and thousands more for validation, about 20,000 in total, and report that no candidate survived basic scrutiny.

Abstract Copyright: © 2025. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Search for extraterrestrial intelligence

Simbad objects: 7

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Number of rows : 7
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 HD 17925 RS* 02 52 32.1281856011 -12 46 10.968056223 7.48 6.91 6.05 5.34 4.89 K1V 557 0
2 HD 22879 Pe* 03 40 22.0652879951 -03 13 01.124265616 7.146 7.222 6.667 6.346 6.016 G0VmF2 529 0
3 HD 97233 PM* 11 11 33.1488855786 -14 59 28.926586491 11.394 10.26 9.038 8.285 7.607 K5Vk: 96 1
4 * iot Crt PM* 11 38 40.0180807728 -13 12 06.981257088   5.97 5.48     F6.5V 90 0
5 * 10 CVn PM* 12 44 59.4049642264 +39 16 44.098132297 6.47 6.50 5.95 5.41 5.12 F9V_Fe-0.3 400 0
6 HD 118096 PM* 13 34 03.2375632359 +33 13 42.211585003   10.28   8.6   K4V 61 0
7 BD+45 4378 ** 23 58 43.4881610546 +46 43 44.737257440   11.02 9.78 9.25   K7V 88 0

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