Journal article icon

Journal article

Simulating the stellar bycatch: constraining the prevalence of extraterrestrial transmitters within radio SETI surveys

Abstract:
Searches for radio technosignatures place constraints on the prevalence of extraterrestrial transmitters in our Galaxy and beyond. It is important to account for the complete stellar population captured within a radio telescope’s field of view, or stellar ‘bycatch’. In recent years, catalogues from ESA’s Gaia mission have enabled the search for extraterrestrial intelligence (SETI) surveys to place tighter limits on extraterrestrial transmitter statistics. However, Gaia remains restricted by magnitude limits, astrometric uncertainty at large distances, and confusion in crowded regions. To address these limitations, we investigate the use of the Besançon Galactic model to simulate the statistical underlying stellar population to derive more realistic constraints on the occurrence of extraterrestrial transmitters. We apply this method to Breakthrough Listen’s Enriquez/Price survey, modelling 6182 364 stellar objects within 1229 individual pointings and extending the search out to distances kpc. We place limits on the prevalence of high-duty-cycle transmitters within 2.5 kpc, suggesting of stellar systems contain such a transmitter (for near-zero drift rates and W). In support of broader adoption, we provide a simple calculator tool that enables other researchers to incorporate this approach into their own SETI analyses. Our results enable a more complete statistical estimation of the number and stellar type of systems probed, thereby strengthening constraints on technosignature prevalence and guiding the analysis of future SETI efforts. We also conclude that SETI surveys are, in fact, much less biased by anthropocentric assumptions than is often suggested.
Publication status:
Published
Peer review status:
Peer reviewed

Actions

Access Document

Files:
Publisher copy:
10.1093/mnras/staf2112

Authors

More by this author
Role:
Author
ORCID:
0009-0003-8412-3613
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Physics - Central
Role:
Author


Publisher:
Oxford University Press
Journal:
Monthly Notices of the Royal Astronomical Society More from this journal
Volume:
545
Issue:
3
Pages:
staf2112
Article number:
staf2112
Publication date:
2025-11-27
Acceptance date:
2025-11-21
DOI:
EISSN:
1365-2966
ISSN:
0035-8711


Language:
English
Keywords:
Pubs id:
2349682
UUID:
uuid_ccbeb1ad-ea69-4a20-bb92-f1889e59cf93
Local pid:
pubs:2349682
Source identifiers:
3585887
Deposit date:
2025-12-22
ARK identifier:
This ORA record was generated from metadata provided by an external service. It has not been edited by the ORA Team.

Terms of use


Views and Downloads






If you are the owner of this record, you can report an update to it here: Report update to this record

TO TOP