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Record W4396702053 · doi:10.1093/mnras/stae1186

Project Hephaistos – II. Dyson sphere candidates from <i>Gaia</i> DR3, 2MASS, and <i>WISE</i>

2024· article· en· W4396702053 on OpenAlexfundno aff
Matías Suazo, Erik Zackrisson, Priyatam K Mahto, Fabian Lundell, Carl Nettelblad, A. J. Korn, Jason T. Wright, Suman Majumdar

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsnot available
FundersNational Cancer InstituteAustralian Astronomical Optics-MacquarieScience Mission DirectorateSmithsonian Astrophysical ObservatoryUniversity of California, Los AngelesJet Propulsion LaboratoryMax-Planck-Institut für AstronomieDurham UniversityMinistry of Education, IndiaQueen's UniversityQueen's University BelfastSwinburne University of TechnologyNational Central UniversityPlanetary Science DivisionMonash UniversitySwedish Collegium for Advanced StudyAustralian GovernmentAustralian Research CouncilSpace Telescope Science InstituteEötvös Loránd TudományegyetemMagnus Bergvalls StiftelseNational Computational InfrastructureRoyal Swedish Academy of SciencesLos Alamos National LaboratoryUppsala UniversitetJohns Hopkins UniversityEuropean Space AgencyAustralian National Data ServiceNational Science FoundationScheme for Promotion of Academic and Research CollaborationAstronomy Australia LimitedAustralian National UniversityNational Aeronautics and Space AdministrationCurtin University of TechnologyCalifornia Institute of TechnologySmithsonian Institution
KeywordsPhysicsSearch for extraterrestrial intelligenceConfusionStarsAstronomyInfraredPipeline (software)SPHERESAstrophysicsConvolutional neural networkTheoretical physicsArtificial intelligenceComputer science

Abstract

fetched live from OpenAlex

ABSTRACT The search for extraterrestrial intelligence is currently being pursued using multiple techniques and in different wavelength bands. Dyson spheres, megastructures that could be constructed by advanced civilizations to harness the radiation energy of their host stars, represent a potential technosignature, that in principle may be hiding in public data already collected as part of large astronomical surveys. In this study, we present a comprehensive search for partial Dyson spheres by analysing optical and infrared observations from Gaia, 2MASS, and WISE. We develop a pipeline that employs multiple filters to identify potential candidates and reject interlopers in a sample of five million objects, which incorporates a convolutional neural network to help identify confusion in WISE data. Finally, the pipeline identifies seven candidates deserving of further analysis. All of these objects are M-dwarfs, for which astrophysical phenomena cannot easily account for the observed infrared excess emission.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.001
metaresearch head score (Gemma)0.001
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.010
Threshold uncertainty score0.020

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.001
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0050.004

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.007
GPT teacher head0.202
Teacher spread0.196 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations21
Published2024
Admission routes1
Has abstractyes

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