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Project Hephaistos - II. Dyson sphere candidates from Gaia DR3, 2MASS, and WISE

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arxiv 2405.02927 v1 pith:KO6YE4CS submitted 2024-05-05 astro-ph.SR

Project Hephaistos - II. Dyson sphere candidates from Gaia DR3, 2MASS, and WISE

classification astro-ph.SR
keywords candidatesdysonwisedatagaiaidentifyinfraredmass
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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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 analyzing 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 7 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.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Project Hephaistos -- IV. James Webb Space Telescope Observations of Two Dyson Sphere Candidates

    astro-ph.GA 2026-07 accept novelty 6.5

    JWST/MIRI data attribute the mid-IR excess of Hephaistos candidates D and E to background galaxies at z≈0.9 (Hot-DOG-like) and z≈0.4 (dusty starburst), not to Dyson spheres or debris disks.