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

被引:5
|
作者
Suazo, Matias [1 ]
Zackrisson, Erik [1 ,2 ]
Mahto, Priyatam K. [3 ]
Lundell, Fabian [1 ]
Nettelblad, Carl [4 ]
Korn, Andreas J. [1 ]
Wright, Jason T. [5 ,6 ,7 ]
Majumdar, Suman [3 ,8 ]
机构
[1] Uppsala Univ, Dept Phys & Astron, Observat Astrophys, Box 516, SE-75120 Uppsala, Sweden
[2] Swedish Coll Adv Study, Linneanum, Thunbergsvagen 2, SE-75238 Uppsala, Sweden
[3] Indian Inst Technol, Dept Astron Astrophys & Space Engn, Indore 453552, India
[4] Uppsala Univ, Dept Informat Technol, Div Sci Comp, Uppsala SE-75105, Sweden
[5] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA
[6] Penn State Univ, Penn State Extraterr Intelligence Ctr, University Pk, PA 16802 USA
[7] Penn State Univ, Ctr Exoplanets & Habitable Worlds, University Pk, PA 16802 USA
[8] Imperial Coll, Dept Phys, Blackett Lab, London SW7 2AZ, England
基金
澳大利亚研究理事会; 美国国家科学基金会; 美国国家航空航天局;
关键词
extraterrestrial intelligence; infrared: stars; WARM DEBRIS DISKS; G INFRARED SEARCH; EXTRATERRESTRIAL CIVILIZATIONS; M-DWARFS; STARS; EVOLUTION; SIGNATURES; CONFUSION; ORIGINS; SAMPLE;
D O I
10.1093/mnras/stae1186
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页码:695 / 707
页数:13
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