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Mining for Strong Gravitational Lenses with Self-supervised Learning
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We employ self-supervised representation learning to distill information from 76 million galaxy images from the Dark Energy Spectroscopic Instrument Legacy Imaging Surveys' Data Release 9. Targeting the identification of new strong gravitational lens candidates, we first create a rapid similarity search tool to discover new strong lenses given only a single labelled example. We then show how training a simple linear classifier on the self-supervised representations, requiring only a few minutes on a CPU, can automatically classify strong lenses with great efficiency. We present 1192 new strong lens candidates that we identified through a brief visual identification campaign, and release an interactive web-based similarity search tool and the top network predictions to facilitate crowd-sourcing rapid discovery of additional strong gravitational lenses and other rare objects: https://github.com/georgestein/ssl-legacysurvey.
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Cited by 3 Pith papers
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The Last Stand Before Rubin: a consolidated sample of strong lensing systems in wide-field surveys
A new compilation of over 30,000 strong-lensing candidates with multi-survey images yields an independent ground-based constraint γ_PPN = 1.023 ± 0.028 and a combined constraint γ_PPN = 1.034 ± 0.025.
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Gravitational Lenses in UNIONS and Euclid (GLUE) I: A Search for Strong Gravitational Lenses in UNIONS with Subaru, CFHT, and Pan-STARRS Data
A ResNet trained on real lenses found 1,346 new strong lens candidates in the UNIONS survey, with 15 systems confirmed by overlapping galaxy spectra.
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Confirming HSC strong lens candidates with DESI Spectroscopy. I. Project overview and first results
Serendipitous DESI DR1 spectra confirm 27 HSC strong-lens systems and add 76 candidates with lensing galaxies at z>0.8.
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