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LinKS: Discovering galaxy-scale strong lenses in the Kilo-Degree Survey using Convolutional Neural Networks

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arxiv 1812.03168 v2 pith:HZ3ITTY3 submitted 2018-12-07 astro-ph.GA

classification astro-ph.GA
keywords candidatessamplestrongkilo-degreelenslenseslinkssurvey
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abstract

We present a new sample of galaxy-scale strong gravitational-lens candidates, selected from 904 square degrees of Data Release 4 of the Kilo-Degree Survey (KiDS), i.e., the "Lenses in the Kilo-Degree Survey" (LinKS) sample. We apply two Convolutional Neural Networks (ConvNets) to $\sim88\,000$ colour-magnitude selected luminous red galaxies yielding a list of 3500 strong-lens candidates. This list is further down-selected via human inspection. The resulting LinKS sample is composed of 1983 rank-ordered targets classified as "potential lens candidates" by at least one inspector. Of these, a high-grade subsample of 89 targets is identified with potential strong lenses by all inspectors. Additionally, we present a collection of another 200 strong lens candidates discovered serendipitously from various previous ConvNet runs. A straightforward application of our procedure to future Euclid or LSST data can select a sample of $\sim3000$ lens candidates with less than 10 per cent expected false positives and requiring minimal human intervention.

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  1. Confirming HSC strong lens candidates with DESI Spectroscopy. I. Project overview and first results

    astro-ph.GA 2025-05 conditional novelty 5.0 of 10

    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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