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

C. E. Petrillo, C. Tortora, G. Vernardos, L. V. E. Koopmans, G. Verdoes Kleijn, M. Bilicki, N. R. Napolitano, S. Chatterjee, G. Covone, A. Dvornik, T. Erben, F. Getman, B. Giblin, C. Heymans, J. T. A. de Jong, K. Kuijken, P. Schneider, H. Shan, C. Spiniello, A. H. Wright

Research output: Contribution to journalArticlepeer-review

Abstract / Description of output

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.
Original languageEnglish
Number of pages19
JournalMonthly Notices of the Royal Astronomical Society
Early online date17 Jan 2019
DOIs
Publication statusE-pub ahead of print - 17 Jan 2019

Keywords / Materials (for Non-textual outputs)

  • astro-ph.GA

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