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 ∼88000 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 ∼3000 lens candidates with less than 10 per cent expected false positives and requiring minimal human intervention.
@article{arxiv.1812.03168,
title = {LinKS: Discovering galaxy-scale strong lenses in the Kilo-Degree Survey using Convolutional Neural Networks},
author = {C. E. Petrillo and C. Tortora and G. Vernardos and L. V. E. Koopmans and G. Verdoes Kleijn and M. Bilicki and N. R. Napolitano and S. Chatterjee and G. Covone and A. Dvornik and T. Erben and F. Getman and B. Giblin and C. Heymans and J. T. A. de Jong and K. Kuijken and P. Schneider and H. Shan and C. Spiniello and A. H. Wright},
journal= {arXiv preprint arXiv:1812.03168},
year = {2019}
}
Comments
19 pages, 11 figures, accepted for publication in MNRAS