4.7 Article

High-quality Strong Lens Candidates in the Final Kilo-Degree Survey Footprint

Journal

ASTROPHYSICAL JOURNAL
Volume 923, Issue 1, Pages -

Publisher

IOP Publishing Ltd
DOI: 10.3847/1538-4357/ac2df0

Keywords

-

Funding

  1. China Postdoctoral Science Foundation [2020M672935, 2021T140773]
  2. Guangdong Basic and Applied Basic Research Foundation [2019A1515110286]
  3. One hundred top talent program of Sun Yat-sen University [71000-18841229]
  4. European Union Horizon 2020 research and innovation program under the Marie Skodowska-Curie grant [721463]
  5. Hintze Fellow at the Oxford Centre for Astrophysical Surveys through Hintze Family Charitable Foundation
  6. European Union's Horizon 2020 research and innovation program under the Marie Sklodovska-Curie grant [897124]
  7. ERC [770935]
  8. European Research Council [770935, 647112]
  9. Max Planck Society
  10. Alexander von Humboldt Foundation
  11. Heisenberg grant of the Deutsche Forschungsgemeinschaft [Hi 1495/5-1]
  12. Marie Curie Actions (MSCA) [897124] Funding Source: Marie Curie Actions (MSCA)
  13. European Research Council (ERC) [770935] Funding Source: European Research Council (ERC)

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Using a new convolutional neural network (CNN) classifier, 97 new high-quality strong lensing candidates were discovered in the KiDS optical survey area, bringing the total to 268 systems. The complementarity of morphology and color information in multi-band composites successfully identified these candidates.
We present 97 new high-quality strong lensing candidates found in the final similar to 350 deg(2) that complete the full similar to 1350 deg(2) area of the Kilo-Degree Survey (KiDS). Together with our previous findings, the final list of high-quality candidates from KiDS sums up to 268 systems. The new sample is assembled using a new convolutional neural network (CNN) classifier applied to r-band (best-seeing) and g, r, and i color-composited images separately. This optimizes the complementarity of the morphology and color information on the identification of strong lensing candidates. We apply the new classifiers to a sample of luminous red galaxies (LRGs) and a sample of bright galaxies (BGs) and select candidates that received a high probability to be a lens from the CNN (P (CNN)). In particular, setting P (CNN) > 0.8 for the LRGs, the one-band CNN predicts 1213 candidates, while the three-band classifier yields 1299 candidates, with only similar to 30% overlap. For the BGs, in order to minimize the false positives, we adopt a more conservative threshold, P (CNN) > 0.9, for both CNN classifiers. This results in 3740 newly selected objects. The candidates from the two samples are visually inspected by seven coauthors to finally select 97 high-quality lens candidates which received mean scores larger than 6 (on a scale from 0 to 10). We finally discuss the effect of the seeing on the accuracy of CNN classification and possible avenues to increase the efficiency of multiband classifiers, in preparation of next-generation surveys from ground and space.

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