Automation of finding strong gravitational lenses in the Kilo Degree Survey with U-DenseLens (DenseLens + Segmentation)
Bharath Chowdhary Nagam, L\'eon V E Koopmans, Edwin A Valentijn, Gijs, Verdoes Kleijn, Jelte T A de Jong, Nicola Napolitano, Rui Li, Crescenzo, Tortora, Valerio Busillo, Yue Dong

TL;DR
This paper enhances automated strong gravitational lens detection in large surveys by integrating segmentation and additional metrics into existing pipelines, significantly reducing false positives while discovering new lens candidates.
Contribution
It introduces a segmentation step with U-Net into the DenseLens pipeline and combines multiple metrics for improved accuracy in lens detection.
Findings
False positive rate reduced by ~25%
14 new strong lens candidates discovered
Segmentation improves detection reliability
Abstract
In the context of upcoming large-scale surveys like Euclid, the necessity for the automation of strong lens detection is essential. While existing machine learning pipelines heavily rely on the classification probability (P), this study intends to address the importance of integrating additional metrics, such as Information Content (IC) and the number of pixels above the segmentation threshold, to alleviate the false positive rate in unbalanced data-sets. In this work, we introduce a segmentation algorithm (U-Net) as a supplementary step in the established strong gravitational lens identification pipeline (Denselens), which primarily utilizes P and IC parameters for the detection and ranking. The results demonstrate that the inclusion of segmentation enables significant reduction of false positives by approximately 25 per cent in the final sample extracted from…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAdaptive optics and wavefront sensing · Geophysics and Gravity Measurements · Astronomical Observations and Instrumentation
