Combining neural networks with galaxy light subtraction for discovering strong lenses in the HSC SSP
Yuichiro Ishida, Kenneth C. Wong, Anton T. Jaelani, Anupreeta More

TL;DR
This paper introduces a new technique that subtracts galaxy light from images to enhance the detection of strong gravitational lenses using neural networks, leading to improved classification accuracy in large imaging surveys.
Contribution
The study demonstrates that combining light-subtracted images with original images enhances CNN performance in identifying strong lenses in the HSC SSP dataset.
Findings
Improved AUC to 0.841 with combined images
Light subtraction increases contrast of lensed sources
Combining images mitigates residual subtraction artifacts
Abstract
Galaxy-scale strong gravitational lenses are valuable objects for a variety of astrophysical and cosmological applications. Strong lensing galaxies are rare, so efficient search methods, such as convolutional neural networks, are often used on large imaging datasets. In this work, we apply a new technique to improve the performance of supervised neural networks by subtracting the central (lensing) galaxy light from both the training and test datasets. We use multiband imaging data from the Hyper Suprime-Cam Subaru Strategic Program (HSC SSP) as our training and test datasets. By subtracting the lensing galaxy light, we increase the contrast of the lensed source compared to the original imaging data. We also apply the light subtraction to non-lenses in order to compare them to the light-subtracted lenses. Residual features resulting from poor light subtraction can adversely affect the…
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 · Astronomy and Astrophysical Research · Astronomical Observations and Instrumentation
