Using deep Residual Networks to search for galaxy-Ly{\alpha} emitter lens candidates based on spectroscopic-selection
Rui Li, Yiping Shu, Jianlin Su, Haicheng Feng, Guobao Zhang, Jiancheng, Wang, Hongtao Liu

TL;DR
This paper introduces a deep Residual Network approach to identify galaxy-Lyα emitter lens candidates from spectroscopic data, achieving high accuracy and discovering new potential lenses in SDSS data.
Contribution
The study applies a 28-layer ResNet to spectroscopic data for lens candidate detection, with a large synthetic training set, demonstrating high accuracy and discovering new candidates.
Findings
Test accuracy of 99.54% on synthetic data
92.5% recovery rate of known candidates
536 new lens candidates identified
Abstract
More than one hundred galaxy-scale strong gravitational lens systems have been found by searching for the emission lines coming from galaxies with redshifts higher than the lens galaxies. Based on this spectroscopic-selection method, we introduce the deep Residual Networks (ResNet, a kind of deep Convolutional Neural Networks) to search for the galaxy-Ly emitter (LAE) lens candidates by recognizing the Ly emission lines coming from high redshift galaxies () in the spectra of early-type galaxies (ETGs) at middle redshift (). The spectra of the ETGs come from the Data Release 12 (DR12) of the Baryon Oscillation Spectroscopic Survey (BOSS) of the Sloan Digital Sky Survey \uppercase\expandafter{\romannumeral3} (SDSS-\uppercase\expandafter{\romannumeral3}). In this paper, we first build a 28 layers ResNet model, and then artificially synthesize 150,000…
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