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LensExtractor: A Convolutional Neural Network in Search of Strong Gravitational Lenses

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arxiv 1705.05857 v2 pith:6SWMF6BE submitted 2017-05-16 astro-ph.IM astro-ph.GA

classification astro-ph.IMastro-ph.GA
keywords algorithmgravitationallensconvolutionallensextractorstrongcandidatesevents
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In this work, we present our classification algorithm to identify strong gravitational lenses from wide-area surveys using machine learning convolutional neural network; LensExtractor. We train and test the algorithm using a wide variety of strong gravitational lens configurations from simulations of lensing events. Images are processed through multiple convolutional layers which extract feature maps necessary to assign a lens probability to each image. LensExtractor provides a ranking scheme for all sources which could be used to identify potential gravitational lens candidates significantly reducing the number of images that have to be visually inspected. We further apply our algorithm to the \textit{HST}/ACS i-band observations of the COSMOS field and present our sample of identified lensing candidates. The developed machine learning algorithm is much more computationally efficient than classical lens identification algorithms and is ideal for discovering such events across wide areas from current and future surveys such as LSST and WFIRST.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 71 citations worldwide. Full citation record

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    astro-ph.GA 2026-06 unverdicted novelty 7.0 of 10

    JWST spectra of six z=5-9 galaxies show low-ionization covering fractions of 0.2-0.9 and diverse kinematics including blueshifted outflows, indicating heterogeneous multiphase ISM.

  2. Detecting Modeling Bias with Continuous Time Flow Models on Weak Lensing Maps

    astro-ph.CO 2025-05 conditional novelty 6.0 of 10

    Continuous time flow models estimating full-field probability densities detect out-of-distribution weak lensing maps from baryonic effects with AUROC up to 0.95, outperforming feature-level normalizing flow baselines.

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