An extended catalog of galaxy-galaxy strong gravitational lenses discovered in DES using convolutional neural networks
arXiv:1905.10522 · doi:10.3847/1538-4365/ab26b6
Abstract
We search Dark Energy Survey (DES) Year 3 imaging for galaxy-galaxy strong gravitational lenses using convolutional neural networks, extending previous work with new training sets and covering a wider range of redshifts and colors. We train two neural networks using images of simulated lenses, then use them to score postage stamp images of 7.9 million sources from the Dark Energy Survey chosen to have plausible lens colors based on simulations. We examine 1175 of the highest-scored candidates and identify 152 probable or definite lenses. Examining an additional 20,000 images with lower scores, we identify a further 247 probable or definite candidates. After including 86 candidates discovered in earlier searches using neural networks and 26 candidates discovered through visual inspection of blue-near-red objects in the DES catalog, we present a catalog of 511 lens candidates.
arXiv commentAccepted for publication in ApJ Supplement Series
References in corpus (61)
- Deep Learning in Neural Networks: An Overview
- COSMOS Photometric Redshifts with 30-bands for 2-deg2
- The Dark Energy Survey: more than dark energy - an overview
- Cluster Lensing And Supernova survey with Hubble (CLASH): An Overview
- Rotation-invariant convolutional neural networks for galaxy morphology prediction
- redMaPPer I: Algorithm and SDSS DR8 Catalog
- Galaxy Clusters Discovered via the Sunyaev-Zel'dovich Effect in the 2500-square-degree SPT-SZ survey
- The Dark Energy Survey Data Release 1
- Strong Lensing by Galaxies
- Stellar Population Diagnostics of Elliptical Galaxy Formation
- The population of galaxy-galaxy strong lenses in forthcoming optical imaging surveys
- The first and second data releases of the Kilo-Degree Survey
- Fast Automated Analysis of Strong Gravitational Lenses with Convolutional Neural Networks
- The Formation of Massive, Compact Galaxies at z=2 in the Illustris Simulation
- The Dark Energy Survey Image Processing Pipeline
- The SL2S Galaxy-scale Lens Sample. IV. The dependence of the total mass density profile of early-type galaxies on redshift, stellar mass, and size
- Star-galaxy Classification Using Deep Convolutional Neural Networks
- redMaGiC: Selecting Luminous Red Galaxies from the DES Science Verification Data
- The Sloan Lens ACS Survey. VI: Discovery and analysis of a double Einstein ring
- Inference of the Cold Dark Matter substructure mass function at z=0.2 using strong gravitational lenses
- CMU DeepLens: Deep Learning For Automatic Image-based Galaxy-Galaxy Strong Lens Finding
- Finding Strong Gravitational Lenses in the Kilo Degree Survey with Convolutional Neural Networks
- The CFHTLS Strong Lensing Legacy Survey: I. Survey overview and T0002 release sample
- The CFHTLS-Strong Lensing Legacy Survey (SL2S): Investigating the group-scale lenses with the SARCS sample
- The luminosity and stellar mass Fundamental Plane of early-type galaxies
- Cosmological Constraints from the double source plane lens SDSSJ0946+1006
- Finding strong lenses in CFHTLS using convolutional neural networks
- Galaxy Morphology Classification with Deep Convolutional Neural Networks
- RingFinder: automated detection of galaxy-scale gravitational lenses in ground-based multi-filter imaging data
- The Co-Evolution of Total Density Profiles and Central Dark Matter Fractions in Simulated Early-Type Galaxies
- Modelling the line-of-sight contribution in substructure lensing
- Space Warps: I. Crowd-sourcing the Discovery of Gravitational Lenses
- Space Warps II. New Gravitational Lens Candidates from the CFHTLS Discovered through Citizen Science
- LinKS: Discovering galaxy-scale strong lenses in the Kilo-Degree Survey using Convolutional Neural Networks
- Statistics of mass substructure from strong gravitational lensing: quantifying the mass fraction and mass function
- Survey of Gravitationally-lensed Objects in HSC Imaging (SuGOHI). I. Automatic search for galaxy-scale strong lenses
- Finding high-redshift strong lenses in DES using convolutional neural networks
- The CASSOWARY spectroscopy survey: A new sample of gravitationally lensed galaxies in SDSS
- The SAMI Galaxy Survey: Exploring the gas-phase Mass-Metallicity Relation
- Transfer learning for galaxy morphology from one survey to another
- Constraints on the identity of the dark matter from strong gravitational lenses
- Automated detection of galaxy-scale gravitational lenses in high resolution imaging data
- Survey of Gravitationally-lensed Objects in HSC Imaging (SuGOHI). II. Environments and Line-of-Sight Structure of Strong Gravitational Lens Galaxies to z ~ 0.8
- Quantifying dwarf satellites through gravitational imaging: the case of SDSS J120602.09+514229.5
- Computational Methods for Gravitational Lensing
- The Blanco Cosmology Survey: An Optically-Selected Galaxy Cluster Catalog and a Public Release of Optical Data Products
- A large sample of shear selected clusters from the Hyper Suprime-Cam Subaru Strategic Program S16A wide field mass maps
- SPT-GMOS: A Gemini/GMOS-South Spectroscopic Survey of Galaxy Clusters in the SPT-SZ Survey
- The SLUGGS Survey: A comparison of total-mass profiles of early-type galaxies from observations and cosmological simulations, to 4 effective radii
- Broadband Photometry of 105 Giant Arcs: Redshift Constraints and Implications for Giant Arc Statistics
- QuasarNET: Human-level spectral classification and redshifting with Deep Neural Networks
- CHITAH: Strong-gravitational-lens hunter in imaging surveys
- Southern Cosmology Survey II: Massive Optically-Selected Clusters from 70 square degrees of the SZE Common Survey Area
- Discovery of the Lensed Quasar System DES J0408-5354
- Observation and Confirmation of Six Strong Lensing Systems in The Dark Energy Survey Science Verification Data
- The PAU Survey: star-galaxy classification with multi narrow-band data
- A Spectroscopically Confirmed Double Source Plane Lens System in the Hyper Suprime-Cam Subaru Strategic Program
- The serendipitous observation of a gravitationally lensed galaxy at z = 0.9057 from the Blanco Cosmology Survey: The Elliot Arc
- The evolution of late-type galaxies from CASSOWARY lensing systems
- The Canarias Einstein Ring: a Newly Discovered Optical Einstein Ring
- The SOAR Gravitational Arc Survey - I: Survey overview and photometric catalogs
Cited by in corpus (11)
- The SPTpol Extended Cluster Survey
- Dark matter halos of massive elliptical galaxies at are well described by the Navarro-Frenk-White profile
- Discovering New Strong Gravitational Lenses in the DESI Legacy Imaging Surveys
- Convolutional neural network identification of galaxy post-mergers in UNIONS using IllustrisTNG
- New high-quality strong lens candidates with deep learning in the Kilo Degree Survey
- Survey of Gravitationally-lensed Objects in HSC Imaging (SuGOHI). V. Group-to-cluster scale lens search from the HSC-SSP Survey
- Deep Learning for Strong Lensing Search: Tests of the Convolutional Neural Networks and New Candidates from KiDS DR3
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: A Catalogue of Strong Galaxy-Galaxy Lens Candidates
- Strong lens modelling: comparing and combining Bayesian neural networks and parametric profile fitting
- The Observable Supernova Rate in Galaxy-Galaxy Lensing Systems with the TESS Satellite
- Core Mass Estimates in Strong Lensing Galaxy Clusters Using a Single-Halo Lens Model