Hubble Asteroid Hunter: II. Identifying strong gravitational lenses in HST images with crowdsourcing
arXiv:2207.06997 · doi:10.1051/0004-6361/202243745
Abstract
The Hubble Space Telescope (HST) archives constitute a rich dataset of high resolution images to mine for strong gravitational lenses. While many HST programs specifically target strong lenses, they can also be present by coincidence in other HST observations. We aim to identify non-targeted strong gravitational lenses in almost two decades of images from the ESA it Hubble Space Telescope archive (eHST), without any prior selection on the lens properties. We used crowdsourcing on the Hubble Asteroid Hunter (HAH) citizen science project to identify strong lenses, alongside asteroid trails, in publicly available large field-of-view HST images. We visually inspected 2354 objects tagged by citizen scientists as strong lenses to clean the sample and identify the genuine lenses. We report the detection of 252 strong gravitational lens candidates, which were not the primary targets of the HST observations. 198 of them are new, not previously reported by other studies, consisting of 45 A grades, 74 B grades and 79 C grades. The majority are galaxy-galaxy configurations. The newly detected lenses are, on average, 1.3 magnitudes fainter than previous HST searches. This sample of strong lenses with high resolution HST imaging is ideal to follow-up with spectroscopy, for lens modelling and scientific analyses. This paper presents an unbiased search of lenses, which enabled us to find a high variety of lens configurations, including exotic lenses. We demonstrate the power of crowdsourcing in visually identifying strong lenses and the benefits of exploring large archival datasets. This study shows the potential of using crowdsourcing in combination with artificial intelligence for the detection and validation of strong lenses in future large-scale surveys such as ESA's future mission Euclid or in JWST archival images.
24 page, 14 figures, 5 tables, accepted for publication in A&A June 28 2022
References in corpus (40)
- The Cosmic Evolution Survey (COSMOS) -- Overview
- Rotation-invariant convolutional neural networks for galaxy morphology prediction
- The Sloan Lens ACS Survey. V. The Full ACS Strong-Lens Sample
- Multiple Images of a Highly Magnified Supernova Formed by an Early-Type Cluster Galaxy Lens
- Bayesian Strong Gravitational-Lens Modeling on Adaptive Grids: Objective Detection of Mass Substructure in Galaxies
- Hubble Space Telescope Combined Strong and Weak Lensing Analysis of the CLASH Sample: Mass and Magnification Models and Systematic Uncertainties
- The Sloan Lens ACS Survey. VI: Discovery and analysis of a double Einstein ring
- The CFHTLS Strong Lensing Legacy Survey: I. Survey overview and T0002 release sample
- Photometric redshift estimation via deep learning
- The SL2S Galaxy-scale Lens Sample. V. Dark Matter Halos and Stellar IMF of Massive Early-type Galaxies out to Redshift 0.8
- First catalog of strong lens candidates in the COSMOS field
- A Highly Magnified Star at Redshift 6.2
- RingFinder: automated detection of galaxy-scale gravitational lenses in ground-based multi-filter imaging data
- COSMOGRAIL XVI: Time delays for the quadruply imaged quasar DES J0408-5354 with high-cadence photometric monitoring
- LinKS: Discovering galaxy-scale strong lenses in the Kilo-Degree Survey using Convolutional Neural Networks
- The Sloan Lens ACS Survey. XIII. Discovery of 40 New Galaxy-Scale Strong Lenses
- Small scatter and nearly-isothermal mass profiles to four half-light radii from two-dimensional stellar dynamics of early-type galaxies
- Molecular gas content in strongly-lensed z~1.5-3 star-forming galaxies with low IR luminosities
- A very bright, highly magnified Lyman-break galaxy at z=3.07
- Super-resolving distant galaxies with gravitational telescopes: Keck-LGSAO and Hubble imaging of the lens system SDSSJ0737+3216
- Two New Large Separation Gravitational Lenses from SDSS
- The MUSE Deep Lensed Field on the Hubble Frontier Field MACS~J0416
- Gravitational lenses and lens candidates identified from the COSMOS field
- Galaxy Clusters from the DESI Legacy Imaging Surveys. I. Cluster Detection
- A Strong-Lens Survey in AEGIS: the influence of large scale structure
- MUSE observations of the lensing cluster SMACSJ2031.8-4036: new constraints on the mass distribution in the cluster core
- The Grism Lens-Amplified Survey from Space (GLASS). IX. The dual origin of low-mass cluster galaxies as revealed by new structural analyses
- A Neural Network Gravitational Arc Finder based on the Mediatrix filamentation Method
- Early-type galaxy density profiles from IllustrisTNG: II. Evolutionary trend of the total density profile
- A Spectroscopically Confirmed Double Source Plane Lens System in the Hyper Suprime-Cam Subaru Strategic Program
- Gravitational lens candidates in the E-CDFS
- Hubble Asteroid Hunter: I. Identifying asteroid trails in Hubble Space Telescope images
- Total mass density slopes of early-type galaxies using Jeans dynamical modelling at redshifts
- A twelve-image gravitational lens system in the z ~ 0.84 cluster Cl J0152.7-1357
- Galaxy And Mass Assembly (GAMA) Blended Spectra Catalog: Strong Galaxy-Galaxy Lens and Occulting Galaxy Pair Candidates
- J0454-0309: Evidence for a strong lensing fossil group falling into a poor galaxy cluster
- Gravitational lens modelling in a citizen science context
- A new Einstein Cross gravitational lens of a Lyman-break galaxy
- Photo- with CuBAN: An improved photometric redshift estimator using Clustering aided Back Propagation Neural network
- The Orthogonally Aligned Dark Halo of an Edge-on Lensing Galaxy in the Hubble Frontier Fields: A Challenge for Modified Gravity