HOLISMOKES. VIII. High-redshift, strong-lens search in the Hyper Suprime-Cam Subaru Strategic Program
arXiv:2201.11135 · doi:10.1051/0004-6361/202243203
Abstract
We carry out a search for strong-lens systems containing high-redshift lens galaxies with the goal of extending strong-lensing-assisted galaxy evolutionary studies to earlier cosmic time. Two strong-lens classifiers are constructed from a deep residual network and trained with datasets of different lens-redshift and brightness distributions. We classify a sample of 5,356,628 pre-selected objects from the Wide-layer fields in the second public data release of the Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) by applying the two classifiers to their HSC -filter cutouts. Cutting off at thresholds that correspond to a false positive rate of on our test set, the two classifiers identify 5,468 and 6,119 strong-lens candidates. Visually inspecting the cutouts of those candidates results in 735 grade-A or B strong-lens candidates in total, of which 277 candidates are discovered for the first time. This is the single largest set of galaxy-scale strong-lens candidates discovered with HSC data to date, and nearly half of it (331/735) contains lens galaxies with photometric redshifts above 0.6. Our discoveries will serve as a valuable target list for ongoing and scheduled spectroscopic surveys such as the Dark Energy Spectroscopic Instrument, the Subaru Prime Focus Spectrograph project, and the Maunakea Spectroscopic Explorer.
arXiv comment15 pages, 8 figures + appendices, published on the A&A
References in corpus (106)
- The Seventh Data Release of the Sloan Digital Sky Survey
- LSST: from Science Drivers to Reference Design and Anticipated Data Products
- The Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III
- The Baryon Oscillation Spectroscopic Survey of SDSS-III
- Overview of the DESI Legacy Imaging Surveys
- The Sixteenth Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra
- The DESI Experiment Part I: Science,Targeting, and Survey Design
- H0LiCOW XIII. A 2.4% measurement of from lensed quasars: tension between early and late-Universe probes
- Extragalactic Science, Cosmology and Galactic Archaeology with the Subaru Prime Focus Spectrograph (PFS)
- The Fourteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the extended Baryon Oscillation Spectroscopic Survey and from the second phase of the Apache Point Observatory Galactic Evolution Experiment
- Spectral Classification and Redshift Measurement for the SDSS-III Baryon Oscillation Spectroscopic Survey
- The Sloan Lens ACS Survey. III - The Structure and Formation of Early-type Galaxies and their Evolution since z~1
- Second Data Release of the Hyper Suprime-Cam Subaru Strategic Program
- The Hyper Suprime-Cam Software Pipeline
- H0LiCOW V. New COSMOGRAIL time delays of HE0435-1223: to 3.8% precision from strong lensing in a flat CDM model
- Strong Lensing by Galaxies
- The Sloan Lens ACS Survey. V. The Full ACS Strong-Lens Sample
- Dissecting the Gravitational Lens B1608+656. II. Precision Measurements of the Hubble Constant, Spatial Curvature, and the Dark Energy Equation of State
- Gravitational detection of a low-mass dark satellite at cosmological distance
- Two accurate time-delay distances from strong lensing: Implications for cosmology
- H0LiCOW I. Lenses in COSMOGRAIL's Wellspring: Program Overview
- The population of galaxy-galaxy strong lenses in forthcoming optical imaging surveys
- The Cosmic Lens All-Sky Survey:II. Gravitational lens candidate selection and follow-up
- Photometric Redshifts for Hyper Suprime-Cam Subaru Strategic Program Data Release 1
- Detection of lensing substructure using ALMA observations of the dusty galaxy SDP.81
- The Dark Energy Survey Data Release 2
- Detection of a Dark Substructure through Gravitational Imaging
- The Sloan-Lens ACS Survey II: stellar populations and internal structure of early-type lens galaxies
- Spectroscopic detection of CIV in a galaxy at z=7.045: Implications for the ionizing spectra of reionization-era galaxies
- TDCOSMO. I. An exploration of systematic uncertainties in the inference of from time-delay cosmography
- Dark Matter Contraction and the Stellar Content of Massive Early-type Galaxies: Disfavoring "Light" Initial Mass Functions
- Gravitational Lens Models Based on Submillimeter Array Imaging of Herschel-selected Strongly Lensed Sub-millimeter Galaxies at z>1.5
- Identity Mappings in Deep Residual Networks
- CMU DeepLens: Deep Learning For Automatic Image-based Galaxy-Galaxy Strong Lens Finding
- The BOSS Emission-Line Lens Survey (BELLS). I. A large spectroscopically selected sample of Lens Galaxies at redshift ~ 0.5
- The Halos of Satellite Galaxies: the Companion of the Massive Elliptical Lens SL2S J08544-0121
- The MUSE Hubble Ultra Deep Field Survey: II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxies
- The CFHTLS-Strong Lensing Legacy Survey (SL2S): Investigating the group-scale lenses with the SARCS sample
- Disentangling Baryons and Dark Matter in the Spiral Gravitational Lens B1933+503
- The Strong Gravitational Lens Finding Challenge
- The BOSS Emission-Line Lens Survey. II. Investigating Mass-Density Profile Evolution in the SLACS+BELLS Strong Gravitational Lens Sample
- Detection of substructure with adaptive optics integral field spectroscopy of the gravitational lens B1422+231
- Finding strong lenses in CFHTLS using convolutional neural networks
- The SL2S Galaxy-scale Lens Sample. III. Lens Models, Surface Photometry and Stellar Masses for the final sample
- Space Warps II. New Gravitational Lens Candidates from the CFHTLS Discovered through Citizen Science
- Gravitationally Lensed Quasars in Gaia: II. Discovery of 24 Lensed Quasars
- LinKS: Discovering galaxy-scale strong lenses in the Kilo-Degree Survey using Convolutional Neural Networks
- The SDSS-IV extended Baryonic Oscillation Spectroscopic Survey: Luminous Red Galaxy Target Selection
- The Sloan Lens ACS Survey. XIII. Discovery of 40 New Galaxy-Scale Strong Lenses
- 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 Sloan Lens ACS Survey. XII. Extending Strong Lensing to Lower Masses
- The CASSOWARY spectroscopy survey: A new sample of gravitationally lensed galaxies in SDSS
- The Low Mass End of the Fundamental Relation for Gravitationally Lensed Star Forming Galaxies at 1<z<6
- The BOSS Emission-Line Lens Survey. IV. : Smooth Lens Models for the BELLS GALLERY Sample
- Finding Strong Gravitational Lenses in the DESI DECam Legacy Survey
- Sloan Digital Sky Survey Spectroscopic Lens Search. I. Discovery of Intermediate-Redshift Star-Forming Galaxies Behind Foreground Luminous Red Galaxies
- Measuring the value of the Hubble constant "à la Refsdal"
- Discovering New Strong Gravitational Lenses in the DESI Legacy Imaging Surveys
- Gravitational lens time delays for distant supernovae: break the degeneracy between radial mass profiles and the Hubble constant
- The Effect of Environment on Shear in Strong Gravitational Lenses
- The SWELLS Survey. I. A large spectroscopically selected sample of edge-on late-type lens galaxies
- HOLISMOKES -- II. Identifying galaxy-scale strong gravitational lenses in Pan-STARRS using convolutional neural networks
- New high-quality strong lens candidates with deep learning in the Kilo Degree Survey
- How to Find Gravitationally Lensed Type Ia Supernovae
- The BOSS Emission-Line Lens Survey. III. : Strong Lensing of Ly Emitters by Individual Galaxies
- 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
- Catalogues of Active Galactic Nuclei From Gaia and unWISE Data
- Substructure in the lens HE 0435-1223
- Survey of Gravitationally-lensed Objects in HSC Imaging (SuGOHI). VI. Crowdsourced lens finding with Space Warps
- Magnified or multiply imaged? - Search strategies for gravitationally lensed supernovae in wide-field surveys
- HOLISMOKES -- I. Highly Optimised Lensing Investigations of Supernovae, Microlensing Objects, and Kinematics of Ellipticals and Spirals
- Photometric Redshift Estimation with a Convolutional Neural Network: NetZ
- High-quality strong lens candidates in the final Kilo Degree survey footprint
- HOLISMOKES. VI. New galaxy-scale strong lens candidates from the HSC-SSP imaging survey
- Survey of Gravitationally-lensed Objects in HSC Imaging (SuGOHI). V. Group-to-cluster scale lens search from the HSC-SSP Survey
- Improved time-delay lens modelling and inference with transient sources
- Survey of Gravitationally-lensed Objects in HSC Imaging (SuGOHI). IV. Lensed quasar search in the HSC survey
- Red nuggets grow inside-out: evidence from gravitational lensing
- On building a cluster watch-list for identifying strongly lensed supernovae, gravitational waves and kilonovae
- HOLISMOKES -- IV. Efficient mass modeling of strong lenses through deep learning
- ALMA Imprint of Intergalactic Dark Structures in the Gravitational Lens SDP.81
- On the evolution of environmental and mass properties of strong lens galaxies in COSMOS
- Evolution of The Velocity-Dispersion Function of Luminous Red Galaxies: A Hierarchical Bayesian Measurement
- The Detailed Science Case for the Maunakea Spectroscopic Explorer, 2019 edition
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: A Catalogue of Strong Galaxy-Galaxy Lens Candidates
- HOLISMOKES -- III. Achromatic Phase of Strongly Lensed Type Ia Supernovae
- A new quadruple gravitational lens from the Hyper Suprime-Cam Survey: the puzzle of HSC~J115252+004733
- Prediction of Supernova Rates in Known Galaxy-galaxy Strong-lens Systems
- SDSS J09094449: A Large-separation Strongly Lensed Quasar at with Three Images
- Kiloparsec Mass/Light Offsets in the Galaxy Pair-Ly Emitter Lens System SDSS\,J10110143
- Discovery of a Strong Lensing Galaxy Embedded in a Cluster at z = 1.62
- A census of optically dark massive galaxies in the early Universe from magnification by lensing galaxy clusters
- HOLISMOKES -- VII. Time-delay measurement of strongly lensed Type Ia supernovae using machine learning
- Planck's Dusty GEMS. III. A massive lensing galaxy with a bottom-heavy stellar initial mass function at z=1.5
- The SWELLS Survey. VI. hierarchical inference of the initial mass functions of bulges and discs
- Three QSOs acting as strong gravitational lenses
- Rest-frame UV Properties of Luminous Strong Gravitationally Lensed Ly Emitters from the BELLS GALLERY Survey
- New "Einstein Cross" Gravitational Lens Candidates in HST WFPC2 Survey Images
- HOLISMOKES -- V. Microlensing of type II supernovae and time-delay inference through spectroscopic phase retrieval
- A Gravitationally Lensed Quasar Discovered in OGLE
- Discovery of a Very Bright and Intrinsically Very Luminous, Strongly Lensed Lyα Emitting Galaxy at z = 2.82 in the BOSS Emission-Line Lens Survey
- Identifying lensed quasars and measuring their time-delays from unresolved light curves
- Discovering Strongly-lensed QSOs From Unresolved Light Curves
- Lensed quasar search via time variability with the HSC transient survey
- The Strong Gravitationally Lensed Herschel Galaxy HLock01: Optical Spectroscopy Reveals a Close Galaxy Merger with Evidence of Inflowing Gas
Cited by in corpus (24)
- Strong gravitational lensing and microlensing of supernovae
- Sensitivity of strong lensing observations to dark matter substructure: a case study with Euclid
- Survey of Gravitationally-lensed Objects in HSC Imaging (SuGOHI). VIII. New galaxy-scale lenses from the HSC SSP
- Streamlined Lensed Quasar Identification in Multiband Images via Ensemble Networks
- Identification of Galaxy-Galaxy Strong Lens Candidates in the DECam Local Volume Exploration Survey Using Machine Learning
- HOLISMOKES -- IX. Neural network inference of strong-lens parameters and uncertainties from ground-based images
- HOLISMOKES -- X. Comparison between neural network and semi-automated traditional modeling of strong lenses
- On the detectability of strong lensing in near-infrared surveys
- Euclid Preparation XXXIII. Characterization of convolutional neural networks for the identification of galaxy-galaxy strong lensing events
- HOLISMOKES -- XI. Evaluation of supervised neural networks for strong-lens searches in ground-based imaging surveys
- A Bayesian Approach to Strong Lens Finding in the Era of Wide-area Surveys
- TEGLIE: Transformer encoders as strong gravitational lens finders in KiDS
- Retrospective Search for Strongly Lensed Supernovae in the DESI Legacy Imaging Surveys
- HOLISMOKES XIII: Strong-lens candidates at all mass scales and their environments from the Hyper-Suprime Cam and deep learning
- Discovery of 19 strongly-lensed quasars, dual and projected quasars in DESI-LS
- Simulation-guided galaxy evolution inference: A case study with strong lensing galaxies
- HOLISMOKES XV. Search for strong gravitational lenses combining ground-based and space-based imaging
- The revolution in strong lensing discoveries from Euclid
- Searching for strong lensing by late-type galaxies in UNIONS
- HOLISMOKES XVI: Lens search in HSC-PDR3 with a neural network committee and post-processing for false-positive removal
- Accelerating lensed quasar discovery and modeling with physics-informed variational autoencoders
- A compact group lens modeled with GIGA-Lens: Enhanced inference for complex systems
- Detection of Unresolved Strongly Lensed Supernovae with 7-Dimensional Telescope
- Confirming HSC strong lens candidates with DESI Spectroscopy. I. Project overview and first results