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0957 + 561 A, B: twin quasistellar objects or gravitational lens?
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Two Accurate Time-Delay Distances from Strong Lensing: Implications for Cosmology
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Dark Energy Survey Year 3 Results: Photometric Data Set for Cosmology
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January 2019 |
Low-mass halo perturbations in strong gravitational lenses at redshift z ∼ 0.5 are consistent with CDM
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THE PHYSICAL CONDITIONS, METALLICITY AND METAL ABUNDANCE RATIOS IN A HIGHLY MAGNIFIED GALAXY AT z = 3.6252
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Ringfinder: Automated Detection of Galaxy-Scale Gravitational Lenses in Ground-Based Multi-Filter Imaging data
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April 2014 |
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Star Formation at z = 2.481 in the Lensed Galaxy SDSS J1110+6459: Star Formation Down to 30 pc Scales
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July 2017 |
On the Possibility of Determining Hubble's Parameter and the Masses of Galaxies from the Gravitational Lens Effect
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Mining for Strong Gravitational Lenses with Self-supervised Learning
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The BOSS Emission-line Lens Survey. V. Morphology and Substructure of Lensed Ly α Emitters at Redshift Z ≈ 2.5 in the BELLS GALLERY
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April 2020 |
The Dark Energy Survey Image Processing Pipeline
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The strong gravitational lens finding challenge
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Hubble Asteroid Hunter
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Revealing the Properties of Dark Matter in the Merging Cluster MACS J0025.4−1222
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Gaia GraL: Gaia DR2 Gravitational Lens Systems: III. A systematic blind search for new lensed systems
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February 2019 |
Is every strong lens model unhappy in its own way? Uniform modelling of a sample of 13 quadruply+ imaged quasars
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December 2018 |
DES meets Gaia: discovery of strongly lensed quasars from a multiplet search
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June 2018 |
Survey of Gravitationally-lensed Objects in HSC Imaging (SuGOHI). I. Automatic search for galaxy-scale strong lenses
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Strong gravitational lensing and the stellar IMF of early-type galaxies
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April 2016 |
Data mining for gravitationally lensed quasars
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The Sloan Lens ACS Survey. III. The Structure and Formation of Early‐Type Galaxies and Their Evolution since z ≈ 1
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The Internal Structure and Formation of Early‐Type Galaxies: The Gravitational Lens System MG 2016+112 at z = 1.004
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Discovery of two gravitationally lensed quasars in the Dark Energy Survey
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HOLISMOKES: I. Highly Optimised Lensing Investigations of Supernovae, Microlensing Objects, and Kinematics of Ellipticals and Spirals
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December 2020 |
Lensing substructure quantification in RXJ1131-1231: a 2 keV lower bound on dark matter thermal relic mass
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May 2017 |
Search of strong lens systems in the Dark Energy Survey using convolutional neural networks
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December 2022 |
HOW TO FIND GRAVITATIONALLY LENSED TYPE Ia SUPERNOVAE
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December 2016 |
Planck 2018 results: VI. Cosmological parameters
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Fast automated analysis of strong gravitational lenses with convolutional neural networks
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August 2017 |
Observation and Confirmation of six Strong-Lensing Systems in the dark Energy Survey Science Verification data
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Giant luminous arcs discovered in two clusters of galaxies
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February 1987 |
Discovery of the First Quadruple Gravitationally Lensed Quasar Candidate with Pan-STARRS
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July 2017 |
The luminosity and stellar mass Fundamental Plane of early-type galaxies
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June 2009 |
TDCOSMO: I. An exploration of systematic uncertainties in the inference of H 0 from time-delay cosmography
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July 2020 |
An Extended Catalog of Galaxy–Galaxy Strong Gravitational Lenses Discovered in DES Using Convolutional Neural Networks
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July 2019 |
Resolved spectroscopy of gravitationally lensed galaxies: global dynamics and star-forming clumps on ∼100 pc scales at 1 < z < 4
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April 2015 |
H0LiCOW – XIII. A 2.4 per cent measurement of H0 from lensed quasars: 5.3σ tension between early- and late-Universe probes
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September 2019 |
Overview of the DESI Legacy Imaging Surveys
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April 2019 |
Two new large-separation gravitational lenses from SDSS
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January 2009 |
Finding strong gravitational lenses in the Kilo Degree Survey with Convolutional Neural Networks
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August 2017 |
Quasar lenses in the south: searches over the DES public footprint
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August 2019 |
The boss Emission-Line lens Survey. iv. Smooth lens Models for the Bells Gallery Sample
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December 2016 |
Gradient-based learning applied to document recognition
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January 1998 |
Detection of a dark substructure through gravitational imaging: Detection of a dark substructure
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Survey of gravitationally-lensed objects in HSC imaging (SuGOHI): III. Statistical strong lensing constraints on the stellar IMF of CMASS galaxies
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September 2019 |
The Sloan Lens ACS Survey. I. A Large Spectroscopically Selected Sample of Massive Early‐Type Lens Galaxies
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February 2006 |
Developing a victorious strategy to the second strong gravitational lensing data challenge
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July 2022 |
Finding Strong Gravitational Lenses in the DESI DECam Legacy Survey
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May 2020 |
Two-dimensional kinematics of SLACS lenses - III. Mass structure and dynamics of early-type lens galaxies beyond z ≃ 0.1: 2D kinematics of SLACS lenses - III
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May 2011 |
Photometric Redshifts and Galaxy Clusters for DES DR2, DESI DR9, and HSC-SSP PDR3 Data
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May 2022 |
Lensing clusters of galaxies in the SDSS-III
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September 2011 |
The Sloan Lens ACS Survey. XIII. Discovery of 40 New Galaxy-scale Strong Lenses
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December 2017 |
New High-quality Strong Lens Candidates with Deep Learning in the Kilo-Degree Survey
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August 2020 |
GalSim: The modular galaxy image simulation toolkit
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April 2015 |
HOLISMOKES: VI. New galaxy-scale strong lens candidates from the HSC-SSP imaging survey
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September 2021 |
The CFHTLS strong lensing legacy survey: I. Survey overview and T0002 release sample
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October 2006 |
Clash-Vlt: Insights on the mass Substructures in the Frontier Fields Cluster macs J0416.1–2403 Through Accurate Strong lens Modeling
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February 2015 |
The Dark Energy Survey Data Release 2
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July 2021 |
Calibration of the Tip of the Red Giant Branch
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March 2020 |
Alma Observations of Spt-Discovered, Strongly Lensed, Dusty, Star-Forming Galaxies
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April 2013 |
Gravitationally lensed quasars and supernovae in future wide-field optical imaging surveys: Lensed quasars and supernovae
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April 2010 |
TDCOSMO: IV. Hierarchical time-delay cosmography – joint inference of the Hubble constant and galaxy density profiles
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November 2020 |
STRIDES: automated uniform models for 30 quadruply imaged quasars
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November 2022 |
The CASSOWARY spectroscopy survey: a new sample of gravitationally lensed galaxies in SDSS
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October 2013 |
THE SLOAN BRIGHT ARCS SURVEY: FOUR STRONGLY LENSED GALAXIES WITH REDSHIFT > 2
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November 2009 |
Detection of Lensing Substructure Using alma Observations of the Dusty Galaxy Sdp.81
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May 2016 |
Gaia GraL: Gaia DR2 gravitational lens systems : I. New quadruply imaged quasar candidates around known quasars
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August 2018 |
Survey of Gravitationally-lensed Objects in HSC Imaging (SuGOHI): VI. Crowdsourced lens finding with Space Warps
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October 2020 |
Prediction of Supernova Rates in Known Galaxy–Galaxy Strong-lens Systems
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September 2018 |
H0LiCOW – I. H0 Lenses in COSMOGRAIL's Wellspring: program overview
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February 2017 |
The dark Energy Camera
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October 2015 |
Photometric redshifts from SDSS images using a convolutional neural network
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December 2018 |
DISCOVERY OF A VERY BRIGHT, STRONGLY LENSED z = 2 GALAXY IN THE SDSS DR5
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June 2009 |
X‐Ray and Optical Microlensing in the Lensed Quasar PG 1115+080
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December 2008 |
Galaxy structure with strong gravitational lensing: decomposing the internal mass distribution of massive elliptical galaxies
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August 2019 |
Double source lensing probing high redshift cosmology
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July 2022 |
Gravitational detection of a low-mass dark satellite galaxy at cosmological distance
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January 2012 |
The Dark Energy Survey Bright Arcs Survey: Candidate Strongly Lensed Galaxy Systems from the Dark Energy Survey 5000 Square Degree Footprint
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March 2022 |
Two-dimensional kinematics of SLACS lenses - I. Phase-space analysis of the early-type galaxy SDSS J2321−097 at z ≈ 0.1 ★
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March 2008 |
The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch
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August 2019 |
HOLISMOKES: II. Identifying galaxy-scale strong gravitational lenses in Pan-STARRS using convolutional neural networks
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December 2020 |
Gaia GraL: Gaia DR2 Gravitational Lens Systems. VI. Spectroscopic Confirmation and Modeling of Quadruply Imaged Lensed Quasars
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October 2021 |
Probing the nature of dark matter by forward modelling flux ratios in strong gravitational lenses
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August 2018 |
Discovering New Strong Gravitational Lenses in the DESI Legacy Imaging Surveys
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March 2021 |
Time delay cosmography
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Precise Time Delays from Strongly Gravitationally Lensed Type Ia Supernovae with Chromatically Microlensed Images
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March 2018 |
Dissecting the Gravitational lens B1608+656. ii. Precision Measurements of the Hubble Constant, Spatial Curvature, and the dark Energy Equation of State
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The 8 O'Clock Arc: A Serendipitous Discovery of a Strongly Lensed Lyman Break Galaxy in the SDSS DR4 Imaging Data
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May 2007 |
Statistics of mass substructure from strong gravitational lensing: quantifying the mass fraction and mass function
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The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: a catalogue of strong galaxy–galaxy lens candidates
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February 2021 |
Survey of Gravitationally Lensed Objects in HSC Imaging (SuGOHI) – VII. Discovery and confirmation of three strongly lensed quasars†
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January 2021 |
Finding high-redshift strong lenses in DES using convolutional neural networks
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January 2019 |
Space Warps– II. New gravitational lens candidates from the CFHTLS discovered through citizen science
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Extending the SAGA Survey (xSAGA). I. Satellite Radial Profiles as a Function of Host-galaxy Properties
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Substructure detection reanalysed: dark perturber shown to be a line-of-sight halo
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Rotation-invariant convolutional neural networks for galaxy morphology prediction
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April 2015 |
Giant star-forming clumps?
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March 2020 |
deeplenstronomy: A dataset simulation package for strong gravitational lensing
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THE SLOAN BRIGHT ARCS SURVEY: DISCOVERY OF SEVEN NEW STRONGLY LENSED GALAXIES FROM z = 0.66-2.94
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The Sloan Lens ACS Survey. V. The Full ACS Strong‐Lens Sample
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Even Simpler Modeling of Quadruply Lensed Quasars (and Random Quartets) Using Witt's Hyperbola
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April 2019 |
COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses: XIII. Time delays and 9-yr optical monitoring of the lensed quasar RX J1131−1231
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Gravitationally lensed quasars in Gaia – III. 22 new lensed quasars from Gaia data release 2
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The image separation distribution of strong lenses: halo versus subhalo populations
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STRIDES: a 3.9 per cent measurement of the Hubble constant from the strong lens system DES J0408−5354
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March 2020 |
Spatial Variation in Strong Line Ratios and Physical Conditions in Two Strongly Lensed Galaxies at z ∼ 1.4
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COSMOS PHOTOMETRIC REDSHIFTS WITH 30-BANDS FOR 2-deg 2
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Resolving on 100 pc scales the UV-continuum in Lyman-α emitters between redshift 2 and 3 with gravitational lensing
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TDCOSMO: V. Strategies for precise and accurate measurements of the Hubble constant with strong lensing
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The DES Bright Arcs Survey: Hundreds of Candidate Strongly Lensed Galaxy Systems from the Dark Energy Survey Science Verification and Year 1 Observations
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HOLISMOKES: III. Achromatic phase of strongly lensed Type Ia supernovae
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A neural network gravitational arc finder based on the Mediatrix filamentation method
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LSST: From Science Drivers to Reference Design and Anticipated Data Products
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COOL-LAMPS. I. An Extraordinarily Bright Lensed Galaxy at Redshift 5.04
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External Shear in Quadruply Imaged Lens Systems
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SHARP – VII. New constraints on the dark matter free-streaming properties and substructure abundance from gravitationally lensed quasars
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Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with ΛCDM
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Survey of Gravitationally lensed Objects in HSC Imaging (SuGOHI): IV. Lensed quasar search in the HSC survey
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THE SLOAN BRIGHT ARCS SURVEY: SIX STRONGLY LENSED GALAXIES AT z = 0.4-1.4
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A Systematic Search for High Surface Brightness Giant Arcs in a Sloan Digital Sky Survey Cluster Sample
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Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond ΛCDM
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The implications of lenses for galaxy structure
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What are the environments of lens galaxies?
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The Cfhtls-Strong Lensing Legacy Survey (Sl2s): Investigating the Group-Scale Lenses with the Sarcs Sample
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