Exotic Image Formation in Strong Gravitational Lensing by Clusters of Galaxies -- III: Statistics with HUDF
arXiv:2107.11955 · doi:10.1093/mnras/stac1080
Abstract
We study the image formation near point singularities (swallowtail and umbilics) in the simulated strongly lensed images of Hubble Ultra Deep Field (HUDF) by the Hubble Frontier Fields (HFF) clusters. In this work, we only consider nearly half of the brightest (a total of 5271) sources in the HUDF region. For every HFF cluster, we constructed 11 realizations of strongly lensed HUDF with an arbitrary translation of the cluster centre within the central region of HUDF and an arbitrary rotation. In each of these realizations, we visually identify the characteristic/exotic image formation corresponding to the different point singularities. We find that our current results are consistent with our earlier results based on different approaches. We also study time delay in these exotic image formations and compare it with typical five-image geometries. We find that the typical time delay in exotic image formations is an order of magnitude smaller than the typical time delay in a generic five-image geometry.
arXiv comment9 pages, 5 figures. Suppl. material available on request from authors. Comments welcome
References in corpus (84)
- LSST: from Science Drivers to Reference Design and Anticipated Data Products
- The Cosmic Evolution Survey (COSMOS) -- Overview
- The James Webb Space Telescope
- The Great Observatories Origins Deep Survey: Initial Results From Optical and Near-Infrared Imaging
- UV Luminosity Functions at redshifts z~4 to z~10: 10000 Galaxies from HST Legacy Fields
- The Hubble Ultra Deep Field
- The Evolution of the Galaxy Rest-Frame Ultraviolet Luminosity Function Over the First Two Billion Years
- A Bayesian approach to strong lensing modelling of galaxy clusters
- The Frontier Fields: Survey Design
- Weak Gravitational Lensing with COSMOS: Galaxy Selection and Shape Measurements
- Gravitationally lensed quasars and supernovae in future wide-field optical imaging surveys
- GEMS: Galaxy Evolution from Morphologies and SEDs
- New Determinations of the UV Luminosity Functions from z~9 to z~2 show a remarkable consistency with halo growth and a constant star formation efficiency
- CLASH: Three Strongly Lensed Images of a Candidate z ~ 11 Galaxy
- The population of galaxy-galaxy strong lenses in forthcoming optical imaging surveys
- The Mass Distribution of SDSS J1004+4112 Revisited
- Multiple Images of a Highly Magnified Supernova Formed by an Early-Type Cluster Galaxy Lens
- A Cosmic Variance Cookbook
- Weighing simulated galaxy clusters using lensing and X-ray
- ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Infrared Excess of UV-selected z=2-10 galaxies as a function of UV-continuum Slope and Stellar Mass
- Probing the Dawn of Galaxies at z~9-12: New Constraints from HUDF12/XDF and CANDELS Data
- Creation of cosmic structure in the complex galaxy cluster merger Abell 2744
- Cluster Lenses
- Time Delay Cosmography
- Mass and magnification maps for the Hubble Space Telescope Frontier Fields clusters: implications for high redshift studies
- The Extreme Faint End of the UV Luminosity Function at Through Gravitational Telescopes: a comprehensive assessment of strong lensing uncertainties
- The Frontier Fields Lens Modeling Comparison Project
- Lens models and magnification maps of the six Hubble Frontier Fields clusters
- RELICS: Reionization Lensing Cluster Survey
- CLASH: The enhanced lensing efficiency of the highly elongated merging cluster MACS J0416.1-2403
- Precise Strong Lensing Mass Modeling of Four Hubble Frontier Fields Clusters and a Sample of Magnified High-Redshift Galaxies
- CMU DeepLens: Deep Learning For Automatic Image-based Galaxy-Galaxy Strong Lens Finding
- The Halos of Satellite Galaxies: the Companion of the Massive Elliptical Lens SL2S J08544-0121
- UVUDF: Ultraviolet Through Near-infrared Catalog and Photometric Redshifts of Galaxies in the Hubble Ultra Deep Field
- The Wide Field Infrared Survey Telescope: 100 Hubbles for the 2020s
- Quantifying cosmic variance
- New redshift z ~ 9 galaxies in the Hubble Frontier Fields: Implications for early evolution of the UV luminosity density
- The ALMA Spectroscopic Survey in the HUDF: CO luminosity functions and the molecular gas content of galaxies through cosmic history
- The ALMA Spectroscopic Survey Large Program: The Infrared Excess of z=1.5-10 UV-selected Galaxies and the Implied High-Redshift Star Formation History
- Evolution of the Sizes of Galaxies over 7<z<12 Revealed by the 2012 Hubble Ultra Deep Field Campaign
- The Extraordinary Amount of Substructure in the Hubble Frontier Fields Cluster Abell 2744
- Hubble Frontier Fields : A High Precision Strong Lensing Analysis of Galaxy Cluster MACSJ0416.1-2403 using ~200 Multiple Images
- Combined reconstruction of weak and strong lensing data with WSLAP
- A refined mass distribution of the cluster MACS J0416.12403 from a new large set of spectroscopic multiply lensed sources
- A Weak-Lensing Mass Reconstruction of the Large-Scale Filament Feeding the Massive Galaxy Cluster MACSJ0717.5+3745
- Intracluster Light at the Frontier II: The Frontier Fields Clusters
- Non-parametric inversion of strong lensing systems
- The galaxy UV luminosity function at z ~ 2 - 4; new results on faint-end slope and the evolution of luminosity density
- Strong Lensing in Abell 1703: Constraints on the Slope of the Inner Dark Matter Distribution
- The UDF05 Follow-up of the HUDF: I. The Faint-End Slope of the Lyman-Break Galaxy Population at z~5
- Characterizing Intra-cluster light in the Hubble Frontier Fields
- Discovery of the largest known lensed images formed by a critically convergent lensing cluster
- Non-parametric mass reconstruction of A1689 from strong lensing data with SLAP
- Lens Models Under the Microscope: Comparison of Hubble Frontier Field Cluster Magnification Maps
- Predictions for deep galaxy surveys with JWST from CDM
- Fundamental physics with the Hubble Frontier Fields: constraining Dark Matter models with the abundance of extremely faint and distant galaxies
- Using Convolutional Neural Networks to identify Gravitational Lenses in Astronomical images
- Enabling Non-Parametric Strong Lensing Models to Derive Reliable Cluster Mass Distributions. WSLAP+
- The Grism Lens-Amplified Survey from Space (GLASS). VI. Comparing the Mass and Light in MACSJ0416.1-2403 using Frontier Field imaging and GLASS spectroscopy
- UVUDF: UV Luminosity Functions at the cosmic high-noon
- Star Formation History of the Hubble Ultra Deep Field: Comparison with the HDFN
- A Free-Form Lensing Grid Solution for A1689 with New Mutiple Images
- An Atlas of Predicted Exotic Gravitational Lenses
- Mass and Light of Abell 370: A Strong and Weak Lensing Analysis
- Detecting Dark Matter Cores in Galaxy Clusters with Strong Lensing
- PICS: Simulations of Strong Gravitational Lensing in Galaxy Clusters
- Mass profile decomposition of the Frontier Fields cluster MACS J0416-02403. Insights on the Dark-Matter inner profile
- A versatile tool for cluster lensing source reconstruction. I. methodology and illustration on sources in the Hubble Frontier Field Cluster MACS J0717.5+3745
- Evidence for the line of sight structure in the largest Hubble Frontier Field cluster, MACSJ0717.5+3745
- Systematic or Signal? How dark matter misalignments can bias strong lensing models of galaxy clusters
- Systematic vs. Statistical Uncertainties in Masses and Magnifications of the Hubble Frontier Fields
- Probability of magnification in the clusters
- Automated Lensing Learner: Automated Strong Lensing Identification with a Computer Vision Technique
- Sparse Lens Inversion Technique (SLIT): lens and source separability from linear inversion of the source reconstruction problem
- Flexion measurement in simulations of Hubble Space Telescope data
- Quantifying substructures in {\it Hubble Frontier Field} clusters: comparison with simulations
- Image simulations for gravitational lensing with SkyLens
- Extended lens reconstructions with Grale: exploiting time domain, substructural and weak-lensing information
- Lensing signals in the Hubble Ultra-Deep Field using all 2nd order shape deformations
- Finding Singularities in Gravitational Lensing
- Multiple Weak Deflections in Galaxy-Galaxy Lensing
- A Stringent Upper Limit on Dark Matter Self-Interaction Cross Section from Cluster Strong Lensing
- Exotic Image Formation in Strong Gravitational Lensing by Clusters of Galaxies. I: Cross-Section
- Exotic Image Formation in Strong Gravitational Lensing by Clusters of Galaxies -- II: Uncertainties