A state-of-the-art strong lensing model of MACS J0416.1-2403 with the largest sample of spectroscopic multiple images
arXiv:2208.14020 · doi:10.1051/0004-6361/202244834
Abstract
The combination of multi-band imaging from HST with MUSE integral field spectroscopy, obtained at the VLT, has recently driven remarkable progress in strong lensing (SL) modeling of galaxy clusters. From a few tens of multiple images with photometric redshifts per cluster, a new generation of high-precision SL models have recently been developed, by exploiting in some cases over a hundred of spectroscopically confirmed multiple images and cluster member galaxies. A further step forward is expected with JWST observations of SL clusters (from hundreds to possibly a thousand of multiple images). In this context, we present a new, state-of-the-art SL model of the galaxy cluster MACS J0416.1-2403, utilizing 237 spectroscopically confirmed multiple images, which is the largest sample of secure multiply lensed sources utilized to date. This model incorporates stellar kinematics information of 64 cluster galaxies and the hot-gas mass distribution of the cluster determined from Chandra X-ray observations. The observed positions of the many multiple images are reproduced with a remarkable accuracy of 0.43 arcsec. To further assess the reliability of this lens model and to highlight the improvement over previously published models, we show the extended surface brightness reconstruction of several lensed galaxies through a newly developed forward modeling software. The comparison with other SL models of the same cluster demonstrates that this new model is better suited to accurately reproduce the positions, shapes and fluxes of the observed multiple images. Besides a robust characterization of the total mass distribution of the cluster, our model can provide accurate and precise magnification maps that are key to studying the intrinsic physical properties of faint, high-redshift lensed sources. The model is made publicly available through our newly developed Strong Lensing Online Tool (or SLOT).
arXiv commentAccepted for publication in Astronomy & Astrophysics (16 pages, 13 figures)
References in corpus (53)
- Cluster Lensing And Supernova survey with Hubble (CLASH): An Overview
- A Bayesian approach to strong lensing modelling of galaxy clusters
- The Frontier Fields: Survey Design
- MACS: A quest for the most massive galaxy clusters in the universe
- Hubble Space Telescope Observations of the Lensing Cluster Abell 2218
- CLASH: Three Strongly Lensed Images of a Candidate z ~ 11 Galaxy
- CLASH: Weak-Lensing Shear-and-Magnification Analysis of 20 Galaxy Clusters
- The GLASS James Webb Space Telescope Early Release Science Program. I. Survey Design and Release Plans
- Lyman-alpha Emission from a Luminous z=8.68 Galaxy: Implications for Galaxies as Tracers of Cosmic Reionization
- X-ray/optical classification of cluster mergers and the evolution of the cluster merger fraction
- Mass and magnification maps for the Hubble Space Telescope Frontier Fields clusters: implications for high redshift studies
- The Grism Lens-Amplified Survey from Space (GLASS). I. Survey overview and first data release
- Multi-scale cluster lens mass mapping I. Strong Lensing modelling
- 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
- A Census of Star-Forming Galaxies in the z~9-10 Universe based on HST+Spitzer Observations Over 19 CLASH clusters: Three Candidate z~9-10 Galaxies and Improved Constraints on the Star Formation Rate Density at z~9
- Cosmological Constraints from Strong Gravitational Lensing in Galaxy Clusters
- CLASH-VLT: Insights on the mass substructures in the Frontier Fields Cluster MACS J0416.1-2403 through accurate strong lens modeling
- An excess of small-scale gravitational lenses observed in galaxy clusters
- JWST's PEARLS: Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results
- Constraining the mass distribution of galaxies using galaxy-galaxy lensing in clusters and in the field
- CLASH-VLT: A Highly Precise Strong Lensing Model of the Galaxy Cluster RXC J2248.7-4431 (Abell S1063) and Prospects for Cosmography
- Hubble Frontier Fields : A High-Precision Strong-Lensing Mass Model of the Massive Galaxy Cluster Abell 2744 using 180 Multiple Images
- An Atlas of MUSE Observations towards Twelve Massive Lensing Clusters
- Hubble Frontier Fields : A High Precision Strong Lensing Analysis of Galaxy Cluster MACSJ0416.1-2403 using ~200 Multiple Images
- A refined mass distribution of the cluster MACS J0416.12403 from a new large set of spectroscopic multiply lensed sources
- CLASH-VLT: Dissecting the Frontier Fields Galaxy Cluster MACS J0416.1-2403 with Spectra of Member Galaxies
- Lens Modeling Abell 370: Crowning the Final Frontier Field with MUSE
- The story of supernova 'Refsdal' told by MUSE
- Measuring the value of the Hubble constant "à la Refsdal"
- Strong lensing models of eight CLASH clusters from extensive spectroscopy: accurate total mass reconstructions in the cores
- Magnifying the early episodes of star formation: super star clusters at cosmological distances
- Enhanced cluster lensing models with measured galaxy kinematics
- The systematics of strong lens modeling quantified: the effects of constraint selection and redshift information on magnification, mass, and multiple image predictability
- Star Formation at z=2.481 in the Lensed Galaxy SDSS J1110+6459: Star Formation down to 30 parsec scales
- Mass distribution in the core of MACS J1206: robust modeling from an exceptionally large sample of central multiple images
- The MUSE Deep Lensed Field on the Hubble Frontier Field MACS~J0416
- Strong Lens Models for 37 Clusters of Galaxies from the SDSS Giant Arcs Survey
- On the stellar masses of giant clumps in distant star-forming galaxies
- On the accuracy of time-delay cosmography in the Frontier Fields Cluster MACS J1149.5+2223 with supernova Refsdal
- New high-precision strong lensing modeling of Abell 2744. Preparing for JWST observations
- Exploring the physical properties of lensed star-forming clumps at
- Early results from GLASS-JWST. VII: evidence for lensed, gravitationally bound proto-globular clusters at z=4 in the Hubble Frontier Field A2744
- Candidate Population III stellar complex at z=6.629 in the MUSE Deep Lensed Field
- A new high-precision strong lensing model of the galaxy cluster MACS J0416.1-2403
- 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
- Dissection of the collisional and collisionless mass components in a mini sample of CLASH and HFF massive galaxy clusters at
- MACS J0416.1-2403: Impact of line-of-sight structures on strong gravitational lensing modelling of galaxy clusters
- The probability of galaxy-galaxy strong lensing events in hydrodynamical simulations of galaxy clusters
- Galaxy cluster strong lensing cosmography: cosmological constraints from a sample of regular galaxy clusters
- Joining X-ray to lensing: an accurate combined analysis of MACS J0416.12403
- Galaxy cluster cores as seen with VLT/MUSE: new strong-lensing analyses of RX J2129.4+0009, MS 0451.6-0305 & MACSJ2129.4-0741
- Free-form lens model and mass estimation of the high redshift galaxy cluster ACT-CL J0102-4915, "El Gordo"
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- An extremely metal poor star complex in the reionization era: Approaching Population III stars with JWST
- The GLASS-JWST Early Release Science Program. III. Strong lensing model of Abell 2744 and its infalling regions
- JWST's PEARLS: Mothra, a new kaiju star at z=2.091 extremely magnified by MACS0416, and implications for dark matter models
- A persistent excess of galaxy-galaxy strong lensing observed in galaxy clusters
- Anatomy of a z=6 Lyman-α emitter down to parsec scales: extreme UV slopes, metal-poor regions and possibly leaking star clusters
- JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at
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- CANUCS: Constraining the MACS J0416.1-2403 Strong Lensing Model with JWST NIRISS, NIRSpec and NIRCam
- Exploring the low-mass regime of galaxy-scale strong lensing: Insights into the mass structure of cluster galaxies
- Model-Independent Mass Reconstruction of the Hubble Frontier Field Clusters with MARS Based on Self-Consistent Strong Lensing Data
- Gravity.jl: fast and accurate gravitational lens modeling in Julia
- BUFFALO Wild Wings: A High Precision Free-Form Lens Model of MACSJ0416 with Constraints on Dark Matter from Substructure and Highly Magnified Arcs
- Enhanced strong-lensing model of MACS~J0138.02155 based on new JWST and VLT/MUSE observations
- The powerful lens galaxy cluster PLCK G287.0+32.9 ()
- Cosmography from accurate mass modeling of the lens group SDSS J0100+1818: five sources at three different redshifts
- The Kaleidoscope Survey: Strong Gravitational Lensing in Galaxy Clusters with Radial Arcs
- Constraints from the Giant Arc in Abell 370. A New Framework for Understanding Systematic Errors in Cluster Lens Modeling. IV. Constraints from the Giant Arc in Abell 370
- Galaxies at the edges: a complete census of MACS J0416.1-2403 cluster
- MrMARTIAN: A Multi-resolution Mass Reconstruction Algorithm Combining Free-form and Analytic Components
- The velocity dispersion function of red galaxies in four Hubble Frontier Fields galaxy clusters
- CLASH-VLT: The Fifth Force in Chameleon Gravity from Joint Lensing and Kinematics Cluster Mass Profiles
- Constraining the geometry of the gas surrounding a typical galaxy at with Ly polarization