Lens models and magnification maps of the six Hubble Frontier Fields clusters
arXiv:1405.0222 · doi:10.1088/0004-637X/797/1/48
Abstract
We present strong-lensing models, as well as mass and magnification maps, for the cores of the six HST Frontier Fields galaxy clusters. Our parametric lens models are constrained by the locations and redshifts of multiple image systems of lensed background galaxies. We use a combination of photometric redshifts and spectroscopic redshifts of the lensed background sources obtained by us (for Abell 2744 and Abell S1063), collected from the literature, or kindly provided by the lensing community. Using our results, we (1) compare the derived mass distribution of each cluster to its light distribution, (2) quantify the cumulative magnification power of the HFF clusters, (3) describe how our models can be used to estimate the magnification and image multiplicity of lensed background sources at all redshifts and at any position within the cluster cores, and (4) discuss systematic effects and caveats resulting from our modeling methods. We specifically investigate the effect of the use of spectroscopic and photometric redshift constraints on the uncertainties of the resulting models. We find that the photometric redshift estimates of lensed galaxies are generally in excellent agreement with spectroscopic redshifts, where available. However, the flexibility associated with relaxed redshift priors may cause the complexity of large-scale structure that is needed to account for the lensing signal to be underestimated. Our findings thus underline the importance of spectroscopic arc redshifts, or tight photometric redshift constraints, for high precision lens models. All products from our best-fit lens models (magnification, convergence, shear, deflection field) and model simulations for estimating errors are made available via the Mikulski Archive for Space Telescopes.
34 pages, 19 figures, 17 tables. Accepted to ApJ. Models are publicly available on the Mikulski Archive for Space Telescopes (http://archive.stsci.edu/prepds/frontier/lensmodels/)
References in corpus (16)
- A direct empirical proof of the existence of dark matter
- The Hubble Ultra Deep Field
- A Bayesian approach to strong lensing modelling of galaxy clusters
- Galaxies in the Hubble Ultra Deep Field: I. Detection, Multiband Photometry, Photometric Redshifts, and Morphology
- Combining Strong and Weak Gravitational Lensing in Abell 1689
- Revealing the properties of dark matter in the merging cluster MACSJ0025.4-1222
- A complete sample of twelve very X-ray luminous galaxy clusters at z>0.5
- Mass and magnification maps for the Hubble Space Telescope Frontier Fields clusters: implications for high redshift studies
- Hubble Frontier Fields : A High Precision Strong Lensing Analysis of Galaxy Cluster MACSJ0416.1-2403 using ~200 Multiple Images
- Strong Lensing in Abell 1703: Constraints on the Slope of the Inner Dark Matter Distribution
- Discovery of the largest known lensed images formed by a critically convergent lensing cluster
- Where is the matter in the Merging Cluster Abell 2218?
- Realistic simulations of gravitational lensing by galaxy clusters: extracting arc parameters from mock DUNE images
- LensPerfect: Gravitational Lens Massmap Reconstructions Yielding Exact Reproduction of All Multiple Images
- An X-ray/optical study of the complex dynamics of the core of the massive intermediate-redshift cluster MACSJ0717.5+3745
- The Redshift Distribution of Giant Arcs in the Sloan Giant Arcs Survey
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- MUSE observations of the lensing cluster SMACSJ2031.8-4036: new constraints on the mass distribution in the cluster core
- The ALMA Frontier Fields Survey - II. Multiwavelength Photometric analysis of 1.1mm continuum sources in Abell 2744, MACSJ0416.1-2403 and MACSJ1149.5+2223
- Young Galaxy Candidates in the Hubble Frontier Fields IV. MACS J1149.5+2223
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