Full Lensing Analysis of Abell 1703: Comparison of Independent Lens-Modelling Techniques
Adi Zitrin, Tom Broadhurst, Keiichi Umetsu, Yoel Rephaeli, Elinor, Medezinski, Larry Bradley, Yolanda Jim\'enez-Teja, Narciso Ben\'itez, Holland, Ford, Jori Liesenborgs, Sven De Rijcke, Herwig Dejonghe, Philippe Bekaert

TL;DR
This study compares parametric and non-parametric strong lensing techniques on Abell 1703, integrating weak lensing data to derive a consistent mass profile, revealing the cluster's high concentration compared to standard cosmological predictions.
Contribution
It demonstrates the consistency of different lensing methods and combines strong and weak lensing data to accurately determine the cluster's mass profile and concentration.
Findings
Both lensing methods agree on the large-scale dark matter distribution.
The combined profile fits an NFW model with high concentration.
Abell 1703 has a higher concentration than predicted by standard models.
Abstract
The inner mass-profile of the relaxed cluster Abell 1703 is analysed by two very different strong-lensing techniques applied to deep ACS and WFC3 imaging. Our parametric method has the accuracy required to reproduce the many sets of multiple images, based on the assumption that mass approximately traces light. We test this assumption with a fully non-parametric, adaptive grid method, with no knowledge of the galaxy distribution. Differences between the methods are seen on fine scales due to member galaxies which must be included in models designed to search for lensed images, but on the larger scale the general distribution of dark matter is in good agreement, with very similar radial mass profiles. We add undiluted weak-lensing measurements from deep multi-colour Subaru imaging to obtain a fully model-independent mass profile out to the virial radius and beyond. Consistency is found in…
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