{"paper":{"title":"The shape of galaxy dark matter halos in massive galaxy clusters: Insights from strong gravitational lensing","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"D. Harvey (EPFL), Durham), M. Jauzac (CEA, R. Massey (CEA","submitted_at":"2017-11-27T18:55:40Z","abstract_excerpt":"We assess how much unused strong lensing information is available in the deep \\emph{Hubble Space Telescope} imaging and VLT/MUSE spectroscopy of the \\emph{Frontier Field} clusters. As a pilot study, we analyse galaxy cluster MACS\\,J0416.1-2403 ($z$$=$$0.397$, $M(R<200\\,{\\rm kpc})$$=$$1.6$$\\times$$10^{14}\\msun$), which has 141 multiple images with spectroscopic redshifts. We find that many additional parameters in a cluster mass model can be constrained, and that adding even small amounts of extra freedom to a model can dramatically improve its figures of merit. We use this information to const"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.09882","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}