A refined mass distribution of the cluster MACS J0416.1$-$2403 from a new large set of spectroscopic multiply lensed sources
G. B. Caminha, C. Grillo, P. Rosati, I. Balestra, A. Mercurio, E., Vanzella, A. Biviano, K. I. Caputi, C. Delgado-Correal, W. Karman, M., Lombardi, M. Meneghetti, B. Sartoris, P. Tozzi

TL;DR
This paper presents a detailed mass distribution analysis of galaxy cluster MACS J0416.1$-$2403, based on a large set of spectroscopically confirmed multiply lensed sources, revealing complex dark matter structures and improving lensing models.
Contribution
It introduces the largest spectroscopic sample of multiply lensed sources in a single system, refining the cluster's mass model and revealing multiple dark matter halos.
Findings
Confirmed 22 new multiply lensed sources with spectroscopic redshifts.
Identified three cored dark-matter halos in the cluster.
Provided updated lensing maps and redshift catalog for MACS 0416.
Abstract
We report the spectroscopic confirmation of 22 new multiply lensed sources behind the Hubble Frontier Field (HFF) galaxy cluster MACS~J0416.12403 (MACS 0416), using archival data from the Multi Unit Spectroscopic Explorer (MUSE) on the VLT. Combining with previous spectroscopic measurements of 15 other multiply imaged sources, we obtain a sample of 102 secure multiple images with measured redshifts, the largest to date in a single strong lensing system. The newly confirmed sources are largely low-luminosity Lyman- emitters with redshift in the range [3.08-6.15]. With such a large number of secure constraints, and a significantly improved sample of galaxy members in the cluster core, we have improved our previous strong lensing model and obtained a robust determination of the projected total mass distribution of MACS 0416. We find evidence of three cored dark-matter halos,…
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