Clash-Vlt: Dissecting the frontier fields galaxy cluster macs j0416.1-2403 with 3c800 spectra of member galaxies

We present VIMOS-Very Large Telescope (VLT) spectroscopy of the Frontier Fields cluster MACS\uf0a0J0416.1-2403 (z\uf0a0=\uf0a00.397). Taken as part of the CLASH-VLT survey, the large spectroscopic campaign provided more than 4000 reliable redshifts over 3c600 arcmin2, including 3c800 cluster member galaxies. The unprecedented sample of cluster members at this redshift allows us to perform a highly detailed dynamical and structural analysis of the cluster out to 3c2.2 r200 ( 3c4Mpc). Our analysis of substructures reveals a complex system composed of a main massive cluster (M200\uf0a0 3c\uf0a00.9\uf0a0 7\uf0a01015Me and \u3c3V,r200\uf0a0 3c\uf0a01000 km s 121) presenting two major features: (i) a bimodal velocity distribution, showing two central peaks separated by \u394Vrf\uf0a0 3c\uf0a01100 kms 121 with comparable galaxy content and velocity dispersion, and (ii) a projected elongation of the main substructures along the NE\u2013SW direction, with a prominent sub-clump 3c600 kpc SW of the center and an isolated BCG approximately halfway between the center and the SW clump. We also detect a low-mass structure at z\uf0a0 3c\uf0a00.390, 3c10\u2032 south of the cluster center, projected at 3c3Mpc, with a relative line-of-sight velocity of \u394Vrf\uf0a0 3c\uf0a0 121700 km s 121. The cluster mass profile that we obtain through our dynamical analysis deviates significantly from the \u201cuniversal\u201d NFW, being best fit by a Softened Isothermal Sphere model instead. The mass profile measured from the galaxy dynamics is found to be in relatively good agreement with those obtained from strong and weak lensing, as well as with that from the X-rays, despite the clearly unrelaxed nature of the cluster. Our results reveal an overall complex dynamical state of this massive cluster and support the hypothesis that the two main subclusters are being observed in a pre-collisional phase, in agreement with recent findings from radio and deep X-ray data. In this article, we also release the entire redshift catalog of 4386 sources in the field of this cluster, which includes 60 identified Chandra X-ray sources and 105 JVLA radio sources