MACSJ1423.8+2404: Gravitational Lensing by a Massive, Relaxed Cluster of Galaxies at z=0.54

TL;DR

This study combines gravitational lensing and optical observations to analyze the mass distribution of the relaxed galaxy cluster MACS J1423.8+2404 at z=0.54, revealing a nearly unimodal, virialized system with a mass of about 4.3×10^{14} solar masses.

Contribution

It provides a detailed mass model of MACS J1423.8+2404 using combined strong and weak lensing constraints, demonstrating a mostly unimodal, relaxed cluster with minimal substructure.

Findings

Mass within 415 kpc is (4.3±0.6)×10^{14} solar masses.

Mass estimate is about 30% higher than X-ray derived mass, indicating a prolate shape.

Mass, light, and gas distributions are well aligned, indicating a highly evolved system.

Abstract

We present results of a gravitational-lensing and optical study of MACS ,J1423.8+2404 (z=0.545, MACS, J1423). Our analysis uses high-resolution images taken with the Hubble Space Telescope in the F555W and F814W passbands, ground based imaging in eight optical and near-infrared filters obtained with Subaru and CFHT, as well as extensive spectroscopic data gathered with the Keck telescopes. At optical wavelengths the cluster exhibits no sign of substructure and is dominated by a cD galaxy that is 2.1 magnitudes (K-band) brighter than the second brightest cluster member, suggesting that MACS, J1423 is close to be fully virialized. Analysis of the redshift distribution of 140 cluster members reveals a Gaussian distribution, mildly disturbed by the presence of a loose galaxy group that may be falling into the cluster along the line of sight. Combining strong-lensing constraints from two spectroscopically confirmed multiple-image systems near the cluster core with a weak-lensing measurement of the gravitational shear on larger scales, we derive a parametric mass model for the mass distribution. All constraints can be satisfied by a uni-modal mass distribution centred on the cD galaxy and exhibiting very little substructure. The derived projected mass of M(<65\arcsec [415 kpc])=(4.3\pm0.6)\times 10^{14} M_sun is about 30% higher than the one derived from X-ray analyses assuming spherical symmetry, suggesting a slightly prolate mass distribution consistent with the optical indication of residual line-of-sight structure. The similarity in shape and excellent alignment of the centroids of the total mass, K-band light, and intra-cluster gas distributions add to the picture of a highly evolved system [ABRIDGED]