Galaxy-galaxy lensing in the outskirts of CLASH clusters: constraints on local shear and testing mass-luminosity scaling relation

TL;DR

This study uses galaxy-galaxy lensing in the outskirts of CLASH clusters to measure local shear, test mass-luminosity relations, and compare strong and weak lensing results, enhancing understanding of cluster mass distributions.

Contribution

It introduces a method to constrain local shear using GGLs in cluster outskirts and tests the mass-luminosity scaling relation of cluster members.

Findings

Local shear from GGLs traces cluster potential at 1-2 arcmin.

Strong and weak lensing shear measurements agree well.

Mass-luminosity relation parameters can vary by up to 30%."

Abstract

We present a selection of 24 candidate galaxy-galaxy lensing (GGLs) identified from Hubble images in the outskirts of the massive galaxy clusters from the CLASH survey. These GGLs provide insights into the mass distributions at larger scales than the strong lensing region in the cluster cores. We built parametric mass models for three of these GGLs showing simple lensing configurations, in order to assess the properties of their lens and its environment. We show that the local shear estimated from the GGLs traces the gravitational potential of the clusters at 1-2 arcmin radial distance, allowing us to derive their velocity dispersion. We also find a good agreement between the strength of the shear measured at the GGL positions through strong-lensing modelling and the value derived independently from a weak-lensing analysis of the background sources. Overall, we show the advantages of using single GGL events in the outskirts of clusters to robustly constrain the local shear, even when only photometric redshift estimates are known for the source. We argue that the mass-luminosity scaling relation of cluster members can be tested by modelling the GGLs found around them, and show that the mass parameters can vary up to $\sim$30% between the cluster and GGL models assuming this scaling relation.