The impact of AGN feedback and baryonic cooling on galaxy clusters as gravitational lenses

TL;DR

This study examines how AGN feedback influences the gravitational lensing capabilities of galaxy clusters, showing that AGN feedback reduces the baryonic boost on strong lensing cross-sections and affects mass profile measurements.

Contribution

It provides a detailed comparison of lensing properties in simulations with and without AGN feedback, highlighting its role in moderating baryonic effects on galaxy cluster lensing.

Findings

AGN feedback reduces the baryonic boost on strong lensing cross-section.

Clusters with AGN feedback have similar lensing cross-sections to dark-matter only clusters.

AGN feedback leads to lower concentration parameters in weak lensing analyses.

Abstract

We investigate the impact of AGN feedback on the gravitational lensing properties of a sample of galaxy clusters with masses in the range 10^14 - 10^15 Msol, using state-of-the-art simulations. Adopting a ray-tracing algorithm, we compute the cross-section of giant arcs from clusters simulated with dark-matter only physics (DM), dark matter plus gas with cooling and star formation (CSF), and dark matter plus gas with cooling, star formation and AGN feedback (CSFBH). Once AGN feedback is included, baryonic physics boosts the strong lensing cross-section by much less than previously estimated using clusters simulated with only cooling and star formation. For a cluster with a virial mass of 7.4 X 10^14 Msol, inclusion of baryonic physics without feedback can boost the cross-section by as much as a factor of 3, in agreement with previous studies, whereas once AGN feedback is included this maximal figure falls to a factor of 2 at most. Typically, clusters simulated with DM and CSFBH physics have similar cross-sections for the production of giant arcs. We also investigate how baryonic physics affects the weak lensing properties of the simulated clusters by fitting NFW profiles to synthetic weak lensing data sets using a Markov Chain Monte Carlo approach, and by performing non-parametric mass reconstructions. Without the inclusion of AGN feedback, measured concentration parameters can be much larger than those obtained with AGN feedback, which are similar to the dark-matter only case.