# Weak lensing in the Horizon-AGN simulation lightcone. Small scale baryonic effects

## TL;DR

This paper uses the Horizon-AGN hydrodynamical simulation to model weak lensing effects, focusing on small scales where baryonic physics significantly influence lensing statistics, aiding future cosmological survey analyses.

## Contribution

It provides a detailed analysis of baryonic effects on weak lensing signals using high-resolution hydrodynamical simulations, including novel methods for ray-tracing through the lightcone.

## Key findings

- Baryons impact cosmic shear statistics at the 10% level below a few arcmin.
- Galaxy-galaxy lensing signals match observations at z~0.5.
- Magnification bias becomes significant at z>1 for separations >1 Mpc.

## Abstract

Context. Accurate model predictions including the physics of baryons are required to make the most of the upcoming large cosmological surveys devoted to gravitational lensing. The advent of hydrodynamical cosmological simulations enables such predictions on sufficiently sizeable volumes. Aims. Lensing quantities (deflection, shear, convergence) and their statistics (convergence power spectrum, shear correlation functions, galaxy-galaxy lensing) are computed in the past lightcone built in the Horizon-AGN hydrodynamical cosmological simulation, which implements our best knowledge on baryonic physics at the galaxy scale in order to mimic galaxy populations over cosmic time. Methods. Lensing quantities are generated over a one square degree field of view by performing multiple-lens plane ray-tracing through the lightcone, taking full advantage of the 1 kpc resolution and splitting the line of sight over 500 planes all the way to redshift z~7. Two methods are explored (standard projection of particles with adaptive smoothing, and integration of the acceleration field) to assert a good implementation. The focus is on small scales where baryons matter most. Results. Standard cosmic shear statistics are impacted at the 10% level by the baryonic component for angular scales below a few arcmin. The galaxy-galaxy lensing signal, or galaxy-shear correlation function, is consistent with measurements for the redshift z~0.5 massive galaxy population. At higher redshift z>1, the impact of magnification bias on this correlation is relevant for separations greater than 1 Mpc. Conclusions. This work is pivotal for all current and upcoming weak lensing surveys and represents a first step towards building a full end-to-end generation of lensed mock images from large cosmological hydrodynamical simulations.