On the Effects of Local Environment on Active Galactic Nucleus (AGN) in the Horizon Run 5 Simulation
Ankit Singh, Changbom Park, Ena Choi, Juhan Kim, Hyunsung Jun, Brad K., Gibson, Yonghwi Kim, Jaehyun Lee, Owain Snaith

TL;DR
This study uses the Horizon Run 5 simulation to analyze how local galaxy environment and intrinsic properties influence AGN activity, highlighting the dominant role of nearest neighbor environment at small scales.
Contribution
It demonstrates that the nearest neighbor environment significantly impacts AGN properties and cold gas content, providing new insights into environmental effects on AGN activity.
Findings
Nearest neighbor environment dominates AGN luminosity and gas content.
Cold gas availability is crucial for triggering AGN activity.
Small-scale environment effects become dominant at less than half the neighbor's virial radius.
Abstract
We use the Horizon Run 5 cosmological simulation to study the effect of galaxy intrinsic properties and the local environment on AGNs characterized by their threshold of the accretion rate. We select galaxies in the stellar mass range in the snapshot at redshift =0.625. Among various intrinsic properties, we find that the star formation rate of the host galaxy is most correlated to the AGN activity. To quantify the environment, we use background galaxy number density (large-scale environment) and distance and morphological type of the nearest neighbors (small-scale environment), and study their relative effects on the AGN properties. We find that, compared to the background density, the nearest neighbor environment is the dominant quantity determining the bolometric luminosity, star formation rate, and kinematic properties of AGNs and…
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