Sunyaev-Zeldovich profiles for clusters and groups of galaxies

TL;DR

This paper develops an empirical model for the 2D and 3D Sunyaev-Zeldovich profiles of galaxy clusters and groups, linking SZ signals to total mass with high accuracy, aiding future SZ survey analyses.

Contribution

The paper introduces a simple, two-parameter empirical model for SZ profiles that accurately relates SZ signals to cluster mass, validated against simulations and observations.

Findings

Tight correlation between model scale, SZ signal, and mass with 4% scatter.

Model applicable to low-resolution SZ data due to simplicity.

Validated against high-resolution simulations and WMAP data.

Abstract

The Sunyaev-Zeldovich (SZ) effect gives a measure of the thermal energy and electron pressure in groups and clusters of galaxies. In the near future SZ surveys will map hundreds of systems, shedding light on the pressure distribution in the systems. The thermal energy is related to the total mass of a system of galaxies, but it is only a projection that is observed through the SZ effect. A model for the 3D distribution of pressure is needed to link the SZ signal to the total mass of the system. In this work we construct an empirical model for the 2D and 3D SZ profile, and compare it to a set of realistic high resolution SPH simulations of galaxy clusters and groups, and to a stacked SZ profile for massive clusters derived from WMAP data. Furthermore, we combine observed temperature profiles with dark matter potentials to yield an additional constraint, under the assumption of hydrostatic equilibrium. We find a very tight correlation between the characteristic scale in the model, the integrated SZ signal, and the total mass in the systems with a scatter of only 4%. The model only contains two free parameters, making it readily applicable even to low resolution SZ observations of galaxy clusters. A fitting routine for the model that can be applied to observed or simulated data can be found at http://www.phys.au.dk/~haugboel/software.shtml