Constrained Cluster Parameters from SZ Observations

Near-future SZ surveys such as ACT, SPT, APEX, and Planck will find thousands of galaxy clusters. Multi-frequency arcminute-resolution SZ observations can, in principle, determine each cluster's gas temperature (T_e), bulk velocity (v_pec), and optical depth (tau). However, the frequency bands and detector sensitivity employed by upcoming surveys will generally not be sufficient to disentangle the degeneracy between these three cluster parameters, even in the absence of SZ signal contamination from point sources and imperfect primary microwave background subtraction. Assuming contaminants can be removed, we find that near-future SZ surveys will be able to constrain well two cluster gas parameters that are linear combinations of tau*T_e, tau*v_z, and tau*T_e^2. Given that the SZ intensity shift is nearly a linear function of tau*T_e, tau*v_z, and tau*T_e^2, a correspondence exists between the two effective gas parameters that SZ surveys can constrain and simple line-of-sight integrals through the three dimensional cluster. We illustrate the parameter constraints and correspondence to line-of-sight integrals using 3D Nbody + hydro cluster simulations and a Markov chain Monte Carlo method. We show that adding an independent T_e measurement to upcoming SZ data breaks the parameter degeneracy. The cluster effective velocity thus constrained is approximately the optical-depth-weighted velocity integrated along the cluster line of sight. A temperature prior with an error as large as 2 keV still gives bulk velocity errors < 100 km/sec, even for average-size clusters with a T_e of 3 keV, for ACT-like SZ observations in the absence of signal contamination. The Markov chain constraints on v_pec and tau are more encouraging and likely more accurate than those obtained from Fisher matrices