Testing for evolution in scaling relations of galaxy clusters: Cross analysis between X-ray and SZ observations

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Abstract

Aims. We present predicted Sunyaev-Zeldovich (SZ) properties of known X-ray clusters of galaxies for which gas temperature measurements are available. The reference sample was compiled from the BAX database for X-ray clusters. Methods. The Sunyaev-Zeldovich signal is predicted according to two different scaling laws for the mass-temperature relation in clusters: a standard relation and an evolving relation that reproduces well the evolution of the X-ray temperature distribution function in a concordance cosmology. Using a Markov chain Monte Carlo (MCMC) analysis we examine the values of the recovered parameters and their uncertainties. Results. The evolving case can be clearly distinguished from the non-evolving case, showing that SZ measurements will indeed be efficient in constraining the thermal history of the intra-cluster gas. However, significant bias appears in the measured values of the evolution parameter for high SZ threshold owing to selection effects. © 2011 ESO.

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Ferramacho, L. D., & Blanchard, A. (2011). Testing for evolution in scaling relations of galaxy clusters: Cross analysis between X-ray and SZ observations. Astronomy and Astrophysics, 533. https://doi.org/10.1051/0004-6361/201016041

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