Hydrostatic mass profiles in X-COP galaxy clusters

Abstract

Aims.We present the reconstruction of hydrostatic mass profiles in 13 X-ray luminous galaxy clusters that have been mapped in their X-ray and Sunyaev–Zeldovich (SZ) signals out toR200for theXMM-NewtonCluster Outskirts Project (X-COP).Methods.Using profiles of the gas temperature, density, and pressure that have been spatially resolved out to median values of 0.9R500, 1.8R500, and 2.3R500, respectively, we are able to recover the hydrostatic gravitating mass profile with several methods and using different mass models.Results.The hydrostatic masses are recovered with a relative (statistical) median error of 3% atR500and 6% atR200. By using several different methods to solve the equation of the hydrostatic equilibrium, we evaluate some of the systematic uncertainties to be of the order of 5% at bothR500andR200. A Navarro-Frenk-White profile provides the best-fit in 9 cases out of 13; the remaining 4 cases do not show a statistically significant tension with it. The distribution of the mass concentration follows the correlations with the total mass predicted from numerical simulations with a scatter of 0.18 dex, with an intrinsic scatter on the hydrostatic masses of 0.15 dex. We compare them with the estimates of the total gravitational mass obtained through X-ray scaling relations applied toYX, gas fraction, andYSZ, and from weak lensing and galaxy dynamics techniques, and measure a substantial agreement with the results from scaling laws, from WL at bothR500andR200(with differences below 15%), from cluster velocity dispersions. Instead, we find a significant tension with the caustic masses that tend to underestimate the hydrostatic masses by 40% atR200. We also compare these measurements with predictions from alternative models to the cold dark matter, like the emergent gravity and MOND scenarios, confirming that the latter underestimates hydrostatic masses by 40% atR1000, with a decreasing tension as the radius increases, and reaches ∼15% atR200, whereas the former reproducesM500within 10%, but overestimatesM200by about 20%.Conclusions.The unprecedented accuracy of these hydrostatic mass profiles out toR200allows us to assess the level of systematic errors in the hydrostatic mass reconstruction method, to evaluate the intrinsic scatter in the NFWc − Mrelation, and to robustly quantify differences among different mass models, different mass proxies, and different gravity scenarios.