Resolving the hydrostatic mass profiles of galaxy clusters at z ∼ 1 with XMM-Newton and Chandra

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Table C.1.

Parameters of the toy models.

Model	Parameters
n_e model 1^{^a}	n₀₁ = 6.28 × 10⁻³ cm⁻³, r_c1 = 198 kpc, β₁ = 0.7, α = 0.57, r_s = 1613 kpc, ϵ = 0.1, n₀₂ = 10^–3 cm⁻³, β₂ = 0.67, r_c2 = 19.8 kpc
T model X^{^b}	T₀ = 9.1 keV, τ = 0.46, r_cl = 22.78 kpc, a_cl = 1.21, r_t = 7391 kpc, b = 1.03, c = 2.56

^(a)

n_e models 2 and 3 were obtained using the same parameters as that of model 1 except for α = 0.29 and α = 1.37, respectively.

^(b)

Model Y was obtained using the same parameters as model X except for T₀ = 7.28, τ = 0.91, and c = 1.28. The temperature model Z is a flat profile with T = 6.5.

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