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

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Table 1.

Relevant quantities computed at fixed radii and overdensities.

Cluster name	z			c₅₀₀
SPT-CLJ2146-4633	0.933
PLCKG266.6-27.3^{^a}	0.972
SPT-CLJ2341-5119	1.003
SPT-CLJ0546-5345	1.066
SPT-CLJ2106-5844	1.132	1576^{^b}	40.19^{^b}	0.01^{^b}

Notes. M^DF and M^BP are the masses computed within using the direct fit (DF) and backward parametric (BP) methods; c₅₀₀ is derived from the DF NFW model. Radii and masses are in units of [kpc] and [10¹⁴ M_⊙], respectively.

^(a)

SPT name: SPT-CLJ0615-5746.

^(b)

The , and the c₅₀₀ values were calculated performing an extrapolation (see text for details). For this reason, these values were not used for quantitative analysis, and the errors are not reported.

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