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Table 4:

Summary of the main results.

Method
$\sigma_v$ [ $\rm km~s^{-1}$] r200 [kpc] M200 [ $10^{14}~M_\odot$]
Galaxy counts - $811\pm46$ $0.74\pm0.15$
Spectr. (early type) $480\pm20$ $1054\pm44$ $1.69\pm0.14$
Spectr. (late type) $590\pm20$ $1295\pm44$ $3.14\pm0.21$
X-ray ($\beta $-model) $316\pm26$ $617\pm28$ $0.34\pm0.10$
Weak lens. (SIS) $476\pm46$ $853\pm82$ $0.90\pm0.26$
Weak lens. (NFW) - $834\pm219$ $0.84\pm0.66$
Weak lens. (MR) - $650\pm50$* $0.38\pm0.09$*
Strong lensing $319\pm4$ $700\pm9$ $0.50\pm0.01$

Notes. Values in bold face are the primary measurements, the others were derived from these.
(*) The mass estimate from the weak lensing mass reconstruction is obtained within a radius of 182 kpc, significantly smaller than r200. The given values are therefore lower limits.


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