Table 2
Best-fit NFW parameters, at different overdensities, derived taking the two brightest galaxies as centre (n = 1,2).
| n | Mvir | cvir | rvir | M2500 | r2500 | M500 | r500 | M200 |
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| 1s |
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| 1b |
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| 1c |
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| 1d |
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| 1e |
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| 2a |
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| 2b |
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| 2c |
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| 2d |
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| 2e |
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Notes. For each centre, in the upper row (a) both Mvir and cvir were taken as free parameters; in the next row (b) the (Mvir, cvir, zcl) relation (Duffy et al. 2008) was used; in the last three rows we use the c−M−z 2D relations in Meneghetti et al. (2014) (c: all, d: relaxed, e: super-relaxed). Masses are in units of 1014M⊙, radii in kpc.
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