Open Access

Table B.1.

Best fit model parameters for the mass distribution in each cluster.

Potential ΔRA ΔDec e θ rcore rcut σ
[″] [″] [deg] [kpc] [kpc] [km s−1]
MACS0257

DM1
DM2
GAL1 [−14.1] [15.1] [0]
GAL2 [−10.6] [17.6] [0.50] [0] [40]
GAL3 [12.2] [19.6] [0]
GAL4 [−0.2] [0.0] [0.46] [−9.6] [0]
L* galaxy [0.15]

MACS0329

DM1 [1000]
DM2 [0.30] [1000]
DM3 [0.30] [25] [1000]
GAL1 [0.0] [0.0] [0.19] [−73.6] [0] [98]
GAL2 [−12.7] [−39.9] [0.14] [56.9] [0] [41]
L* galaxy [0.15] [45]

MACS0416

DM1 [1000]
DM2 [1000]
GAL1 [31.8] [−65.5] [0.04] [−40.4] [0] [62]
GAL2 [25] [200]
L* galaxy [0.15]

Bullet Cluster

DM1 [1000]
DM2 [1000]
DM3 [1000]
GAL1 [0.0] [0.0] [0.26] [43.5] [0] [150]
GAL2 [24.0] [29.1] [0.20] [37.4] [0] [112]
GAL3 [51.9] [48.9] [0.13] [9.9] [0] [60]
GAL4 [5.2] [23.0] [0]
L* galaxy [0.15]

MACS0940

DM1
GAL1 [−0.1] [0.1] [−7.7] [0] [52]
GAL2 [−11.8] [3.1] [0] [17]
GAL3 [5.9] [−5.7] [0.00] [0]
L* galaxy [0.15]

MACS1206

DM1 [1000]
DM2 [1000]
DM3 [1000]
GAL1 [−0.1] [0.0] [0.71] [14.4]
GAL2 [35.8] [16.1] [0.23] [0]
γ
L* galaxy

RXJ1347

DM1 [1000]
DM2 [1000]
DM3 [1000]
GAL1 [0.0] [−0.0] [0.23] [−86.9] [0]
GAL2 [−17.8] [−2.1] [0.30] [−64.1] [0]
GAL3 [15.5] [19.6] [0.06] [14.2] [0]
γ
L* galaxy [0.15]

SMACS2031

DM1 [1000]
DM2 [1000]
GAL1 [0.1] [−0.1] [0.09] [−0.4] [0]
L* galaxy [0.15]

SMACS2131

DM1 [1000]
DM2 [17.0] [1000]
GAL1 [−0.0] [0.0] [0.11] [0]
GAL2 [6.7] [−2.2] [0.76] [0]
L* galaxy [0.15]

MACS2214

DM1 [1000]
DM2 [1000]
DM3 [1000]
GAL1 [0.0] [0.0] [0.20]
GAL2 [8.2] [18.8] [0.0] [0]
GAL3 [19.9] [2.0] [0]
L* galaxy [0.15]

Notes. From left to right: mass component, position relative to cluster centre (ΔRA and ΔDec), dPIE shape (ellipticity and orientation), core and cut radii, velocity dispersion. The final row is the generic galaxy mass at the characteristic luminosity L*, which is scaled to match each of cluster member galaxies. Parameters in square brackets are fixed a priori in the model.

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