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 | ![]() |
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DM2 | ![]() |
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GAL1 | [−14.1] | [15.1] | ![]() |
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[0] | ![]() |
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GAL2 | [−10.6] | [17.6] | [0.50] | ![]() |
[0] | [40] | ![]() |
GAL3 | [12.2] | [19.6] | ![]() |
![]() |
[0] | ![]() |
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GAL4 | [−0.2] | [0.0] | [0.46] | [−9.6] | [0] | ![]() |
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L* galaxy | [0.15] | ![]() |
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MACS0329 | |||||||
DM1 | ![]() |
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[1000] | ![]() |
DM2 | ![]() |
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[0.30] | ![]() |
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[1000] | ![]() |
DM3 | ![]() |
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[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 | ![]() |
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[1000] | ![]() |
DM2 | ![]() |
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[1000] | ![]() |
GAL1 | [31.8] | [−65.5] | [0.04] | [−40.4] | [0] | [62] | ![]() |
GAL2 | ![]() |
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[25] | [200] | ![]() |
L* galaxy | [0.15] | ![]() |
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Bullet Cluster | |||||||
DM1 | ![]() |
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[1000] | ![]() |
DM2 | ![]() |
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[1000] | ![]() |
DM3 | ![]() |
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[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] | ![]() |
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[0] | ![]() |
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L* galaxy | [0.15] | ![]() |
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MACS0940 | |||||||
DM1 | ![]() |
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GAL1 | [−0.1] | [0.1] | ![]() |
[−7.7] | [0] | [52] | ![]() |
GAL2 | [−11.8] | [3.1] | ![]() |
![]() |
[0] | [17] | ![]() |
GAL3 | [5.9] | [−5.7] | [0.00] | ![]() |
[0] | ![]() |
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L* galaxy | [0.15] | ![]() |
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MACS1206 | |||||||
DM1 | ![]() |
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[1000] | ![]() |
DM2 | ![]() |
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[1000] | ![]() |
DM3 | ![]() |
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[1000] | ![]() |
GAL1 | [−0.1] | [0.0] | [0.71] | [14.4] | ![]() |
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GAL2 | [35.8] | [16.1] | [0.23] | ![]() |
[0] | ![]() |
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γ | ![]() |
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L* galaxy | ![]() |
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RXJ1347 | |||||||
DM1 | ![]() |
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[1000] | ![]() |
DM2 | ![]() |
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[1000] | ![]() |
DM3 | ![]() |
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[1000] | ![]() |
GAL1 | [0.0] | [−0.0] | [0.23] | [−86.9] | [0] | ![]() |
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GAL2 | [−17.8] | [−2.1] | [0.30] | [−64.1] | [0] | ![]() |
![]() |
GAL3 | [15.5] | [19.6] | [0.06] | [14.2] | [0] | ![]() |
![]() |
γ | ![]() |
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L* galaxy | [0.15] | ![]() |
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SMACS2031 | |||||||
DM1 | ![]() |
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[1000] | ![]() |
DM2 | ![]() |
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[1000] | ![]() |
GAL1 | [0.1] | [−0.1] | [0.09] | [−0.4] | [0] | ![]() |
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L* galaxy | [0.15] | ![]() |
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SMACS2131 | |||||||
DM1 | ![]() |
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[1000] | ![]() |
DM2 | ![]() |
[17.0] | ![]() |
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[1000] | ![]() |
GAL1 | [−0.0] | [0.0] | [0.11] | ![]() |
[0] | ![]() |
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GAL2 | [6.7] | [−2.2] | [0.76] | ![]() |
[0] | ![]() |
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L* galaxy | [0.15] | ![]() |
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MACS2214 | |||||||
DM1 | ![]() |
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[1000] | ![]() |
DM2 | ![]() |
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[1000] | ![]() |
DM3 | ![]() |
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[1000] | ![]() |
GAL1 | [0.0] | [0.0] | [0.20] | ![]() |
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GAL2 | [8.2] | [18.8] | ![]() |
[0.0] | [0] | ![]() |
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GAL3 | [19.9] | [2.0] | ![]() |
![]() |
[0] | ![]() |
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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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