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Table A.1.

Median values and confidence levels of the cluster total mass distribution parameters from the MCMC analyses of the reference strong lensing models (see Table 5).

Median 68% CL 95% CL 99.7% CL
RX J2129

Smooth component 1

x (″) 2.4
y (″) −1.6
ε 0.67
θ (°) −23.7
rcore (″) 14.0
σv (km s−1) 1079

Galaxy members

(kpc) 2.1
(km s−1) 392

MACS J1931

Smooth component 1

x (″) 0.09
y (″) 0.22
ε 0.56
θ (°) 83.1
rcore (″) 9.6
σv (km s−1) 1199

Smooth component 2

x (″) 42
y (″) −131
rcore (″) 12
σv (km s−1) 756

Galaxy members

(kpc) 7
(km s−1) 248

MACS J0329

Smooth component 1

x (″) 0.04
y (″) 0.02
ε 0.25
θ (°) 86
rcore (″) 4.7
σv (km s−1) 931

Smooth component 2

x (″) 40
y (″) 20
ε 0.52
θ (°) 71
rcore (″) 29
σv (km s−1) 1113

External shear

γshear 0.07
θ (°) −56

Galaxy members

(kpc) 65
(km s−1) 161

MACS J2129

Smooth component 1

x (″) 2.33
y (″) 1.62
ε 0.62
θ (°) −5.5
rcore (″) 11.1
σv (km s−1) 1331

Smooth component 2

x (″) 6.0
y (″) −39.1
ε 0.86
θ (°) 45
rcore (″) 2.3
σv (km s−1) 452

Galaxy members

(kpc) 8
(km s−1) 277

MACS J1115

Smooth component 1

x (″) 1.6
y (″) 2.1
ε 0.49
θ (°) 52
rcore (″) 16
σv (km s−1) 1300

Redshifts

z3 2.8

Galaxy members

(kpc) 28
(km s−1) 152

MACS 0429

Smooth component 1

x (″) 0.52
y (″) 0.00
ε 0.57
θ (°) 79.9
rcore (″) 4.5
σv (km s−1) 1023

Redshifts

z3 1.72

Galaxy members

(kpc) 29
(km s−1) 128

RX J1347

Smooth component 1

x (″) −0.9
y (″) −1.9
ε 0.49
θ (°) 104
rcore (″) 9
σv (km s−1) 1244

Smooth component 2

x (″) −17
y (″) −2
ε 0.80
θ (°) 118
rcore (″) 9
σv (km s−1) 811

External shear

γshear 0.10
θ (°) 81

Redshifts

z5 2.13
z6 3.08
z7 2.48
z8 4.37

Galaxy members

(kpc) 30
(km s−1) 213

MACS J1311

Smooth component 1

x (″) −0.9
y (″) −0.8
ε 0.35
θ (°) 92
rcore (″) 4.9
σv (km s−1) 1015

Redshifts

z2 6.12
z3 2.27

Galaxy members

(kpc) 48
(km s−1) 147

Notes. The values of the velocity dispersion parameters (σv) are rescaled by the factor as described in the lenstool manual (see http://projets.lam.fr/projects/lenstool/wiki/PIEMD). The reference luminosities for the galaxy member parameters ( and , see Eq. (1)) correspond to the rest-frame magnitude of MF160W = −23 for each cluster.

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