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Table 1.

dPIE parameters.

Model Δ RA Δ Dec e θ σ rcore rs
(″) (″) (km s−1) (″) (″)
DM 0.32 ± 0.21 –1.13 ± 0.27 0.74 ± 0.02 54.6 ± 0.3 904 ± 15 14.1 ± 0.7 [325]
(0.37) (–1.0) (0.72) (54.9) (895) (14.0)

BCG 0.59 ± 0.13 –0.13 ± 0.17 289 ± 11 [0] [10.0]
(0.37) (–0.06) (284)

Gas #1 3.15 ± 0.38 13.24 ± 0.67 0.51 ± 0.03 68.3 ± 1.8 168 ± 5 18.1 ± 0.8 [270]
(2.69) (12.69) (0.50) (68.7) (172) (18.7)

Gas #2 –12.5 ± 1.9 –41.7 ± 2.3 0.81 ± 0.02 45.8 ± 1.2 272 ± 12 62.4 ± 3.8 [270]
(–9.1) (–39.0) (0.82) (46.3) (270) (64.0)

Gas #3 –68.5 ± 1.5 –49.9 ± 3.6 0.20 ± 0.09 126.5 ± 11.3 328 ± 10 110.7 ± 5.7 [270]
(–68.7) (–52.3) (0.25) (127.8) (325) (325.5)

Notes. dPIE parameters inferred for the mass model of AC 114, constrained using both SL and X-ray constraints, with an RMS equal to 0.43″. Error bars on all parameters quoted in this paper correspond to ±1σ confidence levels inferred from the MCMC optimisation. Coordinates are given in arcseconds relative to α = 344.701518, δ = –34.802364; e and θ are the ellipticity and position angle of the mass distribution. Each parameter is given as the median with the best fit value in parenthesis except the ones fixed a priori that are shown in brackets. For an L* galaxy, we have σ = 187 ± 5 km s−1 and rs = 11 ± 1.2″. The external shear component is equal to 0.11 ± 0.01, with an angle of 138.1 ± 0.8.

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