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Table 5.

Modelled lens and source parameter values for the different configurations of the composite mock data (presented in Sect. 3.2.4), with kinematic data having a signal-to-noise of 15 in the brightest pixel and binned to have a signal-to-noise of 30 in each bin (shown in Fig. 11).

Parameter description Parameter Input Prior LD composite L composite LD power-law L power-law
Source

Light
x centroid xc, s [″] 4.1058 (2.5,5.5)
y centroid yc, s [″] 3.4667 (2.,5.)
Axis ratio qs 0.850 (0.5,1.)
Position angle θs [radians] 0.00
Intensity Ie, s [counts] 200. (120,250)
Effective radius Reff, s [″] 0.5 (0.2,2.)
Sersic index ns 4.00 (0.5,10.)

Mass
Anisotropy β −0.15 (−0.3,0.3)
Inclination i [radians] 0.10 (0.,0.2))
Axis ratio 0.90 (0.5,1.)
Einstein radius [″] 1.15 (0.,5)

Lens

Light
Axis ratio ql 0.768 (0.2,1.)
Intensity Ie, l [counts] 965. (800.,1100.)
Effective radius Reff, l [″] 0.90 (0.3,2.)
Sersic index nl 4.00 (0.5,10.)

Mass (composite)
x centroid xc, l [″] 4.4108 (4.,5.)
y centroid yc, l [″] 4.0112 (3.5,5.5)
Axis ratio ql, 1 0.883 (0.2,1.)
Position angle θl [radians] 0.551
Chameleon parameter wc, 1 [″] 2.03 (0,10)
Chameleon parameter wt, 1 [″] 2.47 (0,10)
Axis ratio ql, 2 0.847 (0.2,1.)
Chameleon parameter wc, 2 [″] 0.06 (0,10)
Chameleon parameter wt, 2 [″] 0.67 (0,10)
x centroid [″] 4.39 (3.5,5.)
y centroid [″] 3.90 (3.5,5.)
Axis ratio 0.734 (0.3,1.)
Position angle [radians] 3.593
Einstein radius [″] 0.399 (0.,5.)
Scale radius [″] 23.7 Gaussian (18.6,2.6)
Mass-to-light ratio 4.10 (2.5,6.5)

Mass (power law)
x centroid [″] (4.,5.)
y centroid [″] (3.5,5.5)
Axis ratio (0.2,1.)
Position angle [radians]
Einstein radius [″]
Slope (0.2,0.8)

External shear
Strength γext, ∞ 0.151 (0.,0.3)
Position angle ϕext [radians] 1.416 (−3.1415,3.1415)

0.99 0.99 1.03 1.02
0.99 1.25
0.99 0.99 1.03 1.02

Notes. The model presented are that including both the lensing and dynamics constraints (LD composite), that including only the lensing ones (L composite), and the two power-law models, with lensing and dynamics constraints (LD power-law) and with those from lensing only (L power-law). Parameters are presented with the 1σ uncertainties.

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