Table C.1.
Model parameter priors and inferred values from observed image positions and stellar velocity dispersion measurements.
| Parameter | Description | Prior | iso_halo | PL_halo | iso_halo+sheet | iso_halo+ell_BCG | baseline |
|---|---|---|---|---|---|---|---|
| Scaling relation (IDphot = 115) | |||||||
| σv, 115 [km/s] | velocity dispersion | 𝒢(206,25) |
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180 ± 21 | 170 ± 21 |
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| rt, 115 [″] | truncation radius | flat(1.8,40) |
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| BCG | |||||||
| (xBCG, yBCG) [″] | centroid | exact | (0, 0) | (0, 0) | (0, 0) | (0, 0) | (0, 0) |
| qBCG | axis ratio | exact or flat(0.4,1) | 1 | 1 | 1 |
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1 |
| ϕBCG [°] | position angle | flat(0,360) | — | — | — | 36 ± 63 | — |
| θE, ∞, BCG [″] | Einstein radius | 𝒢(3.08,0.32)† |
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| rt, BCG [″] | truncation radius | flat(1,50) |
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| Cluster member not in scaling relation | |||||||
| (x116, y116) [″] | centroid | exact | (0.314, 9.819) | (0.314, 9.819) | (0.314, 9.819) | (0.314, 9.819) | (0.314, 9.819) |
| q116 | axis ratio | exact | 1 | 1 | 1 | 1 | 1 |
| θE, ∞, 116 [″] | Einstein radius G1 | 𝒢(1.67,0.19)† | 1.6 ± 0.2 | 1.6 ± 0.2 | 1.6 ± 0.2 | 1.6 ± 0.2 | 1.6 ± 0.2 |
| rt, 116 [″] | truncation radius | flat(0.05,10) |
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1.1 ± 0.4 |
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| Jellyfish galaxies | |||||||
| (xJF1, yJF1) [″] | centroid | exact | (19.094, −13.361) | (19.094, −13.361) | (19.094, −13.361) | (19.094, −13.361) | (19.094, −13.361) |
| θE, ∞, JF1 [″] | Einstein radius | flat(0.01,10) | 0.25 ± 0.07 | 0.25 ± 0.08 |
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| rt, JF1 [″] | truncation radius | exact | 5 | 5 | 5 | 5 | 5 |
| (xJF2, yJF2) [″] | centroid | exact | (−5.114, 6.941) | (−5.114, 6.941) | (−5.114, 6.941) | (−5.114, 6.941) | (−5.114, 6.941) |
| θE, ∞, JF2 [″] | Einstein radius | flat(0.01,10) |
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0.63 ± 0.14 |
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| rt, JF2 [″] | truncation radius | exact | 5 | 5 | 5 | 5 | 5 |
| (xJF3, yJF3) [″] | centroid | exact | (−1.649, 2.597) | (−1.649, 2.597) | (−1.649, 2.597) | (−1.649, 2.597) | (−1.649, 2.597) |
| θE, ∞, JF3 [″] | Einstein radius | flat(0.01,10) |
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| rt, JF3 [″] | truncation radius | exact | 5 | 5 | 5 | 5 | 5 |
| Foreground galaxy | |||||||
| (xfg, yfg) [″] | centroid | exact | (−0.868, −16.564) | (−0.868, −16.564) | (−0.868, −16.564) | (−0.868, −16.564) | (−0.868, −16.564) |
| θE, ∞, fg [″] | Einstein radius | flat(0.1,10) |
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0.24 ± 0.04 |
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0.20 ± 0.03 |
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| rt, fg [″] | truncation radius | flat(0.1,40) |
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| Background galaxy | |||||||
| (xbkg, ybkg) [″] | centroid | exact | (6.871, 3.843) | (6.871, 3.843) | (6.871, 3.843) | (6.871, 3.843) | (6.871, 3.843) |
| θE, ∞, bkg [″] | Einstein radius | 𝒢(1.66,0.10)† |
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1.67 ± 0.09 | 1.64 ± 0.10 |
| rt, bkg [″] | truncation radius | flat(0.1,40) |
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22 ± 12 |
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| Dark matter halos | |||||||
| xDM1 [″] | x centroid | flat(−20,20) | −0.1 ± 0.3 | −0.2 ± 0.3 | −0.1 ± 0.3 | −0.3 ± 0.3 | 0.1 ± 0.3 |
| yDM1 [″] | y centroid | flat(−20,20) | −1.2 ± 0.5 |
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−1.1 ± 0.4 |
| qDM1 | axis ratio | flat(0.2,1) | 0.64 ± 0.02 | 0.64 ± 0.02 | 0.63 ± 0.02 |
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0.63 ± 0.02 |
| ϕDM1 [°] | position angle | flat(0,360) | 43 ± 1 |
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44 ± 2 |
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45 ± 2 |
| θE, ∞, DM1 [″] | Einstein radius | flat(0,50) |
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— |
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| E [″] | halo strength | flat(0,50) | — | 13 ± 2 | — | — | — |
| rc, DM1 [″] | core radius | flat(0,50) |
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6.6 ± 0.8 |
| γ | radial slope | flat(0.,2.) | — | 0.51 ± 0.03 | — | — | — |
| xDM2 [″] | x centroid | flat(−30,30) |
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| yDM2 [″] | y centroid | flat(−30,30) |
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−22 ± 4 |
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| qDM2 | axis ratio | flat(0.2,1) |
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| ϕDM2 [°] | position angle | flat(0,360) |
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145 ± 3 |
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141 ± 4 |
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| θE, ∞, DM2 [″] | Einstein radius | flat(0,50) |
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23 ± 6 |
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| rc, DM2 [″] | core radius | flat(0,70) |
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24 ± 5 |
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| Mass sheet | |||||||
| κ0 | mass sheet | flat(−1,1) | — | — |
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— | — |
Notes. Columns 1 and 2 are the parameter and description. Column 3 is the prior on the parameter, where the letter 𝒢 denotes a Gaussian prior, with its center and 1σ width in parentheses. The Gaussian priors on the Einstein radii with a † symbol are based on the first version of velocity dispersion measurements from Granata et al. (2025) using an older version of stellar template libraries; the final velocity dispersion measurements change by ≲1 km s−1, which has negligible effect on the modeling results. Columns 4 to 7 list the inferred parameter values of the corresponding mass models indicated in the header line. Parameter values that have no uncertainties are parameters that are fixed with priors listed as ‘exact’. A dashed line in the parameter value indicates that the parameter is not present in the particular mass model. Position angles are measured east of north in degrees.
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