Table D.1.
Relevant measurements and values for the 17 cluster members with more than two measurements in their LOS velocity dispersion profiles.
| A2744 | ||||||||||
| dPIE-J | NFW-J | |||||||||
| Gal ID | z | mF160W | ReF814W | σ0 | rt | ![]() |
ρ0 | rs | ![]() |
zscore |
| [kpc] | [km s−1] | [kpc] | [km s−1] | [109 M⊙ kpc−3] | [kpc] | [km s−1] | ||||
| 34423 | 0.303 | 17.68 | 3.53 | ![]() |
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2.71 |
| 36527 | 0.316 | 18.08 | 2.75 | ![]() |
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0.91 |
| 38010 | 0.317 | 18.76 | 1.53 | ![]() |
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0.07 |
| 38067 | 0.317 | 18.18 | 3.24 | ![]() |
Flat | ![]() |
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3.20 |
| 38117 | 0.299 | 18.60 | 1.71 | ![]() |
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![]() |
0.89 |
| 38729 | 0.319 | 19.20 | 2.83 | ![]() |
Flat | ![]() |
![]() |
![]() |
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1.27 |
| 39428 | 0.300 | 18.20 | 3.13 | ![]() |
![]() |
![]() |
![]() |
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0.82 |
| 40689 | 0.301 | 17.02 | 7.26 | ![]() |
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2.55 |
| 41950 | 0.317 | 18.44 | 1.94 | ![]() |
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![]() |
![]() |
![]() |
0.94 |
| 42443 | 0.303 | 18.77 | 2.56 | ![]() |
Flat | ![]() |
![]() |
![]() |
![]() |
1.73 |
| M0416 | ||||||||||
| dPIE-J | NFW-J | |||||||||
| Gal ID | z | mF160W | ReF814W | σ0 | rt | ![]() |
ρ0 | rs | ![]() |
zscore |
| [kpc] | [km s−1] | [kpc] | [km s−1] | [109 M⊙ kpc−3] | [kpc] | [km s−1] | ||||
| 80726 | 0.402 | 17.78 | 5.09 | ![]() |
Flat | ![]() |
![]() |
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12.82 |
| 81838 | 0.396 | 19.08 | 1.11 | ![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
1.55 |
| 81883 | 0.406 | 19.44 | 1.85 | ![]() |
Flat | ![]() |
![]() |
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2.93 |
| 82063 | 0.395 | 17.96 | 4.37 | ![]() |
![]() |
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3.87 |
| 83064 | 0.397 | 18.91 | 2.83 | ![]() |
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1.33 |
| 85770 | 0.406 | 19.59 | 1.78 | ![]() |
![]() |
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![]() |
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1.23 |
| −22 | 0.397 | 17.79 | 4.64 | ![]() |
Flat | ![]() |
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2.21 |
Notes. We report each galaxy ID, redshift, apparent magnitude in the F160W band, and circularized effective radius in the F814W band that were presented in Tortorelli et al. (2023) and Granata et al. (2026). We also list the values of the parameters σ0 and rt inferred with the dPIE-J dynamical models; and ρ0 and rs inferred with the NFW-J dynamical models. The maximum circular velocities are indicated with
, with the zscore to compare their distributions. We highlight the ID of the galaxies in the RS sample.
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