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Table 2.

Properties of the sample galaxies extracted by the models.

Object Mtot, e fDM, e fcold, e fcold, 2e ⟨tcold, e⟩ ⟨thot, e⟩ ⟨Zcold, e⟩ ⟨Zhot, e⟩ ∇tcold, e ∇thot, e ∇Zcold, e ∇Zhot, e tinfall
[1010 M⊙] [Gyr] [Gyr] [Z⊙] [Z⊙] [Gyr/Re] [Gyr/Re] Z⊙/Re Z⊙/Re [Gyr ago]
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14)
FCC 083 2.67±0.19 0.40±0.05 0.18±0.02 0.19±0.02 11.8±0.6 11.4±0.5 0.72±0.24 0.38±0.20 −2.52±1.73 −2.92±0.48 −0.99±0.67 −0.91±0.15 8.7±3.1
FCC 119 0.04±0.02 0.66±0.05 0.17±0.06 0.12±0.03 5.9±1.1 4.2±0.5 0.36±0.05 0.43±0.05 18.24±5.75 10.02±1.14 −1.22±0.28 −0.7±0.07 2.4±2.3
FCC 143 0.15±0.03 0.24±0.06 0.06±0.01 0.05±0.01 11.9±1.3 13.0±0.5 0.98±0.71 0.36±0.19 ... −2.05±0.44 ... −0.49±0.25 11.4±1.2
FCC 147 2.88±0.30 0.19±0.03 0.11±0.02 0.12±0.02 12.7±0.8 13.5±0.3 0.91±0.33 0.46±0.13 −2.07±1.87 −1.01±0.26 −1.19±0.84 −1.32±0.04 9.6±3.0
FCC 148 0.56±0.03 0.47±0.03 0.27±0.02 0.33±0.02 4.9±0.6 5.7±0.6 0.90±0.11 0.95±0.18 0.97±2.05 4.13±0.87 −1.37±0.6 −1.47±0.1 3.8±2.4
FCC 153 1.03±0.14 0.43±0.01 0.32±0.01 0.49±0.01 9.4±0.2 9.9±0.6 1.52±0.09 0.51±0.19 3.69±2.11 2.85±0.6 −0.81±0.50 −1.24±0.34 8.9±1.7
FCC 161 1.33±0.07 0.25±0.04 0.10±0.02 0.09±0.02 11.6±1.1 12.9±0.4 0.49±0.14 0.47±0.04 ... −1.41±0.23 ... −0.37±0.03 9.0±3.0
FCC 167 12.16±0.87 0.25±0.03 0.12±0.01 0.20±0.01 11.6±0.1 13.6±0.1 1.95±0.01 1.61±0.01 −4.08±1.88 −0.32±0.28 −0.3±0.83 −0.73±0.13 8.8±3.1
FCC 170 1.31±0.3 0.14±0.02 0.03±0.01 0.15±0.01 13.2±0.6 13.2±0.1 1.05±0.44 0.47±0.03 −0.1±0.20 −0.5±0.08 −0.02±0.30 −0.48±0.08 9.8±3.0
FCC 177 0.74±0.05 0.62±0.03 0.32±0.01 0.30±0.01 6.7±0.4 8.1±0.8 1.25±0.20 0.81±0.23 −0.12±2.80 5.71±0.40 0.65±0.85 −1.30±0.13 6.3±2.2
FCC 179 2.2±0.09 0.19±0.02 0.31±0.02 0.47±0.03 5.0±0.5 7.2±0.7 1.12±0.15 0.77±0.05 1.59±1.59 −2.45±1.03 −1.11±0.67 −0.22±0.10 3.7±2.4
FCC 182 0.05±0.01 0.34±0.08 0.05±0.01 0.03±0.01 11.6±1.3 10.3±0.8 0.81±0.46 0.44±0.09 ... −0.84±0.24 ... −0.3±0.05 10.4±0.9
FCC 249 0.60±0.02 0.17±0.03 0.07±0.03 0.05±0.02 13.3±0.7 12.0±0.5 1.26±1.18 0.37±0.13 ... −1.97±0.25 ... −0.41±0.21 12.3±1.7
FCC 255 0.11±0.01 0.44±0.03 0.12±0.02 0.16±0.02 3.7±2.5 8.2±1.5 0.98±0.27 0.37±0.05 6.42±3.51 3.5±0.93 −0.64±0.32 −0.45±0.06 1.0±1.0
FCC 263 0.21±0.02 0.88±0.01 0.08±0.01 0.10±0.02 ... ... ... ... ... ... ... ... ...
FCC 276 4.23±0.46 0.33±0.04 0.04±0.01 0.03±0.01 13.1±0.7 12.7±0.3 0.79±0.52 0.35±0.05 ... −2.01±0.37 ... 0.74±0.06 9.4±3.0
FCC 290 2.08±0.13 0.68±0.05 0.25±0.03 0.37±0.04 ... ... ... ... ... ... ... ... ...
FCC 301 0.15±0.01 0.28±0.05 0.07±0.01 0.11±0.01 6.4±0.9 7.8±0.8 0.87±0.01 0.38±0.05 1.66±3.80 0.3±0.65 −1.16±0.36 0.35±0.04 6.5±2.1
FCC 308 0.33±0.03 0.51±0.03 0.09±0.01 0.09±0.01 ... ... ... ... ... ... ... ... ...
FCC 312 6.16±0.72 0.63±0.06 0.32±0.04 0.32±0.05 ... ... ... ... ... ... ... ... ...

Notes. (1) Name; (2) total dynamical mass; (3) dark matter fraction; (4) 1Re luminosity fraction of the cold disk; (5) 2Re luminosity fraction of the cold disk; (6) mean age of the cold disk; (7) mean age of the non-disk component; (8) mean metallicity of the cold disk; (9) mean metallicity of the non-disk component; (10) age gradient of the cold disk; (11) age gradient of the non-disk component; (12) metallicity gradient of the cold disk; (13) metallicity gradient of non-disk component. All values in Cols. (2)–(4) and (6)–(13) are calculated within the effective radius Re, except for (5) which is extracted within 2Re. Columns (10) and (12) of FCC 170 and FCC 255 are extracted within the whole data coverage as their disks have very low surface-brightness at r < Re. For five ETGs FCC 143, FCC 161, FCC 182, FCC 249, and FCC 276, we only show the age and metallicity gradient of non-disk component because of the low surface-brightness of cold disk at r < Re. Column (14) gives the infall time into the cluster based on the cold-disk age using a correlation calibrated with TNG50 simulations. For four LTGs FCC 263, FCC 290, FCC 308, and FCC 312, we only have the stellar kinematics and thus only orbital models without coloring.

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