Table 1.
Properties of the sample galaxies.
| Object | Type | Distance | Re | M⋆ | i | PA | S/N | |
|---|---|---|---|---|---|---|---|---|
| [Mpc] | [kpc] | [1010 M⊙] | [°] | [°] | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | |
| FCC 083 | E5 | 19.2 | 3.46 | 2.27 | 68.2±13.3 | 139.7 | 100 | |
| FCC 119 | S0 | 20.9 | 1.17 | 0.05 | 64.9±5.4 | 45.4 | 40 | |
| FCC 143 | E3 | 19.3 | 1.07 | 0.28 | 64.6±7.1 | 124.6 | 60 | |
| FCC 147 | E0 | 19.6 | 2.40 | 2.40 | 33.3±6.0 | 120.9 | 100 | |
| FCC 148 | S0 | 19.9 | 2.74 | 0.58 | 75.8±3.1 | 89.2 | 60 | |
| FCC 153 | S0 | 20.8 | 1.92 | 0.76 | 87.5±0.1 | 82.6 | 100 | |
| FCC 161 | E0 | 19.9 | 2.77 | 2.63 | 33.1±3.3 | 0.0 | 100 | |
| FCC 167 | S0/a | 21.2 | 5.47 | 9.85 | 78.0±2.1 | 5.0 | 100 | |
| FCC 170 | S0 | 21.9 | 1.54 | 2.25 | 84.9±1.5 | −42.0 | 100 | |
| FCC 177 | S0 | 20.0 | 3.48 | 0.85 | 85.8±1.3 | 177.8 | 100 | |
| FCC 179 | Sa | 20.9 | 2.91 | 1.58 | 69.9±0.7 | 64.34 | 100 | |
| FCC 182 | SB0 | 19.6 | 0.96 | 0.15 | 63.2±4.4 | 169.3 | 60 | |
| FCC 249 | E0 | 20.9 | 0.93 | 0.98 | 37.8±4.1 | 150.6 | 60 | |
| FCC 255 | S0 | 20.9 | 1.34 | 0.31 | 78.1±5.8 | 172.9 | 60 | |
| FCC 263 | SBcdIII | 20.9 | 2.64 | 0.04 | 66.4±1.9 | 87.9 | 60 | |
| FCC 276 | E4 | 19.6 | 4.33 | 1.81 | 66.6±9.0 | 75.4 | 100 | |
| FCC 290 | ScII | 20.9 | 4.70 | 0.64 | 52.8±1.1 | 122.5 | 60 | |
| FCC 301 | E4 | 19.7 | 1.13 | 0.20 | 82.0±5.7 | 155.8 | 60 | |
| FCC 308 | Sd | 20.9 | 3.60 | 0.04 | 73.5±1.4 | 88.5 | 60 | |
| FCC 312 | Scd | 20.9 | 10.62 | 1.48 | 81.0±0.9 | 136.2 | 100 |
Notes. (1) Name; (2) Hubble type taken from Ferguson (1989); (3) distance; (4) effective radius; and (5) stellar mass is from Iodice et al. (2019b) and Martín-Navarro et al. (2021); (6) the inclination angle obtained from our orbit-superposition model; (7) the positional angle determined by photometric isophotes and adopted for the multi-Gaussian expansion fitting; and (8) target S/N used in binning the spectra to obtain kinematic maps.
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