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Table C.1.

Main morphological, photometric, and kinematic properties of the F3D galaxies.

Object Morph. mr Re M* Rproj/Rvir cz Rmax/Re PAkin ΔPA Kinem. σe λRe ϵe Kinem. Altern.
Type Structure Type Name
(mag) (arcsec) (1010M) (km s−1) (deg) (deg) (km s−1)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14) (15) (16)
FCC 083 E5 10.84 35.7 ... 0.83 1532 ± 1 2.0 142 ± 1 2 ± 1 RR 103 0.51 0.35 FR NGC 1351
FCC 090 E4 pec 13.62 12.1 0.08 0.82 1832 ± 1 2.2 188 ± 12 72 ± 13 NR 33 0.17 0.20 FR ...
FCC 113 ScdIII pec 14.44 20.6 0.02 0.62 1395 ± 1 1.9 2 ± 5 −11 ± 8 RR ... 0.36 0.40 FR ESO 358-G015
FCC 119 S0 pec ... 17.4 0.1 1.39 1409.7 ± 0.4 1.5 43 ± 6 1 ± 7 RR 17 0.33 0.07 FR ...
FCC 143 E3 12.66 11.0 0.28 0.37 1379 ± 1 2.4 188 ± 3 0 ± 3 DC 62 0.14 0.04 FR NGC 1373
FCC 147 E0 10.50 24.8 2.40 0.32 1350 ± 1 2.6 123 ± 2 2 ± 3 RR 131 0.22 0.04 FR NGC 1374
FCC 148 S0 11.70 28.3 0.58 0.32 777 ± 1 2.1 264 ± 2 −3 ± 4 RR 43 0.65 0.60 FR NGC 1375
FCC 153 S0 11.70 19.8 0.76 0.57 1642 ± 1 3.2 82 ± 2 −1 ± 3 RR 55 0.73 0.65 FR IC 1963
FCC 161 E0 10.47 28.6 2.63 0.24 1369 ± 1 2.0 179 ± 2 −4 ± 5 RR 96 0.19 0.02 FR NGC 1379
FCC 167 S0/a 9.27 56.4 9.85 0.30 1878 ± 2 1.9 186 ± 1 1 ± 1 RR 143 0.53 0.49 FR NGC 1380
FCC 170 S0 10.99 15.9 2.25 0.20 1743 ± 2 4.3 138 ± 1 −3 ± 2 RR 113 0.45 0.50 FR NGC 1381
FCC 176 SBa 11.74 53.7 0.68 0.43 1428 ± 1 0.7 170 ± 5 −15 ± 7 RR 46 0.46 0.15 FR NGC 1369
FCC 177 S0 11.80 35.9 0.85 0.38 1591 ± 1 1.6 180 ± 3 5 ± 4 RR 42 0.69 0.70 FR NGC 1380A
FCC 179 Sa 10.68 30.0 1.58 0.32 915 ± 4 3.0 24.7 ± 0.4 7 ± 1 KDC 70 0.77 0.50 FR NGC 1386
FCC 182 SB0 pec 13.58 9.9 0.15 0.15 1705.1 ± 0.4 2.2 151 ± 13 −25 ± 15 DC 39 0.17 0.05 FR ...
FCC 184 SB0 10.00 35.5 4.70 0.15 1302.6 ± 0.6 2.5 54 ± 3 36 ± 4 KDC 143 0.19 0.10 FR NGC 1387
FCC 190 SB0 12.26 18.3 0.54 0.18 1794 ± 1 2.1 128 ± 3 −83 ± 4 RR 75 0.32 0.20 FR NGC 1380B
FCC 193 SB0 10.69 28.2 3.32 0.19 976 ± 1 2.0 221 ± 1 9 ± 1 KDC 95 0.55 0.40 FR NGC 1389
FCC 219 E2 8.57 161.0 12.7 0.08 1933 ± 2 0.5 153 ± 1 10 ± 1 RR 154 0.22 0.20 FR NGC 1404
FCC 249 E0 ... 9.6 0.5 1.02 1579 ± 1 3.3 156 ± 5 2 ± 12 DC 104 0.08 0.04 FR NGC 1419
FCC 255 S0 ... 13.8 0.5 0.85 1328 ± 3 2.7 −7 ± 3 0 ± 3 RR 38 0.41 0.77 FR ESO 358-G050
FCC 263 SBcdIII 12.70 27.2 0.04 0.41 1746 ± 2 1.4 165 ± 10 −33 ± 12 RR 28 0.60 0.50 FR ESO 358-G051
FCC 276 E4 10.15 44.7 1.81 0.38 1434 ± 1 1.7 73 ± 3 −5 ± 3 DC 123 0.09 0.31 SR NGC 1427
FCC 277 E5 12.34 12.8 0.34 0.42 1657 ± 2 2.6 116 ± 4 3 ± 2 RR 80 0.77 0.36 FR NGC 1428
FCC 285 SdIII 13.02 49.9 0.02 0.60 901 ± 1 0.7 124 ± 7 40 ± 10 RR ... 0.41 0.20 FR NGC 1437A
FCC 290 ScII 11.08 48.5 0.64 0.54 1398 ± 4 1.5 152 ± 3 −3 ± 4 RR 39 0.60 0.30 FR NGC 1436
FCC 301 E4 12.65 11.7 0.20 0.70 1043 ± 2 2.3 153 ± 3 −2 ± 3 DC 49 0.36 0.20 FR ESO 358-G059
FCC 306 SBmIII 15.18 9.7 0.01 0.83 902 ± 34 1.7 2 ± 7 −47 ± 9 PR 69 0.12 0.40 FR ...
FCC 308 Sd 12.54 37.1 0.04 0.85 1519 ± 2 1.3 10 ± 2 5 ± 3 RR 43 0.33 0.60 FR NGC 1437B
FCC 310 SB0 11.81 35.6 0.54 0.97 1383 ± 1 1.0 219 ± 5 −35 ± 5 RR 48 0.46 0.27 FR NGC 1460
FCC 312 Scd 10.89 109.5 1.48 0.82 1937 ± 4 1.0 −47 ± 1 3 ± 1 RR 63 0.74 0.50 FR ESO 358-G063

Notes. (1) and (2) Galaxy name and morphological type from Ferguson (1989). (3)–(5) Total r-band magnitude, r-band effective radius, and total stellar mass from Iodice et al. (2019) for ETGs and Raj et al. (2019) for LTGs. (6) Ratio between the projected distance from the cluster centre and virial radius of the cluster (Rvir = 0.7 Mpc, Drinkwater et al. 2001). (7) Heliocentric systemic velocity from the stellar velocity field. (8) Ratio between the maximum radial extension of the MUSE data along the galaxy major axis and the r-band effective radius. (9) and (10) Kinematic position angle and difference with respect to the photometric position angle from Iodice et al. (2019). (11) Kinematic structure following the classification by Krajnović et al. (2011): RR = regularly rotating galaxy, NR = non-rotating galaxy, DC = galaxy with a distinct core, KDC = galaxy with a kinematically decoupled core, PR = prolate rotating galaxy. (12) Average stellar velocity dispersion inside the r-band effective radius. (13) Effective stellar angular momentum. (14) Ellipticity at the effective radius. (15) Kinematic type following the classification by Emsellem et al. (2011): FR = fast-rotating galaxy, SR = slowly-rotating galaxy. (16) Galaxy alternative name.

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