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Table 1.

Main sample properties.

Object Alt. Type Distance M Nbins
(Mpc) (1010M)
(1) (2) (3) (4) (5) (6)
FCC 083 NGC 1351 E5 19.2 2.27 1475
FCC 119 S0 20.9 0.05 32
FCC 143 NGC 1373 E3 19.3 0.28 252
FCC 147 NGC 1374 E0 19.6 2.40 3515
FCC 148 NGC 1375 S0 19.9 0.58 625
FCC 153 IC 1963 S0 20.8 0.76 804
FCC 161 NGC 1379 E0 19.9 2.63 2069
FCC 167 NGC 1380 S0/a 21.2 9.85 6154
FCC 170 NGC 1381 S0 21.9 2.25 2013
FCC 176 NGC 1369 SBa 20.9 0.68 114
FCC 177 S0 20.0 0.85 799
FCC 179 NGC 1386 Sa 20.9 1.58 1804
FCC 182 SB0 19.6 0.15 71
FCC 184 NGC 1387 SB0 19.3 4.70 8862
FCC 190 NGC 1382 SB0 20.3 0.54 900
FCC 193 NGC 1389 SB0 21.2 3.32 2804
FCC 219 NGC 1404 E2 20.2 12.7 5997
FCC 249 NGC 1419 E0 20.9 0.98 654
FCC 255 S0 20.9 0.31 324
FCC 276 NGC 1427 E4 19.6 1.81 2748
FCC 277 NGC 1428 E5 20.7 0.34 478
FCC 301 E4 19.7 0.20 238
FCC 310 NGC 1460 SB0 20.9 0.54 607

Notes. (1), (2) and (3) come from Ferguson (1989). (4) When available, distances come from Iodice et al. (2019b). Otherwise, a fixed distance from the Fornax cluster of 20.9 Mpc is assumed. (5) Stellar masses as listed in Iodice et al. (2019a). (6) Number of independent Voronoi bins used in our analysis (see Sect. 3).

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