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Table 4.
Number of galaxies and repetitions in each group obtained when applying UMSCANGALACTIK to the mixture of the kinematic maps for the same galaxies observed at three different inclinations.
C0 | C1 | C2 | C3 | C4 | C5 | |
---|---|---|---|---|---|---|
Cluster size | 308 | 1890 | 303 | 2047 | 528 | 887 |
N° of distinct galaxies | 154 | 672 | 174 | 749 | 224 | 369 |
N° of galaxies not repeated | 65 | 29 | 102 | 39 | 53 | 73 |
N° of galaxies repeated twice | 24 | 68 | 15 | 122 | 38 | 74 |
N° of galaxies repeated three times | 65 (42 per cent) | 575 (86 per cent) | 57 (33 per cent) | 588 (79 per cent) | 133 (59 per cent) | 222 (60 per cent) |
Notes. The percentage of well-classified galaxies is included.
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