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Table 3
Distance grouping of primary galaxies (brighter than MR = −20).
| Set ID | Minor axis range [Mpc] | Number of galaxies |
| (1) | (2) | (3) |
|
|
||
| Inner | ]0.25, 0.5] | 31 |
| Outer | ]0.5, 0.75] | 24 |
| Outer II | ]0.75, 1] | 17 |
| Outer III | ]1, 1.5] | 31 |
| Outer IV | ]1.5, 2] | 34 |
| Outer V | ]2, 2.5] | 20 |
| Outer VI | ]2.5, 3] | 26 |
| Outer VII | ]3, 3.5] with restriction of a<3.9 Mpc | 14 |
Notes. The columns list the following: (1) name of the set; (2) range for the primary minor axis b; (3) number of galaxies in each subsample. The whole set of elliptical annuli is also shown in the Coma cluster map of WGL11 data, Fig. 2.
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