| Galaxy | l | b | d | Vr | M |
| N2403 | 149.6 | 29.3 | 3.3 | 227 | 11.8 |
| N4236 | 12.3 | 47.3 | 3.9 | 118 | 11.5 |
| Circinus | 311.3 | 3.7 | 3.3 | 268 | 11.5 |
| N55 | 332.6 | -75.6 | 1.6 | 96 | 11.5 |
| N7793 | 4.4 | -77.1 | 4.1 | 230 | 11.5 |
| N300 | 299.2 | -79.4 | 2.1 | 101 | 11.3 |
| N1569 | 143.6 | 11.2 | 2.4 | 47 | 11 |
| N404 | 126.9 | -27.1 | 3.6 | 115 | 10.8 |
| N3109 | 262.1 | 23.0 | 1.3 | 194 | 10.5 |
| IC5152 | 343.8 | -50.1 | 1.7 | 85 | 10 |
| SexA,B | 240.3 | 42.0 | 1.4 | 165 | 10 |
| N6822 | 25.3 | -18.3 | 0.5 | 45 | 10 |
| N1311 | 264.2 | -52.6 | 3.1 | 425 | 9.8 |
| IC1613 | 129.7 | -60.5 | 0.7 | -155 | 9.8 |
| WLM | 75.8 | -73.6 | 0.9 | -65 | 9.7 |
| VIIZw403 | 127.8 | 37.3 | 4.5 | 50 | 9.6 |
| SagDIG | 21.0 | -16.5 | 1.1 | 7 | 9.1 |
| PegDIG | 94.7 | -43.5 | 0.8 | -22 | 8.9 |
| LeoA | 196.8 | 52.4 | 0.7 | -18 | 8.8 |
| DDO210 | 34.0 | -31.3 | 0.9 | -24 | 8.7 |
| DDO155 | 310.8 | 76.9 | 1.5 | 183 | 8.6 |
| Phoenix | 272.0 | -68.9 | 0.4 | -34 | 7.7 |
This sample is added to the sample of Table 2. The effect of these galaxies can be considered as a perturbation. The coordinates l and b are in  ,
the distances d are in Mpc (as in the previous table
we omit the uncertainties on the distances and velocities), the
radial velocity Vr is in km s-1, and the galaxy masses are in solar
units. They are expressed as  .
|