Table 4: Velocities and positions of the galaxies used in the minimization procedure.
Galaxy $v_x^{\rm G}$ $v_y^{\rm G}$ $v_x^{\rm G}$ $x^{\rm G}$ $y^{\rm G}$ $z^{\rm G}$
name km s-1 km s-1 km s-1 kpc kpc kpc
IC 342 -294.7 80.0 -21.1 1309.6 1176.0 -368.2
Maffei -359.1 97.1 -66.1 1426.0 1427.6 -999.7
Andromeda 125.5 -25.9 -85.1 -742.5 -381.6 -1255.0
Milky Way 117.3 -67.0 -65.7 -1108.5 -986.0 -975.3
M 81 -391.3 49.8 97.4 1098.3 731.9 1447.3
Cen A 725.4 -200.7 83.4 -2728.4 -2951.1 -78.4
Sculptor 822.1 -51.7 149.5 -1044.7 -760.5 2216.2
M 83 618.0 -250.6 89.1 -3807.0 -3684.5 1409.4
The masses have been taken from Table 2. The positions are referred
to the barycentre of the sample located at ${\vec x}_{\rm G} = \left\{ {{\rm 1117}{\rm , 986}{\rm , 975}} \right\}$ kpc.

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