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The expansion center Universe (ECU) gives a dipole anisotropy to the Hubbleratio, at any Hubble depth D. After a long series of successful dipole tests,here is a crucial multiple dipole test at z bins centred on the mean <z>=z0=1,or Hubble depth D=c/H0, and based on data from SCP Union & Union2 compilation.Table 5abc lists data of two main samples, with 48 SCPU SNe Ia and 58 SCPU2 SNeIa respectively. The confirmed dipole anisotropy, shown by 6 primary sampletests and by another 27 from 9 encapsulated z bins with DL=D(1+z) assumed andthe Hubble Magnitude definition, gives a model independent result, in fullaccordance with the expansion center model (ECM). That means a maximum cz rangeof about 50000 km/s at the central redshift z0=1. As a complement to the dipoletests, here is a new computation of the relativistic deceleration parameter q0,based on the extrapolated total M spread, that is the deviation of the HubbleMagnitude M of high-z SCP Union supernovae at a normal or central redshift<z>=z0=z << 1 from the absolute magnitude M0 at z0=0 (cf. parallel paper XVI).A total M spread according to ECM is derived from 249 high-z SCPU SNe listed inpaper XVI. In a concordance test with the expansion center model, the obtainednew relativistic q0 agrees with the value q0=+2 inferred from the ECM paper Ieq. (41), when R0 is the proper distance at t0 of the expansion center from theGalaxy.

A crucial dipole test of the expansion center Universe - based on high-z SCP Union & Union2 supernovae