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It is shown here that a model for inertial mass, called quantised inertia, orMiHsC (Modified inertia by a Hubble-scale Casimir effect) predicts therotational acceleration of the 153 good quality galaxies in the SPARC dataset(2016 AJ 152 157), with a large range of scales and mass, from just theirvisible baryonic matter, the speed of light and the co-moving diameter of theobservable universe. No dark matter is needed. The performance of quantisedinertia is comparable to that of MoND, yet it needs no adjustable parameter. Asa further critical test, quantised inertia uniquely predicts a specificincrease in the galaxy rotation anomaly at higher redshifts. This test is nowbecoming possible and new data shows that galaxy rotational accelerations doincrease with redshift in the predicted manner, at least up to Z=2.2.

Galaxy rotations from quantised inertia and visible matter only