  We test the Grumiller's quantum motivated modified gravity model, which at
large distances modifies the Newtonian potential and describes the galactic
rotation curves of disk galaxies in terms of a Rindler acceleration term
without the need of any dark matter, against the baryonic Tully-Fisher feature
that relates the total baryonic mass of a galaxy with flat rotation velocity of
the galaxy. We estimate the Rindler acceleration parameter from observed
baryonic mass versus rotation velocity data of a sample of sixty galaxies.
Grumiller's model is found to describe the observed data reasonably well.
