Comparison of the magnitude of the Newtonian gravity from two Milky Way models, the Miyamoto-Nagai model a_MN (Eq. (13)), and a model using exponential disks, a_Exp, similar to that of Banik & Zhao (2018) (Eqs. (14) and (15)) at the position of the eight dwarf galaxies. The model parameters for the two models are given in Table 2. The black line is a one-to-one line. We see that the two models give similar gravitational strengths.