Kinematics of the bulge RRLs compared with the data of K22 using our approach. Top panels: Rotation curve of the bulge-confined RRLs of our sample separated by those farther away (dashed red line) and those more centrally concentrated (dashed grey line). The rotation curves from K22 using our orbital selection are also presented where with green crosses are the inner bulge and white circles for the central bulge RRLs. Bottom panels: The velocity dispersion curves using the same symbols. The velocity dispersion of the central bulge RRLs from K22 have larger errors because there are fewer stars per bin.