Kinematic and orbital properties for RR Lyrae variables, nonvariable giants, and stellar particles from the simulation. The top panels show the distribution of average v_GV and its dispersion σ_vGV across the Galactic longitude bins. The middle and bottom panels display the distribution of orbital properties z_max vs. r_apo for RR Lyrae (middle left panel), nonvariable giants (middle right panel), and model HG1 (bottom left panel, at 10 Gyr). The color-coding in all panels is based on ${\mathrm{\Omega }}_{\phi }^{\text{rot}}$. The black dashed lines in the top panels represent the rotation and dispersion curve based on the bar model Shen et al. (2010) for b = 4 deg.