Two-point correlation function models are derived from the power spectrum models introduced in Sect. 4, using the parameter values listed in Table 2. The top panel illustrates the galaxy auto-two-point correlation function ${\xi }_{\mathit{gg}}^{\ell }$, the middle panel presents the monopole of the galaxy auto-velocity correlation function Ψ, and the bottom panel displays the dipole component of the galaxy-velocity cross-correlation function ${\xi }_{\mathit{gv}}^1$.