[guided]The reason for introducing $R_\delta$ is that weak convergence in $\ell^\infty(\mathcal F)$ is infinite-dimensional, while the hypothesis only gives finite-dimensional convergence. Total boundedness supplies the bridge: every $f\in\mathcal F$ is within $d_P$-distance $\delta$ of one of finitely many points.
Formally, because $(\mathcal F,d_P)$ is totally bounded, for the fixed number $\delta>0$ there are functions $f_{\delta,1},\dots,f_{\delta,N_\delta}\in\mathcal F$ such that every $f\in\mathcal F$ satisfies
\begin{align*}
d_P(f,f_{\delta,j})<\delta
\end{align*}
for at least one index $j\in\{1,\dots,N_\delta\}$. We choose one such index for each $f$ and denote the chosen net point by $\pi_\delta(f)$. This defines a map
\begin{align*}
\pi_\delta:\mathcal F\to\{f_{\delta,1},\dots,f_{\delta,N_\delta}\}.
\end{align*}
Given a [bounded function](/page/Bounded%20Function) $z:\mathcal F\to\mathbb R$, define
\begin{align*}
R_\delta z:\mathcal F\to\mathbb R
\end{align*}
by
\begin{align*}
(R_\delta z)(f):=z(\pi_\delta(f)).
\end{align*}
This replacement is constant on the cells of the finite net, so it depends only on the finitely many coordinates $z(f_{\delta,1}),\dots,z(f_{\delta,N_\delta})$.
The approximation error is controlled by the local $d_P$-oscillation of $z$. Indeed, for every $f\in\mathcal F$ the chosen net point satisfies $d_P(f,\pi_\delta(f))<\delta$, hence
\begin{align*}
|z(f)-(R_\delta z)(f)|=|z(f)-z(\pi_\delta(f))|\le \sup_{\substack{u, v\in\mathcal F, d_P(u, v)<\delta}}|z(u)-z(v)|.
\end{align*}
Taking the supremum over $f\in\mathcal F$ gives
\begin{align*}
\|z-R_\delta z\|_{\mathcal F}\le \sup_{\substack{u, v\in\mathcal F, d_P(u, v)<\delta}}|z(u)-z(v)|.
\end{align*}
This is the exact point where asymptotic equicontinuity will enter.[/guided]