Alcubierre's warped metric in ($1+1$)D is typically given in the form of:
$$ds^2 = -dt^2 + [dx-v(t)f(r) dt]^2 \ \ .$$
Then it is nicely discussed how manipulating:
$$-dt^2 + [dx-v(t) f(r) \ dt]^2=0$$
leads to:
$$\frac{dx}{dt}=1+v(t)f(r)$$
and hence the claimed property of travel that appears superluminal to a remote observer (sitting away far enough to be in what is approximately Minkowski spacetime).
At first glance, this derivation seems to rely on the coordinates chosen to present the metric as in the above. Is this also the case in other coordinates? I am asking this because no matter what, the remote observer far outside the "bubble" sits in (approximately) Minkowski spacetime, meaning there are coordinate transformations that will not change this, such as going to synchronous coordinates. So it appears to me, that the remote observer, to a degree, does not care what coordinates we choose as it only changes the metric far away from it, while the observer remains in Minkowski spacetime.
Does this mean that the observation of superluminal travel is independent of the choice of coordinates for the Alcubierre metric, or more generally is the observed velocity independent of coordinate choice for asymptotically flat spacetimes, where the observer is in the approximately flat region?