I am following Peskin & Schroeder's QFT book. And on equation 2.51, we get an expression for the free Klein-Gordon propagator for timelike intervals $x^0-y^0=t$, $x-y=0$: $$D(x-y) \sim e^{-imt}\tag{2.51}$$ as $t$ goes to infinity. He then goes on to the spacelike case, where we get: $$D(x-y) \sim e^{-mr}\tag{2.52}$$ as $r$ goes to infinity. I understand how we got to those results, but not what he means by (p.28):
"Outside the light cone, the propagation amplitude is exponentially vanishing but nonzero".
Isn't this an issue? Don't we want this to be zero outside the light cone in order to preserve causality?
He then claims that what we really have to do is calculate $[\phi(x),\phi(y)]$. But then, what was the point of the previous calculation? What is my takeaway here? I am really confused about this.