  We provide an exhaustive numerical exploration of the predictions of loop
quantum cosmology (LQC) with a post-bounce phase of inflation for the
primordial power spectrum of scalar and tensor perturbations. We extend
previous analysis by characterizing the phenomenologically relevant parameter
space and by constraining it using observations. Furthermore, we characterize
the shape of LQC-corrections to observable quantities across this parameter
space. Our analysis provides a framework to contrast more accurately the theory
with forthcoming polarization data, and it also paves the road for the
computation of other observables beyond the power spectra, such as
non-Gaussianity.
