We propose a class of scalar models that, once coupled to gravity, lead tocosmologies that smoothly and stably connect an inflationary quasi-de Sitteruniverse to a low, or even zero-curvature, maximally symmetric spacetime in theasymptotic past, strongly violating the null energy condition ($\dot H\gg H^2$)at intermediate times. The models are deformations of the conformal galileonlagrangian and are therefore based on symmetries, both exact and approximate,that ensure the quantum robustness of the whole picture. The resultingcosmological backgrounds can be viewed as regularized extensions of thegalilean genesis scenario, or, equivalently, as `early-time-complete'realizations of inflation. The late-time inflationary dynamics possessesphenomenologically interesting properties: it can produce a largetensor-to-scalar ratio within the regime of validity of the effective fieldtheory and can lead to sizeable equilateral nongaussianities.