VLT/X-shooter spectrum of the optical transient that followed GRB 120714B, taken at t_obs = 0.353 days after the burst. The binned original spectrum is shown in black, the host-galaxy SED template as obtained from the Le PHARE fit (Appendix A.3) in red. The green curve shows the smoothed host-galaxy template that was subtracted from the original spectrum. The host-subtracted SED is drawn in light gray. Flux densities refer to the observer frame. Telluric features are indicated.