We consider a moving refractive index perturbation in an optical medium as an optical analogue to waves under the influence of gravity. We start with the Lagrangian of the Hopfield model to describe the dielectric medium. Next, we apply field theory in curved spacetime to solve the scattering problem for all frequencies analytically. Because of dispersion, the kinematic configuration of the field modes may contain optical event horizons for some frequencies. We calculate the spectra of spontaneous emission in the frame co-moving with the perturbation and in the laboratory frame. We also calculate the spectrally-resolved photon number correlations in either frame. In [1] we found the spectral shape with paired modes and the multimode correlation structure to be characteristic of the horizon emission. Here, we find that these signatures are robust against changes in the system parameters and thus are genuine features of optical and non-optical analogues. These methods and findings pave the way to the observation of particles from the event horizon in dispersive systems.