The THz spectral region includes a number of important transitions which allow us to trace the evolution of the interstellar medium. Because of theopacity of the atmosphere in this spectral range, the best sites forground-based THz observations are on the Antarctic Plateau; of these sites,Dome A is expected to be the best. THz survey science can be carried out with small telescopes, easing logistical constraints. By deploying a submillimetre-wave tipper/telescope to Dome A, we have trialled severaltechnologies for such an instrument, and we are able to test whether thesite quality is sufficient for THz surveys.