Multi-wavelength observations of very high energy sources can place better constraints on the emission processes at work in these systems as well as the location of this emission. For example, the spectral energy distributions of Active Galactic Nuclei (AGN) display two distinct components that radiate at lower (radio to UV/X-ray) and higher (X-ray to gamma-ray) energies. If the emission is the result of a simple one zone model, correlations should be observable between these different components. Such correlations are, however, more complicated than a simple linear relation, but show variations based on colour and spectral distribution. It is therefore important to undertake multi-wavelength observations of known TeV gamma-ray sources to establish multiwavelength correlations. We are beginning a long term optical monitoring campaign of known TeV AGN/Blazars, from the Boyden Observatory, using, in particular, the Watcher Robotic Telescopes. Additional observations are capable with the Boyden 1.5-m telescope as well as with the 20-inch telescope recently obtained from the South African Astronomical Observatory. We present an overview of the new monitoring campaign which is being undertaken as well as a brief overview of the Boyden Observatory, and the status of the available telescopes.