Magnetic and temperature spots on the surface of the Sun can be easily observed and studied. Other stars are too far away and can only be partially resolved even with the most powerful telescopes. However, high-resolution stellar spectra contain sufficient information to detect and map stellar surface inhomogeneities using Doppler imaging, a well-established method for probing the stellar magnetic dynamos responsible for the generation of magnetic fields and activity cycles. Dark surface spot features on rapidly rotating stars cause "bumps" in their spectral line profiles. Doppler Imaging inverts a time series of these "bumps" to produce a map of the surface spot features on a star. Photometry plays an important role in obtaining important information about these stars and there is the opportunity for a pro-am collaboration to assist in building the database of new southern targets.