Results from Classification Observations and a Multi‐site Campaign on γ Doradus and SPB Type Stars

As part of a observational project aiming to investigate the effects of rotation on main‐sequence g‐mode non‐radial pulsation we have obtained at least one (generally more) high‐resolution spectroscopic observation of more than 50 confirmed or candidate γ Doradus and slowly pulsating B stars and have completed a spectroscopic multi‐site campaign. The campaign was one of those outlined in De Cat et al. (these proceedings) and included five observatories and focused on the γ Doradus, and now planet hosting star HD 218396 (HR 8799) and the SPB stars HD 21071 and HD 25558.