Spectroscopic analysis of stars and other targets is often a complex and challenging task. New software pipelines have been utilised to streamline this process while still retaining the validity and precision of results. This has been done with iSpec, a software package that bundles a variety of models within a user-friendly interface. Applying these methods to data collected from the Mount John Observatory in New Zealand, allows the chemical abundances, atmospheric characteristics and other parameters of the targets to be determined. The study focuses on the relatively recent stellar classification of Gamma Doradus variables in the hope of shedding further light on the nature of these stars and allowing them to be more readily distinguished from other categories of variable.