Kepler EB + Pulsator analysis

A survey of the background objects in the original Kepler field reveals a number of interesting objects. This project deals with the analysis of a number of eclipsing binary stars that have a pulsating component, either Gamma Doradus or Delta Scuti types. The analysis of these is important for asteroseismology modelling. It requires that the EB and pulsator signals be separated in an accurate manner, by the use of pre-whitening and EB modelling procedures.