Instability strip grid for SPB stars including the effect of the rotation and metallicity

This dataset contains the results of a grid of stellar evolutionary models computed using the CLES code, along with the corresponding non-adiabatic oscillation computations performed with the MAD non-adiabatic oscillation code. The grid includes the global stellar properties of models with masses ranging from 2.5 to 8.0 solar mass and initial metal mass fractions Z between 0.0125 and 0.025. For each stellar model in the grid, the associated non-adiabatic oscillations have been computed. The dataset provides, for each case, the individual mode frequencies and their corresponding damping or growth rates for example.