Tar archive of simulations of circumbinary planets orbiting a range of host binary stars. Each file in the archive has the assumed mass ratio, mu, and binary eccentricity, e_bin, in the file name as a tuple (mu,e_bin). Tools in python to manipulate and plot the data are provided through a GitHub repository, https://github.com/saturnaxis/CBP_stability. Inside each file contains a comma delimited text file, where the columns are the initial semimajor axis ratio, the initial phase of the planet, the maximum planetary eccentricity attained over 10^5 yr, the minimum planetary eccentricity attained over 10^5 yr, and the collision/escape time. Collisions are defined as crossing the binary orbit, where the escape is when the radial distance of the planet exceeds 10 AU.