Asteroseismic detection of latitudinal differential rotation in 13 Sun-like stars

Power spectrum used for the Asteroseismic inference of the latitudinal differential rotation. Each .data files contain two columns. The first column is the frequency (in microHz) and the second column is the power (in ppm^2/microHz). The data are limited to the range in which the MCMC fit was performed using the code available at https://github.com/OthmanB/TAMCMC-C. The data can be downloaded in their entirety (lightcurve, full power spectrum) in the KASOC website (kasoc.phys.au.dk, requires to create an account).