Each *.dat dataset contains the 1D distribution of quantities through a cosmological simulation, from z=0 to z=2, through a random line of sight. The additional .eps files show the trend of data in density, temperature and magnetic field. The files with "cR" in the name are for a model only with cooling and an initial magnetic field of B=10^-11 G at z=30. The files with "cqhR" are a resimulation of the same volume, including also the magnetic/thermal output from active galactic nuclei. The fixed comoving resolution of the simulation is 166.6 kpc per cell. Each dataset is written as follows: "z","gas dens","DM dens","temp","Bx","By","Bz","Btot" with comoving units "# ", "[g/cm^3]","[g/cm^3]","[K]","[G/4pi]","[G/4pi_greek]","[G/4pi_greek]","[G/4pi_greek]" The parent simulations have been run on CSCS-ETHZ (Lugano) using the ENZO code, see Vazza et al. 2014 (http://adsabs.harvard.edu/abs/2014MNRAS.445.3706V) for details.