Initial conditions for galaxy merger setup in the Phantom smoothed particle hydrodynamics and magnetohydrodynamics code

** these files are downloaded automatically by Phantom when running the code ** The two files here contain initial conditions (particle positions, velocities etc) for the sample galaxy merger simulation shown in Figure 55 of the Phantom code paper (Price et al. 2018). They were created by James Wurster as part of a code comparison with the Hydra code described in section 6.4 of the paper. The files were originally created for use in Wurster & Thacker (2013) For details of how to read these files, see the Phantom source code (setup_galaxies.f90)