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

<p>** these files are downloaded automatically by Phantom when running the code **</p> <p>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 (<a href="http://adsabs.harvard.edu/abs/2018PASA...35...31P">Price et al. 2018</a>). They were created by James Wurster as part of a code comparison with the Hydra code described in section 6.4 of the paper.</p> <p>The files were originally created for use in <a href="http://adsabs.harvard.edu/abs/2013MNRAS.431..539W">Wurster &amp; Thacker (2013)</a></p> <p>For details of how to read these files, see the Phantom source code (<a href="https://github.com/danieljprice/phantom/blob/master/src/setup/setup_galaxies.f90">setup_galaxies.f90</a>)</p>