These simulations also include MHD+, magnetohydrodynamics as well as fully-anisotropic Spitzer-Braginskii conduction and viscosity.

We ran these simulations after we fixed the cosmic-ray heating bug in Gizmo (after 2018-4-26). That bug erroneously applied a heating term from cosmic rays to all gas in the simulation at z >~ 8, which prevented gas cooling and star formation at those early times, and which affects other FIRE-2 simulations.

Most of these MHD+ and Cosmic Ray simulations have a subset of 61 out of 601 snapshots available, specifically, every tenth snapshot. However, we have more snapshots available for m12i (127), m12f (253), and m12m (309), and for them we also provide halo/galaxy catalogs, merger trees, and particle tracking. In addition, the following simulations are missing some snapshots (see their notes.txt):
m10q, m11c, m11q

For m12f, m12i, and m12m, within track/ we provide pointers between particles, as well as host galaxy coordinates, but only for the available snapshots. We also provide star formation coordinates (specifically, the coordinates of a star particle at the first snapshots after it formed). Because we did not have all 601 snapshots when we ran particle tracking for these simulations, these 'formation' coordinates could be up to ~250 Myr after a star particle formed, so use caution in interpreting them.