Simulated stellar halo in the presence of the LMC

<p>This file contains a simulated Milky Way stellar halo from Erkal et al. 2020 (<a href="https://ui.adsabs.harvard.edu/abs/2020arXiv200111030E/abstract">https://ui.adsabs.harvard.edu/abs/2020arXiv200111030E/abstract</a>)&nbsp;which has been evolved in the presence of a 1.5e11 Msun LMC. This stellar halo has a nearly constant anisotropy of 0.5. As described in the header, the first 6&nbsp;columns give the Galactocentric position and velocity of each particle in cartesian coordinates and the next 6 columns give the observables from the Sun&#39;s location (l,b,dist,mu_l*,mu_b,v_gsr). The Sun is taken to be at a distance of 8.122 kpc in the -x direction. Note that the proper motions are reflex corrected.</p> <p>Please cite&nbsp;<a href="https://ui.adsabs.harvard.edu/abs/2020arXiv200111030E/abstract">Erkal et al. 2020</a>&nbsp;if you make use of this simulation.</p>