Stellar Stream Models in the presence of the Milky Way and LMC

<p>These&nbsp;files include simulated stream models from Shipp et al. 2021 (https://ui.adsabs.harvard.edu/abs/2021arXiv210713004S/abstract).</p> <p>These streams are simulated using a modified Lagrange Cloud Stripping technique developed in Gibbons 2014, in a McMillan 2017 Milky Way potential, and with an LMC modeled as a Hernquist profile, with details described in Shipp et al. 2021. These are best-fit models resulting from fits to data from the Southern Stellar Stream Spectroscopic Survey (S5), Gaia, and the Dark Energy Survey (DES).</p> <p>The columns, as listed in the file headers, are ra and dec (deg), stream coordinates phi1 and phi2 (deg), proper motion in ra and dec&nbsp;(mas/yr, without reflex correction), radial velocity (km/s), Heliocentric distance (kpc), and stream positions and velocities&nbsp;in standard Galactocentric cartesian coordinates,&nbsp;x, y, z (kpc), vx, vy, vz (km/s).</p> <p>Please cite <a href="https://ui.adsabs.harvard.edu/abs/2021arXiv210713004S/abstract">Shipp et al. 2021</a> if you make use of this data.</p>