Best fit model of the Radcliffe Wave

Tab-separated ASCII machine readable table of the best fit model in Konietzka et al. 2024. <br> The best fit model was derived by applying the model described in Konietzka et al. 2024 to the spatial and kinematic molecular cloud and stellar cluster observations.<br> <br> Data columns are as follows:<br> <br> (1) x: Heliocentric Galactic Cartesian x position (pc)<br> (2) y: Heliocentric Galactic Cartesian y position (pc)<br> (3) z: Heliocentric Galactic Cartesian z position (pc)<br> (4) vz: motion along the Heliocentric Galactic Cartesian z direction (km/s)<br>