Height (left panel) and z/r (right panel) profiles for the available CO isotopologs and CN transitions in Elias 2-27. The CN emission is separated by a hyperfine group. Solid lines show the best-fit exponentially tapered vertical profile and the shadowed regions show the uncertainty on the best-fit model, derived from the spread of the posteriors in each tracer. Due to the absorption and asymmetries that affect Elias 2-27, the data corresponds to measurements only from the west side of the disk (for all tracers).