Outflow parameters derived from PVDs of disk-subtracted CO residuals at different vertical heights below and above the disk midplane: (a) X location r and FWHM width of the outflow cone walls. The errorbars denote the FWHM widths of the cone walls, not the uncertainty of the mean (which is smaller than the symbols). The light gray data points at z = ±40 au might be affected by imperfections in the disk model that was subtracted from the data. (b) Line-of-sight (LoS) velocity (relative to systemic velocity υ₀) and FWHM width of the outflow cone walls. Red squares show the center velocity between left and right outflow cone. (c) Radius R of the outflow cone, with uncertainties derived from the FWHM widths of the outflow cone walls. (d) Rotation velocity and 1σ uncertainty of the outflow cone walls. The red solid and dotted lines show the expected rotation velocity and uncertainty for angular momentum conservation of a wind that is launched from the disk at a single radius R_conn = 35 ± 10 au with a Keplerian rotation velocity of υ_K = 3.7 ± 0.3 km s⁻¹. (e) Specific angular momentum j and 1σ uncertainty. (f) Half-opening angle 9 and 1σ uncertainty.