Same as Fig. 9, but for the spectroscopic dataset based on He I lines. Top: SED dataset for He I lines exhibits results very similar to spectroscopy based on Balmer lines. The higher P_rot and i values are excluded because of other datasets. Bottom: SED dataset for He I lines, indicating two possible solutions at T = 25 000 K or 27 500 K, due to systematic offsets in some lines. The model with T = 25 000 K fits the depths of He I lines better. The map also shows no preference for mass.