Comparison of T_e[N II] measurements used in this work (Brazzini et al. 2024) with three different sets of measurements from the literature. While the auroral line fits in Kreckel et al. (2022) (left) and Rickards Vaught et al. (2024) (center) are both based on the same underlying MUSE data set, different assumptions have been made in the SSP fitting and region boundaries. The Berg et al. (2015) measurements (right) are based on independent long-slit spectroscopy. As there are only five regions in common with Berg et al. (2015), no offset or scatter is calculated in comparison with this sample.