Examples of the extinction-corrected, continuum- and iron-subtracted over-flare-2 spectra fit using PYQSOFIT. The higher-resolution DBSP spectra were convolved to match with LRIS to allow comparison. The emission lines of interest were modeled with a set of broad and/or narrow Gaussian line components. Left: The LRIS spectrum taken on 2023-06-15, zooming into the Hβ and Hα regions. Right: The DBSP spectrum taken on 2024-05-21, where we also fit the [Fe X] λ6375 high-ionization coronal line as a separate component.