Example of the full spectral modeling using PyParadise for one binned spectrum of HE 0433−1028. The input spectrum and error spectrum are shown in the top panels as a black and green line, respectively. Emission-line contaminated regions and prominent sky or telluric absorption features are indicated by the gray and red shaded areas. The corresponding best-fit continuum model is shown as the red line. The residual spectrum is highlighted in the lower panel with best-fit single Gaussian emission-line models represented by the blue lines. The wavelength range modeled for the emission-line detection are represented by the blue shaded areas. All fitted emission lines are annotated for reference and identification.