Visual (top) and NIR (bottom) spectral line identifications for SN 2013L. It is important to note that the spectra in the top panel were smoothed (dark lines) for presentation purposes. In the optical, we plotted the expected positions for the Fe II lines (red) for a model with Fe II Lyα and Lyβ pumping, from Sigut & Pradhan (2003). These lines can explain the blue excess in the spectrum at late epochs.