Spectral evolution of SN 2022qml as shown through the most significant spectra. Numbers close to the spectra indicate the phase from explosion corrected for time dilation. All spectra are scaled with respect to the Hα and arbitrarily shifted for better visualisation. The spectra have not been corrected for extinction. We also plot the narrow Hα in velocity space to show the P Cygni profile due to the wind that formed the CSM.