LDT/DeVeny optical spectrum of the host galaxy of FRB 20201124A at z = 0.0978 ± 0.0002. The spectrum (solid purple line) has been smoothed with a Gaussian kernel. Dashed black lines indicate the expected location of emission lines at this redshift; we do not observe oxygen lines or Hβ. The inset figure shows a zoomed-in view of the region of the detected emission lines between 7150 and 7450 Å. The spectrum is not corrected for Galactic extinction.