One-dimensional spectrum covering the Lyα line for ID 62-85 in the new faint quasar sample. The ID of each quasar is shown in the top left corner of each panel. Each panel shows the spectrum integrated from the MUSE data cube inside a 1.5″ radius aperture centered at the quasar location (black line) and the integrated spectrum of each detected nebula integrated from the PSF- and continuum-subtracted data cubes within the 2σ isophotes from Figure 5 (red line), respectively. The wavelength of the peak of the Lyα emission of each quasar is indicated with a blue vertical line. The gray lines are the spectra integrated within a 1.5″ radius aperture from subtracted data cubes where we found no extended Lyα emission. We mask the 1″ × 1″ PSF normalization region when extracting a spectrum using the PSF- and continuum-subtracted data cubes. All the spectra are shown with the same y-axis scale and we indicate with a label in the top right corner of the panel if the quasar spectra has been rescaled by 0.6× or 0.3× for visualization. The reminder of the spectra (IDs 86 to 120) are shown in Figures A.1 and A.2.