Integrated spectra of NGC 1365 from MUSE data. The blue and green curves represent the integrated spectra extracted with a 0.7″radius aperture from regions dominated by the stellar disk and outflow emission, respectively (see Fig. 1, lower right panel). Detected emission lines are marked with vertical lines: ionized gas emission lines in yellow, atomic lines in violet, and H I recombination lines in green. An asterisk indicates species corresponding to blends of two or three emission lines.