Aperture-corrected nuclear spectrum of NGC 4395, extracted from the central region, spans the rest-frame wavelength range 1.66–28.6 μm, combining observations from JWST/NIRSpec and MIRI Channels 1–4. Some of the prominent emission lines are indicated along the spectrum. Molecular features, including PAH and H₂ lines, together with HI recombination lines, are shown by solid lines, while ionized gas lines are denoted by dashed lines. Low-ionization species (e.g., [Fe II], [Ne II], [S III], [O IV]) are marked in purple, whereas high-ionization lines are indicated in dark green.

(The data used to create this figure are available in the online article.)

(The data used to create this figure are available.)