The energy of 13.6 eV corresponds to the ionization energy of hydrogen, meaning the electron is excited to the highest possible energy level and then de-excites.
The emitted spectral lines belong to the Lyman series when an electron transitions to the
n=1 energy level:
ΔE=hν=13.6(1−n21)eV
Since all transitions end at
n=1, the emitted radiation falls in the ultraviolet region, characteristic of the Lyman series.