Fragments of smoothed spectra in the LyC region for 11 galaxies at z ∼ 0.6–1.0 (a) – (k) (this paper), and for J1243+4646 (l) from Izotov et al. (2018b). Modelled intrinsic SEDs, attenuated by Milky Way extinction with R(V)_MW = 3.1 and internal extinction with R(V)_int = 2.7, assuming the Cardelli et al. (1989) reddening law, and the unreddened SEDs are shown by solid red and dash-dotted blue lines, respectively. Emission features at the observed wavelengths λ1216Å and λ1301Å are geocoronal Lyα and O I emission lines, respectively. The parts of the observed spectra containing the LyC bumps for a) J0232+0025, h) J1021+0436, and l) J1243+4646 are highlighted by magenta lines. Dotted black lines in all panels indicate the GALEX FUV response curve reduced to the galaxy rest-frame. The vertical dotted line in all panels indicates the location of the LyC limit at 912 Å. Fluxes are in 10⁻¹⁶ erg s⁻¹ cm⁻² Å⁻¹, and wavelengths are in angstrom.