Spectra of three peculiar Be-type stars from the VFTS, in which each spectrum has been smoothed and rebinned to R = 4000 for clarity. In addition to the Balmer lines, the emission lines identified in VFTS 1003 are [S II] λ4069; Fe II λλ4173, 4179, 4233, 4303, 4352, 4385, 4481, 4491, 4508, 4515, 4520-23, 4549, 4556; [Fe II] λλ4244, 4277, 4287, 4358-59, 4414-16. Emission lines identified in VFTS 822 are Fe II λλ4584, 4620.5, 4629. Absorption lines identified in VFTS 766 are He I λλ4009, 4026, 4121, 4144, 4388, 4471, 4713; Si II λλ4128-32; Mg II λ4481.