We present a further list of 274 bright QSOs, 106 (195) of which have B les
s than or similar to 17 (17.5), selected semiautomatically from objective p
rism plates taken with the Calar Alto 80 cm Schmidt telescope. All QSOs hav
e been confirmed by follow-up spectroscopy and we display their flux-calibr
ated spectra. We also discuss the completeness of our search technique and
demonstrate that for 0.1 less than or equal to z < 3.2 and B less than or e
qual to 17 we have been able to recover roughly 85% of known QSOs; 10% were
lost due to overlaps while 5% were lost during the selection process. In p
articular the bright z greater than or equal to 2 QSOs (17 with B less than
or similar to 17) are potential targets for follow-up spectroscopy both at
high-resolution from the ground and in the ultraviolet from space.