  We present progress results of a new survey for bright QSOs (V<14.5, R<15.4,
B_J<15.2) covering the whole sky at high galactic latitudes, |b|>30. The
surface density of QSOs brighter than B_J=14.8 turns out to be 2.9 +- 0.8
10^{-3} deg^{-2}. The optical Luminosity Function at 0.04 < z < 0.3 shows
significant departures from the standard pure luminosity evolution, providing
new insights in the modelling of the QSO phenomenon.
