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 \pm 0.8 \cdot 10 ^ { -3 } deg ^ { -2 } .
The optical Luminosity Function at 0.04 < z \leq 0.3 shows significant departures from the standard pure luminosity evolution , providing new insights in the modelling of the QSO phenomenon .