The bright end of the QSO luminosity function

We have analysed the optical luminosity-redshift distribution properties of bright QSOs, using a new large sample from the Hamburg/ESO survey. The sam ple provides in sight into the hitherto poorly sampled bright tail of the l uminosity function, allowing to monitor its evolution with redshift up to z approximate to 3. The slope increases significantly towards higher z, inco nsistent with the predictions of pure luminosity evolution, but also with o ther recently proposed parameterisations. This phenomenon is opposite to wh at would be expected from gravitational lensing, showing that magnification bias does not significantly distort the QSO luminosity function within the redshift range covered. The space density of high-luminosity QSOs continue s to increase up to the high-redshift limit of the survey, without indicati on of reduced evolution above z approximate to 2. The sam pie also permits an improved estimate of the local (z approximate to 0) luminosity function of QSOs and bright Seyfert 1 nuclei, over the luminosity range -27 less tha n or similar to M-BJ, less than or similar to -20. No evidence for a break or change of slope is found down to absolute magnitudes M-B, - -20.