2009AJ....138..305J

We present the discovery of six new quasars at z ∼ 6 selected from the Sloan Digital Sky Survey (SDSS) southern survey, a deep imaging survey obtained by repeatedly scanning a stripe along the celestial equator. The six quasars are about 2 mag fainter than the luminous z ∼ 6 quasars found in the SDSS main survey and 1 mag fainter than the quasars reported in Paper I. Four of them comprise a complete flux-limited sample at 21 < z_AB< 21.8 over an effective area of 195 deg². The other two quasars are fainter than z _AB= 22 and are not part of the complete sample. The quasar luminosity function at z ∼ 6 is well described as a single power law Φ(L₁₄₅₀) ∝ L ^β₁₄₅₀ over the luminosity range -28 < M₁₄₅₀< -25. The best-fitting slope β varies from -2.6 to -3.1, depending on the quasar samples used, with a statistical error of 0.3-0.4. About 40% of the quasars discovered in the SDSS southern survey have very narrow Lyα emission lines, which may indicate small black hole masses and high Eddington luminosity ratios, and therefore short black hole growth timescales for these faint quasars at early epochs.