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The 2dF-SDSS LRG and QSO Survey: The z<2.1 Quasar Luminosity Function from 5645 Quasars to g=21.85

G. T. Richards·S. M. Croom·S. F. Anderson·J. Bland-Hawthorn·B. J. Boyle·R. De Propris·M. J. Drinkwater·X. Fan·J. E. Gunn·Z. Ivezic·S. Jester·J. Loveday·A. Meiksin·L. Miller·A. Myers·R. C. Nichol·P. J. Outram·K. A. Pimbblet·I. G. Roseboom·N. Ross·D. P. Schneider·T. Shanks·R. G. Sharp·C. Stoughton·M. A. Strauss·A. S. Szalay·D. E. Vanden Berk·D. G. York
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Abstract

We have used the 2dF instrument on the AAT to obtain redshifts of a sample of z<3, 18.0 21 deep surveys. The 2SLAQ data exhibit no well defined ``break'' but do clearly flatten with increasing magnitude. The shape of the quasar luminosity function derived from 2SLAQ is in good agreement with that derived from type I quasars found in hard X-ray surveys. [Abridged]

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G. T. Richards, S. M. Croom, S. F. Anderson, J. Bland-Hawthorn, B. J. Boyle, R. De Propris, M. J. Drinkwater, X. Fan, J. E. Gunn, Z. Ivezic, S. Jester, J. Loveday, A. Meiksin, L. Miller, A. Myers, R. C. Nichol, P. J. Outram, K. A. Pimbblet, I. G. Roseboom, N. Ross, D. P. Schneider, T. Shanks, R. G. Sharp, C. Stoughton, M. A. Strauss, A. S. Szalay, D. E. Vanden Berk, D. G. York. 2005-04-13. The 2dF-SDSS LRG and QSO Survey: The z<2.1 Quasar Luminosity Function from 5645 Quasars to g=21.85. https://doi.org/10.1111/j.1365-2966.2005.09096.x

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