The shallow slope of the z~6 quasar luminosity function: limits from the lack of multiple image gravitational lenses

Abstract

We place a limit on the logarithmic slope of the luminous quasar luminosity function at z~6 of beta>-3.0 (90%) using gravitational lensing constraints to build on the limit of beta>-3.3 (90%) derived from an analysis of the luminosity distribution (Fan et al. 2003). This tight constraint is obtained by noting that of the two quasars which are lensed by foreground galaxies, neither are multiply imaged. These observations are surprising if the luminosity function is steep because magnification bias results in an overabundance of multiply imaged relative to singly imaged lensed quasars. Our Bayesian analysis uses the a-posteriori information regarding alignments with foreground galaxies of the two lensed quasars, and provides a constraint on beta that is nearly independent of the uncertain evolution in the lens population. The results suggest that the bright end of the quasar luminosity function continues to flatten out to z~6, as is observed between z~3 and z~5 (Fan et al. 2001). Provided that SDSS J1148-5251 at z=6.37 is magnified by an intervening lens galaxy at z~5 (White et al. 2003), we also show that the high lens redshift in this system implies a co-moving density of massive galaxies that is close to constant out to high redshift. This is in agreement with the lack of redshift evolution in the velocity function of dark-matter halos with velocity dispersions near 200 km/sec as predicted by the Press-Schechter formalism. The combination of constraints on the quasar luminosity function and lens galaxy evolution are used to compute an improved estimate for the z~6 multiple image lens fraction of ~1-3%.

11 pages, 6 figures, submitted to MNRAS

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Cited by in corpus (9)

• An Observational Determination of the Bolometric Quasar Luminosity Function
• The CFHTLS-Strong Lensing Legacy Survey (SL2S): Investigating the group-scale lenses with the SARCS sample
• The Discovery of a Gravitationally Lensed Quasar at z = 6.51
• The Formation of the First Massive Black Holes
• First results from the Canada-France High-z Quasar Survey: Constraints on the z=6 quasar luminosity function and the quasar contribution to reionization
• On the faint end of the high redshift AGN luminosity function
• High-resolution radio imaging of the most distant radio quasar SDSS J0836+0054
• On inferring extinction laws in z~6 quasars as signatures of supernova dust
• A Snapshot Survey for Gravitational Lenses Among z>=4.0 Quasars: II. Constraints on the 4.0<z<4.5 Quasar Population