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

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

2003-08-18

arxiv.org/abs/astro-ph/0308290v1

Mon.Not.Roy.Astron.Soc.351:1266,2004

Astronomy and Astrophysics

Astrophysics

11 pages, 6 figures, submitted to MNRAS

Scientific paper

10.1111/j.1365-2966.2004.07866.x

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%.

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