The luminosity function, halo masses and stellar masses of luminous Lyman-break galaxies at redshifts 5 6

R. J. McLure, M. Cirasuolo, J. S. Dunlop, S. Foucaud, O. Almaini

Research output: Contribution to journalArticlepeer-review

Abstract / Description of output

We present the results of a study of a large sample of luminous (z'(AB) < 26) Lyman-break galaxies (LBGs) in the redshift interval 4.7 < z < 6.3, selected from a contiguous 0.63 deg(2) area covered by the UKIRT Infrared Deep Sky Survey Ultra Deep Survey and the Subaru XMM-Newton Survey. Utilizing the large area coverage and the excellent available optical+near-infrared data, we use a photometric redshift analysis to derive a new, robust, measurement of the bright end (L >= L*) of the ultraviolet-selected luminosity function at high redshift. When combined with literature studies of the fainter LBG population, our new sample provides improved constraints on the luminosity function of redshift 5 < z < 6 LBGs over the luminosity range 0.1L* less than or similar to L less than or similar to 10L*. A maximum likelihood analysis returns best-fitting Schechter function parameters of M*(1500) = -20.73 +/- 0.11, phi* = 0.0009 +/- 0.0002 Mpc(-3) and alpha = -1.66 +/- 0.06 for the luminosity function at z = 5, and M*(1500) = -20.04 +/- 0.12, phi* = 0.0018 +/- 0.0005 Mpc(-3) and alpha = -1.71 +/- 0.11 at z = 6. In addition, an analysis of the angular clustering properties of our LBG sample demonstrates that luminous 5 < z < 6 LBGs are strongly clustered (r(0) = 8.1(-1.5)(+2.1)h(70)(-1) Mpc), and consistent with the occupation of dark matter haloes with masses of similar or equal to 10(11.5-12)M(circle dot). Moreover, by stacking the available multiwavelength imaging data for the high-redshift LBGs, it is possible to place useful constraints on their typical stellar mass. The results of this analysis suggest that luminous LBGs at 5 < z < 6 have an average stellar mass of log(10)( M/M-circle dot) = 10.0(-0.4)(+0.2), consistent with the results of the clustering analysis assuming plausible values for the ratio of stellar to dark matter. Finally, by combining our luminosity function results with those of the stacking analysis we derive estimates of similar or equal to 1 x 10(7) and similar or equal to 4 x 10(6)M(circle dot) Mpc(-3) for the stellar mass density at z similar or equal to 5 and 6, respectively.

Original languageEnglish
Pages (from-to)2196-2209
Number of pages14
JournalMonthly Notices of the Royal Astronomical Society
Issue number4
Publication statusPublished - 1 Jun 2009


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