2002/02/07 by Antoinette Songaila, Lennox L. Cowie · 6 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Extrapolation #Flux (metallurgy) #Galaxies: Formation, Evolution, Phenomena #Lambda #Lyman limit #Lyman-alpha forest #Metallicity #Quasar #Redshift #Scientific Research and Discoveries #Spectral line #astro-ph
paper · pdf · doi:10.1086/340079
published as Astron.J. 123 (2002) 2183 · 17 pages, including 13 figures. Accepted for publication in Astronomical Journal (May 2002)
arxiv created 2002/02/07 · openalex publication_date 2002/05/01 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We analyze the Lyα forest properties of a sample of 15 high-redshift quasars lying between z = 4.42 and z = 5.75, using high signal-to-noise spectra obtained with the Echellette Spectrograph and Imager on the Keck II 10 m telescope. The distribution of transmissions in the Lyα region in this redshift range is shown to be consistent with that found in lambda cold dark matter simulations with a smoothly evolving ionization rate as a function of redshift. The extrapolation of the ionizing flux to z = 6.05 lies a factor of 2 higher than a 2 σ upper limit placed by Cen & McDonald at this redshift, based on the Becker et al. spectra of the z = 6.28 quasar SDSS 1030+0524. However, the data are also consistent with models in which there is substantial variation of the ionization parameter about the mean value, and in this case, dark gaps such as those seen by Becker et al. become much more likely. We conclude that further data are needed before we can be sure that we have seen the epoch of reionization. We also summarize the damped Lyα systems (DLAs) seen in these quasar lines of sight and measure their metallicities and kinematic properties. We argue that the mean DLA metallicity has dropped substantially by z = 5, compared with its value at z < 4.