A direct precision measurement of the intergalactic Lyman-α opacity at 2 ≤ z ≤ 4.2

C. A. Faucher-Giguère*, J. X. Prochaska, A. Lidz, L. Hernquist, M. Zaldarriaga

*Corresponding author for this work

Research output: Contribution to journalArticle

Abstract

We directly measure the evolution of the intergalactic Lyman-α effective optical depth, τeff, over the redshift range 2 ≤ z ≤ 4.2 from a sample of 86 high-resolution, high-signal-to-noise quasar spectra obtained with Keck/ESI, Keck/HIRES, and Magellan/MIKE. We find that our estimates of the quasar continuum levels in the Lya forest obtained by spline fitting are systematically biased low, but that this bias can be accounted for using mock spectra. The mean fractional error 〈ΔC/Ct rue〉 is < 1% at z = 2, 4% at z = 3, and 12% at z = 4. We provide estimates of the level of absorption arising from metals in the Lya forest based on both direct and statistical metal removal results in the literature, finding that this contribution is ≈ 6-9% at z = 3 and decreases monotonically with redshift. The high precision of our measurement indicates significant departures from the best-fit power law redshift evolution, particularly near z = 3.2.

Original languageEnglish (US)
Pages (from-to)1249-1252
Number of pages4
JournalNuovo Cimento della Societa Italiana di Fisica B
Volume122
Issue number9-11
DOIs
StatePublished - Sep 1 2007

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Fingerprint Dive into the research topics of 'A direct precision measurement of the intergalactic Lyman-α opacity at 2 ≤ z ≤ 4.2'. Together they form a unique fingerprint.

  • Cite this