A Direct Precision Measurement of the Intergalactic Lyman-alpha Opacity at 2<z<4.2

Details A Direct Precision Measurement of the Intergalactic Lyman-alpha Opacity at 2<z<4.2 A Direct Precision Measurement of the Intergalactic Lyman-alpha Opacity at 2<z<4.2

2007-09-17

arxiv.org/abs/0709.2382v3

Astronomy and Astrophysics

Astrophysics

27 pages, including 18 figures, published in ApJ

Scientific paper

10.1086/588648

We directly measure the evolution of the intergalactic Lya effective optical depth, tau_eff, over the redshift range 2~3 based on directly fitting the quasar continua in the Lya forest, which have generally neglected this effect, are therefore likely biased low. 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, attaining 3% in redshift bins of width Delta z=0.2 around z=3, indicates significant departures from the best-fit power-law redshift evolution (tau_eff=0.0018(1+z)^3.92, when metals are left in), particularly near z=3.2. The observed downward departure is statistically consistent with a similar feature detected in a precision statistical measurement using Sloan Digital Sky Survey spectra by Bernardi and coworkers using an independent approach.

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