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

TL;DR

This study provides a highly precise measurement of the intergalactic Lyman-alpha opacity evolution between redshifts 2 and 4.2, revealing deviations from simple models and highlighting the importance of accounting for systematic biases and metal absorption.

Contribution

It offers the largest high-resolution dataset for this redshift range, improves error estimation, and identifies biases in previous continuum fitting methods, advancing understanding of intergalactic medium evolution.

Findings

Measured tau_eff with 3% precision at z=3

Detected significant deviations from power-law evolution near z=3.2

Quantified metal absorption contribution as 6-9% at z=3

Abstract

We directly measure the evolution of the intergalactic Lya effective optical depth, tau_eff, over the redshift range 2<z<4.2 from a sample of 86 high-resolution, high-signal-to-noise quasar spectra obtained with the ESI and HIRES spectrographs on Keck, and with the MIKE spectrograph on Magellan. This represents an improvement over previous analyses of the Lya forest from high-resolution spectra in this redshift interval of a factor of two in the size of the data set alone. We pay particular attention to robust error estimation and extensively test for systematic effects. We find that our estimates of the quasar continuum levels in the Lya forest obtained by spline fitting are systematically biased low, with the magnitude of the bias increasing with redshift, but that this bias can be accounted for using mock spectra. The mean fractional error is <1% at z=2, 4% at z=3, and 12% at z=4. Previous measurements of tau_eff at z>~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.