Statistical properties of damped Lyman-alpha systems from Sloan Digital Sky Survey DR12

TL;DR

This paper analyzes the statistical properties of damped Lyman-alpha systems using SDSS DR12 data, providing new measurements of their distribution and density at high redshifts, and demonstrating the robustness of results against data noise.

Contribution

It introduces a method to estimate DLA properties from SDSS DR12 data that accounts for uncertainties and extends measurements to redshifts above 4.

Findings

Non-zero column density distribution at all tested values

First SDSS measurements of line density and neutral hydrogen density at z>4

Results are robust against spectral noise but show residual redshift dependence below z=2.5

Abstract

We present new estimates for the statistical properties of damped Lyman-$\alpha$ absorbers (DLAs). We compute the column density distribution function at $z>2$, the line density, $\mathrm{d}N/\mathrm{d}X$, and the neutral hydrogen density, $\Omega_\mathrm{DLA}$. Our estimates are derived from the DLA catalogue of Garnett 2016, which uses the SDSS-III DR12 quasar spectroscopic survey. This catalogue provides a probability that a given spectrum contains a DLA, allowing us to use even the noisiest data without biasing our results and thus substantially increase our sample size. We measure a non-zero column density distribution function at $95\%$ confidence for all column densities $N_\mathrm{HI} < 5\times 10^{22}$ cm$^{-2}$. We make the first measurements from SDSS of $\mathrm{d}N/\mathrm{d}X$ and $\Omega_\mathrm{DLA}$ at $z>4$. We show that our results are insensitive to the signal-to-noise ratio of the spectra, but that there is a residual dependence on quasar redshift for $z<2.5$, which may be due to remaining systematics in our analysis.