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

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.

7 pages, 6 figures, plus 6 tables of figure values. Accepted by MNRAS with minor changes

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