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Detecting Multiple DLAs per Spectrum in SDSS DR12 with Gaussian Processes

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arxiv 2003.11036 v2 pith:PQBRR3MS submitted 2020-03-24 astro-ph.CO astro-ph.GAphysics.data-an

classification astro-ph.COastro-ph.GAphysics.data-an
keywords dlasgaussianalphadensitylyman-absorbersalongdetect
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We present a revised version of our automated technique using Gaussian processes (GPs) to detect Damped Lyman-$\alpha$ absorbers (DLAs) along quasar (QSO) sightlines. The main improvement is to allow our Gaussian process pipeline to detect multiple DLAs along a single sightline. Our DLA detections are regularised by an improved model for the absorption from the Lyman-$\alpha$ forest which improves performance at high redshift. We also introduce a model for unresolved sub-DLAs which reduces mis-classifications of absorbers without detectable damping wings. We compare our results to those of two different large-scale DLA catalogues and provide a catalogue of the processed results of our Gaussian process pipeline using 158 825 Lyman-$\alpha$ spectra from SDSS data release 12. We present updated estimates for the statistical properties of DLAs, including the column density distribution function (CDDF), line density ($dN/dX$), and neutral hydrogen density ($\Omega_{\textrm{DLA}}$).

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