English

Detecting Multiple DLAs per Spectrum in SDSS DR12 with Gaussian Processes

Cosmology and Nongalactic Astrophysics 2020-07-01 v2 Astrophysics of Galaxies Data Analysis, Statistics and Probability

Abstract

We present a revised version of our automated technique using Gaussian processes (GPs) to detect Damped Lyman-α\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-α\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-α\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/dXdN/dX), and neutral hydrogen density (ΩDLA\Omega_{\textrm{DLA}}).

Keywords

Cite

@article{arxiv.2003.11036,
  title  = {Detecting Multiple DLAs per Spectrum in SDSS DR12 with Gaussian Processes},
  author = {Ming-Feng Ho and Simeon Bird and Roman Garnett},
  journal= {arXiv preprint arXiv:2003.11036},
  year   = {2020}
}

Comments

24 pages, 20 figures, plus 3 tables of figure values. Minor changes to match version published in MNRAS. Code available in https://github.com/rmgarnett/gp_dla_detection/tree/master/multi_dlas

R2 v1 2026-06-23T14:25:55.038Z