{ "id": "2011.12296", "version": "v1", "published": "2020-11-24T19:00:00.000Z", "updated": "2020-11-24T19:00:00.000Z", "title": "Modelling the Statistics of Cold Neutral Medium in Absorption-selected High-redshift Galaxies", "authors": [ "Jens-Kristian Krogager", "Pasquier Noterdaeme" ], "comment": "A&A Letter, Accepted for publication, 5 pages (incl. 2 page auxiliary data table)", "categories": [ "astro-ph.GA" ], "abstract": "We present a statistical model of the selection function of cold neutral gas in high-redshift (z~2.5) absorption systems. The model is based on the canonical two-phase model of the neutral gas in the interstellar medium and contains only one parameter for which we do not have direct observational priors: namely the central pressure (P*) of an L* halo at z=2.5. Using observations of the fraction of cold gas absorption in strong HI-selected absorbers, we are able to constrain P*. The model simultaneously reproduces the column density distributions of HI and H$_2$, and we derive an expected total incidence of cold gas at z~2.5 of $l_{CNM} = 12\\times 10^{-3}$. Compared to recent measurements of the incidence of CI-selected absorbers (EW$_{CI\\,1560}$ > 0.4 \\r{A}), the value of $l_{CNM}$ from our model indicates that only ~15% of the total cold gas would lead to strong CI absorption (EW > 0.4 \\r{A}). Nevertheless, CI lines are extremely useful probes of the cold gas as they are relatively easy to detect and provide direct constraints on the physical conditions. Lastly, our model self-consistently reproduces the fraction of cold gas absorbers as a function of N(HI).", "revisions": [ { "version": "v1", "updated": "2020-11-24T19:00:00.000Z" } ], "analyses": { "keywords": [ "cold neutral medium", "absorption-selected high-redshift galaxies", "statistics", "strong ci absorption", "direct observational priors" ], "note": { "typesetting": "TeX", "pages": 5, "language": "en", "license": "arXiv", "status": "editable" } } }