N.H.M. Crighton
The neutral hydrogen cosmological mass density at z = 5
Crighton, N.H.M.; Murphy, M.T.; Prochaska, J.X.; Worseck, G.; Rafelski, M.; Becker, G.D.; Ellison, S.L.; Fumagalli, M.; Lopez, S.; Meiksin, A.; O'Meara, J.M.
Authors
M.T. Murphy
J.X. Prochaska
G. Worseck
M. Rafelski
G.D. Becker
S.L. Ellison
Professor Michele Fumagalli michele.fumagalli@durham.ac.uk
Academic Visitor
S. Lopez
A. Meiksin
J.M. O'Meara
Abstract
We present the largest homogeneous survey of z > 4.4 damped Lyα systems (DLAs) using the spectra of 163 QSOs that comprise the Giant Gemini GMOS (GGG) survey. With this survey we make the most precise high-redshift measurement of the cosmological mass density of neutral hydrogen, ΩHi. At such high redshift, important systematic uncertainties in the identification of DLAs are produced by strong intergalactic medium absorption and QSO continuum placement. These can cause spurious DLA detections, result in real DLAs being missed or bias the inferred DLA column density distribution. We correct for these effects using a combination of mock and higher resolution spectra, and show that for the GGG DLA sample the uncertainties introduced are smaller than the statistical errors on ΩHi. We find ΩHI=0.98+0.20−0.18×10−3 at 〈z〉 = 4.9, assuming a 20 per cent contribution from lower column density systems below the DLA threshold. By comparing to literature measurements at lower redshifts, we show that ΩHi can be described by the functional form ΩHI(z)∝(1+z)0.4. This gradual decrease from z = 5 to 0 is consistent with the bulk of H I gas being a transitory phase fuelling star formation, which is continually replenished by more highly ionized gas from the intergalactic medium and from recycled galactic winds.
Citation
Crighton, N., Murphy, M., Prochaska, J., Worseck, G., Rafelski, M., Becker, G., …O'Meara, J. (2015). The neutral hydrogen cosmological mass density at z = 5. Monthly Notices of the Royal Astronomical Society, 452(1), 217-234. https://doi.org/10.1093/mnras/stv1182
Journal Article Type | Article |
---|---|
Acceptance Date | May 21, 2015 |
Publication Date | Sep 1, 2015 |
Deposit Date | Aug 20, 2015 |
Publicly Available Date | Aug 20, 2015 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 452 |
Issue | 1 |
Pages | 217-234 |
DOI | https://doi.org/10.1093/mnras/stv1182 |
Keywords | Quasars: absorption lines, Cosmological parameters. |
Public URL | https://durham-repository.worktribe.com/output/1403808 |
Related Public URLs | http://adsabs.harvard.edu/abs/2015MNRAS.452..217C |
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Copyright Statement
This article has been accepted for publication in Monthly notices of the Royal Astronomical Society. ©: 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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