G. Worseck
The Giant Gemini GMOS survey of zem > 4.4 quasars – I. Measuring the mean free path across cosmic time
Worseck, G.; Prochaska, J.X.; O'Meara, J.; Becker, G.; Ellison, S.; Lopez, S.; Meiksin, A.; Ménard, B.; Murphy, M.; Fumagalli, M.
Authors
J.X. Prochaska
J. O'Meara
G. Becker
S. Ellison
S. Lopez
A. Meiksin
B. Ménard
M. Murphy
Professor Michele Fumagalli michele.fumagalli@durham.ac.uk
Academic Visitor
Abstract
We have obtained spectra of 163 quasars at zem > 4.4 with the Gemini Multi Object Spectrometers, the largest publicly available sample of high-quality, low-resolution spectra at these redshifts. From this data set, we generated stacked quasar spectra in three redshift intervals at z ∼ 5 to model the average rest-frame Lyman continuum flux and to assess the mean free path λ912mfp of the intergalactic medium to H I-ionizing radiation. At mean redshifts zq = (4.56, 4.86, 5.16), we measure λ912mfp=(22.2±2.3,15.1±1.8,10.3±1.6)h−170 proper Mpc with uncertainties dominated by sample variance. Combining our results with measurements from lower redshifts, the data are well modelled by a power law λ912mfp=A[(1+z)/5]η with A=(37±2)h−170 Mpc and η = −5.4 ± 0.4 at 2.3 < z < 5.5. This rapid evolution requires a physical mechanism – beyond cosmological expansion – which reduces the effective Lyman limit opacity. We speculate that the majority of H I Lyman limit opacity manifests in gas outside galactic dark matter haloes, tracing large-scale structures (e.g. filaments) whose average density and neutral fraction decreases with cosmic time. Our measurements of the mean free path shortly after H I reionization serve as a valuable boundary condition for numerical models thereof. Our measured λ912mfp≈10 Mpc at z = 5.2 confirms that the intergalactic medium is highly ionized without evidence for a break that would indicate a recent end to H I reionization.
Citation
Worseck, G., Prochaska, J., O'Meara, J., Becker, G., Ellison, S., Lopez, S., …Fumagalli, M. (2014). The Giant Gemini GMOS survey of zem > 4.4 quasars – I. Measuring the mean free path across cosmic time. Monthly Notices of the Royal Astronomical Society, 445(2), 1745-1760. https://doi.org/10.1093/mnras/stu1827
Journal Article Type | Article |
---|---|
Publication Date | Dec 1, 2014 |
Deposit Date | Oct 17, 2014 |
Publicly Available Date | Oct 17, 2014 |
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 | 445 |
Issue | 2 |
Pages | 1745-1760 |
DOI | https://doi.org/10.1093/mnras/stu1827 |
Keywords | Galaxies: formation, Intergalactic medium, Quasars: absorption lines, Dark ages, Reionization, First stars, Diffuse radiation. |
Public URL | https://durham-repository.worktribe.com/output/1443629 |
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Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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