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Improved measurements of the intergalactic medium temperature around quasars: possible evidence for the initial stages of He-II reionisation at z~6

S. Bolton, James; D. Becker, George; Raskutti, Sudhir; Stuart B. Wyithe, J.; G. Haehnelt, Martin; L. W. Sargent, Wallace

Authors

George D. Becker

Sudhir Raskutti

J. Stuart B. Wyithe

Martin G. Haehnelt

Wallace L. W. Sargent



Abstract

We present measurements of the intergalactic medium (IGM) temperature within ~5 proper Mpc of seven luminous quasars at z~6. The constraints are obtained from the Doppler widths of Lyman-alpha absorption lines in the quasar near-zones and build upon our previous measurement for the z=6.02 quasar SDSS J0818+1722. The expanded data set, combined with an improved treatment of systematic uncertainties, yields an average temperature at the mean density of log (T_0/K) = 4.21 \pm 0.03 (\pm^0.06_0.07) at 68 (95) per cent confidence for a flat prior distribution over 3.2 < log (T_0/K) < 4.8. In comparison, temperatures measured from the general IGM at z~5 are ~0.3 dex cooler, implying an additional source of heating around these quasars which is not yet present in the general IGM at slightly lower redshift. This heating is most likely due to the recent reionisation of He-II in vicinity of these quasars, which have hard, non-thermal ionising spectra. The elevated temperatures may therefore represent evidence for the earliest stages of He-II reionisation in the most biased regions of the high-redshift Universe. The temperature as a function of distance from the quasars is consistent with being constant, log(T_0/K)~4.2, with no evidence for a line-of-sight thermal proximity effect. However, the limited extent of the quasar near-zones prevents the detection of He-III regions larger than ~5 proper Mpc. Under the assumption the quasars have reionised the He-II in their vicinity, we infer the data are consistent with an average optically bright phase of duration in excess of 10^6.5 yr. These measurements represent the highest-redshift IGM temperature constraints to date, and thus provide a valuable data set for confronting models of H-I reionisation.

Journal Article Type Article
Acceptance Date Sep 20, 2011
Online Publication Date Jan 9, 2012
Publication Date 2012-02
Deposit Date Sep 16, 2019
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 419
Issue 4
Pages 2880–2892
DOI https://doi.org/10.1111/j.1365-2966.2011.19929.x
Keywords Cosmology and Nongalactic Astrophysics
Public URL https://nottingham-repository.worktribe.com/output/2462266
Publisher URL https://academic.oup.com/mnras/article/419/4/2880/2908033