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A new measurement of the intergalactic temperature at z∼2.55 − 2.95

Rorai, Alberto; Carswell, R.F.; Haehnelt, Martin G.; Becker, George D.; Bolton, James S.; Murphy, Michael T.

A new measurement of the intergalactic temperature at z∼2.55 − 2.95 Thumbnail


Authors

Alberto Rorai

R.F. Carswell

Martin G. Haehnelt

George D. Becker

Michael T. Murphy



Abstract

We present two measurements of the temperature-density relationship (TDR) of the intergalactic medium (IGM) in the redshift range 2.55 < z < 2.95 using a sample of 13 high-quality quasar spectra and high resolution numerical simulations of the IGM. Our approach is based on fitting the neutral hydrogen column density NHI and the Doppler parameter b of the absorption lines in the Lyα forest. The first measurement is obtained using a novel Bayesian scheme which takes into account the statistical correlations between the parameters characterising the lower cut-off of the b − NHI distribution and the power-law parameters T0 and γ describing the TDR. This approach yields T0/103 K = 15.6 ± 4.4 and γ = 1.45 ± 0.17 independent of the assumed pressure smoothing of the small scale density field. In order to explore the information contained in the overall b − NHI distribution rather than only the lower cut-off, we obtain a second measurement based on a similar Bayesian analysis of the median Doppler parameter for separate column-density ranges of the absorbers. In this case we obtain T0/103 K = 14.6 ± 3.7 and γ = 1.37 ± 0.17 in good agreement with the first measurement. Our Bayesian analysis reveals strong anti-correlations between the inferred T0 and γ for both methods as well as an anti-correlation of the inferred T0 and the pressure smoothing length for the second method, suggesting that the measurement accuracy can in the latter case be substantially increased if independent constraints on the smoothing are obtained. Our results are in good agreement with other recent measurements of the thermal state of the IGM probing similar (over-)density ranges.

Citation

Rorai, A., Carswell, R., Haehnelt, M. G., Becker, G. D., Bolton, J. S., & Murphy, M. T. (2017). A new measurement of the intergalactic temperature at z∼2.55 − 2.95. Monthly Notices of the Royal Astronomical Society, 474(3), 2871-2883. https://doi.org/10.1093/mnras/stx2862

Journal Article Type Article
Acceptance Date Nov 1, 2017
Publication Date Nov 7, 2017
Deposit Date Nov 30, 2017
Publicly Available Date Nov 30, 2017
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 474
Issue 3
Pages 2871-2883
DOI https://doi.org/10.1093/mnras/stx2862
Keywords intergalactic medium; quasar:absorption lines
Public URL https://nottingham-repository.worktribe.com/output/893500
Publisher URL https://academic.oup.com/mnras/article/474/3/2871/4600557
Additional Information This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

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