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The Fraction of Ionizing Photons Escaping from High-Redshift Galaxies

Published online by Cambridge University Press:  02 January 2013

Jhan A. Srbinovsky  and
J. Stuart B. Wyithe
Jhan A. Srbinovsky
Affiliation:
School of Physics, University of Melbourne, Parkville, Victoria, Australia
J. Stuart B. Wyithe*
Affiliation:
School of Physics, University of Melbourne, Parkville, Victoria, Australia
*
BCorresponding author. Email: swyithe@unimelb.edu.au
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Abstract

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The fraction (fesc) of ionizing photons that escape their host galaxy and so are able to ionize hydrogen in the intergalactic medium is a critical parameter in studies of the reionization era. In this paper we constrain fesc at high redshift by modelling the observed Lyα transmission. Using an N-body simulation of the cosmic web, we first model an ionizing background due to star-bursting galaxies. We then extract an ensemble of mock absorption spectra from the simulation and compute the mean transmission. We adjust the free parameter, fesc in our model of the ionizing background to reproduce the observed transmission. We find that fesc increases with the minimum galaxy mass considered to contribute to the ionizing background, and that at high redshift fesc must be greater than 5% irrespective of galaxy mass. Based on our numerical results we calibrate a semi-analytic model which shows that the ionizing background observed at z ∼ 5.5–6 implies a sufficient number of ionizing photons to have reionized the Universe by z ∼ 6. However, if the minimum mass for star-formation were ≳109 M⊙, the ionizing background would be over-produced at z ≲ 5. In summary, our results indicate that the Universe was reionized by low mass galaxies.

Keywords

cosmology: diffuse radiationgalaxies: high redshiftintergalactic mediumlarge scale structure of Universe

Information

Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 27 , Issue 1 , 2010 , pp. 110 - 123
Copyright
Copyright © Astronomical Society of Australia 2010

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