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Journal article

Tracing the sources of reionization in cosmological radiation hydrodynamics simulations

Abstract:

We use the photon flux and absorption tracer algorithm presented in Katz et al. 2018, to characterise the contribution of haloes of different mass and stars of different age and metallicity to the reionization of the Universe. We employ a suite of cosmological multifrequency radiation hydrodynamics AMR simulations that are carefully calibrated to reproduce a realistic reionization history and galaxy properties at z ≥ 6. In our simulations, haloes with mass 109M⊙h−1 < M < 1010M⊙h−1, star...

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Publication status:
Published
Peer review status:
Peer reviewed
Version:
Publisher's version

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Publisher copy:
10.1093/mnras/sty3154

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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics
Subgroup:
Astrophysics
Oxford college:
Brasenose College
Role:
Author
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Grant:
Advanced Grant 320596 “The Emergence of Structure during the Epoch of reionization"
Publisher:
Oxford University Press Publisher's website
Journal:
Monthly Notices of the Royal Astronomical Society Journal website
Volume:
483
Issue:
1
Pages:
1029–1041
Publication date:
2018-11-23
Acceptance date:
2018-11-20
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
Pubs id:
pubs:944634
URN:
uri:c285d0de-18d7-4f2c-9239-45a201f4be3a
UUID:
uuid:c285d0de-18d7-4f2c-9239-45a201f4be3a
Local pid:
pubs:944634

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