Journal article icon

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...

Expand abstract
Publication status:
Published
Peer review status:
Peer reviewed

Actions

  • Cite

  • Print

Access Document

Files:
Publisher copy:
10.1093/mnras/sty3154

Authors

More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Oxford college:
Brasenose College
Role:
Author
More authors...
More from this funder
Funding agency for:
Katz, HB
Grant:
Nicholas Kurti Junior Fellowship
More from this funder
Funding agency for:
Katz, HB
Grant:
Nicholas Kurti Junior Fellowship
More from this funder
Grant:
Advanced Grant 320596 “The Emergence of Structure during the Epoch of reionization"
Publisher:
Oxford University Press
Journal:
Monthly Notices of the Royal Astronomical Society More from this journal
Volume:
483
Issue:
1
Pages:
1029–1041
Publication date:
2018-11-23
Acceptance date:
2018-11-20
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
Keywords:
Pubs id:
pubs:944634
UUID:
uuid:c285d0de-18d7-4f2c-9239-45a201f4be3a
Local pid:
pubs:944634
Source identifiers:
944634
Deposit date:
2018-11-20

Terms of use

Views and Downloads





If you are the owner of this record, you can report an update to it here: Report update to this record

TO TOP