Cosmic Reionization on Computers

Properties of the Post-reionization IGM

Nickolay Y. Gnedin, George D. Becker, Xiaohui Fan

Research output: Contribution to journalArticle

13 Citations (Scopus)

Abstract

We present a comparison between several observational tests of the post-reionization intergalactic medium and the numerical simulations of reionization completed under the Cosmic Reionization On Computers (CROC) project. The CROC simulations match the gap distribution reasonably well, and also provide a good match for the distribution of peak heights, but there is a notable lack of wide peaks in the simulated spectra and the fluxprobability distribution functions are poorly matched in the narrow redshift interval 5.5 < z < 5.7, with the match at other redshifts being significantly better, albeit not exact. Both discrepancies are related: simulations show more opacity than the data.

Original languageEnglish (US)
Article number26
JournalAstrophysical Journal
Volume841
Issue number1
DOIs
StatePublished - May 20 2017

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intergalactic media
opacity
simulation
computerized simulation
distribution functions
intervals
computer simulation
distribution
project
comparison
test

Keywords

  • cosmology: theory
  • intergalactic medium
  • large-scale structure of universe
  • methods: numerical

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Cosmic Reionization on Computers : Properties of the Post-reionization IGM. / Gnedin, Nickolay Y.; Becker, George D.; Fan, Xiaohui.

In: Astrophysical Journal, Vol. 841, No. 1, 26, 20.05.2017.

Research output: Contribution to journalArticle

Gnedin, Nickolay Y. ; Becker, George D. ; Fan, Xiaohui. / Cosmic Reionization on Computers : Properties of the Post-reionization IGM. In: Astrophysical Journal. 2017 ; Vol. 841, No. 1.
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