The accuracy of seminumerical reionization models in comparison with radiative transfer simulations
Author:
Affiliation:
1. Swinburne University of Technology, Hawthorn, VIC 3122, Australia
2. ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)
Funder
American Society for Radiation Oncology
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/477/2/1549/25009549/sty683.pdf
Reference78 articles.
1. THE PAN-STARRS1 DISTANT z > 5.6 QUASAR SURVEY: MORE THAN 100 QUASARS WITHIN THE FIRST GYR OF THE UNIVERSE
2. REIONIZATION ON LARGE SCALES. I. A PARAMETRIC MODEL CONSTRUCTED FROM RADIATION-HYDRODYNAMIC SIMULATIONS
3. Hydrogen reionization in the Illustris universe
4. The observed ionization rate of the intergalactic medium and the ionizing emissivity at z >= 5: evidence for a photon-starved and extended epoch of reionization
5. THE LYMAN-CONTINUUM PHOTON PRODUCTION EFFICIENCYξIONOFz∼ 4–5 GALAXIES FROM IRAC-BASED HαMEASUREMENTS: IMPLICATIONS FOR THE ESCAPE FRACTION AND COSMIC REIONIZATION
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