21CMMC with a 3D light-cone: the impact of the co-evolution approximation on the astrophysics of reionization and cosmic dawn-Reference-Cited by-同舟云学术

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21CMMC with a 3D light-cone: the impact of the co-evolution approximation on the astrophysics of reionization and cosmic dawn

Published:2018-03-27 Issue:3 Volume:477 Page:3217-3229
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Greig Bradley¹²³,Mesinger Andrei³

Affiliation:

1. ARC Centre of Excellence for All-Sky Astrophysics in 3 Dimensions (ASTRO 3D), University of Melbourne, VIC 3010, Australia

2. School of Physics, University of Melbourne, Parkville, VIC 3010, Australia

3. Scuola Normale Superiore, Piazza dei Cavalieri 7, I-56126 Pisa, Italy

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/477/3/3217/24802887/sty796.pdf

Reference87 articles.

1. The Formation of the First Star in the Universe

2. CosmoHammer: Cosmological parameter estimation with the MCMC Hammer

3. THE EFFECT OF ABSORPTION SYSTEMS ON COSMIC REIONIZATION

4. In the beginning: the first sources of light and the reionization of the universe

5. A Method for Separating the Physics from the Astrophysics of High-Redshift 21 Centimeter Fluctuations

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