Abstract
Efforts are being made to observe the 21-cm signal from the 'cosmic dawn' using sky-averaged observations with individual radio dipoles. In this paper, we develop a model of the observations accounting for the 21-cm signal, foregrounds and several major instrumental effects. Given this model, we apply Markov Chain Monte Carlo techniques to demonstrate the ability of these instruments to separate the 21-cm signal from foregrounds and quantify their ability to constrain properties of the first galaxies. For concreteness, we investigate observations between 40 and 120MHz with the proposedDark Ages Radio Explorermission in lunar orbit, showing its potential for science return.
Original language | English (US) |
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Pages (from-to) | 1070-1084 |
Number of pages | 15 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 419 |
Issue number | 2 |
DOIs | |
State | Published - Jan 2012 |
Keywords
- Cosmology: theory
- Diffuse radiation
- Methods: statistical
- Radio lines: general
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science