期刊
ASTROPHYSICAL JOURNAL
卷 608, 期 2, 页码 611-621出版社
UNIV CHICAGO PRESS
DOI: 10.1086/420735
关键词
cosmology : theory; diffuse radiation; galaxies : formation; intergalactic medium; large-scale structure of universe; radio lines : general
We use cosmological simulations of reionization to predict the possible signal from the redshifted 21 cm line of neutral hydrogen in the pre-reionization era and to investigate the observability of this signal. We show that the separation of the mean (global) signal over the whole sky from the known foreground contamination may be feasible but very challenging. In agreement with previous studies, we demonstrate that measuring angular fluctuations in the H 1 signal is likely to be extremely difficult if not impossible because of the overwhelming contamination from the Galactic and extragalactic foregrounds. However, we show that the sharp H 1 fluctuations in the frequency domain should be easily separable from the relatively smooth spectra of the foregrounds and that these fluctuations should be detectable even at moderate angular resolution (similar to10'-20').
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据