Statistics of the epoch of reionization (EoR) 21-cm signal - II. The evolution of the power-spectrum error-covariance

被引:52
作者
Mondal, Rajesh [1 ,2 ]
Bharadwaj, Somnath [1 ,2 ]
Majumdar, Suman [3 ]
机构
[1] Indian Inst Technol Kharagpur, Dept Phys, Kharagpur 721302, W Bengal, India
[2] Indian Inst Technol Kharagpur, Ctr Theoret Studies, Kharagpur 721302, W Bengal, India
[3] Imperial Coll, Blackett Lab, Dept Phys, London SW7 2AZ, England
基金
欧洲研究理事会;
关键词
methods: statistical; cosmology: theory; dark ages; reionization; first stars; diffuse radiation; large-scale structure of Universe; 21 CM RADIATION; COSMIC REIONIZATION; HII-REGIONS; 150; MHZ; CONSTRAINTS; GALAXIES; LOFAR; DAWN; I; FLUCTUATIONS;
D O I
10.1093/mnras/stw2599
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The epoch of reionization (EoR) 21-cm signal is expected to become highly non-Gaussian as reionization progresses. This severely affects the error-covariance of the EoR 21-cm power spectrum that is important for predicting the prospects of a detection with ongoing and future experiments. Most earlierworks have assumed that the EoR 21-cm signal is aGaussian random field where (1) the error-variance depends only on the power spectrum and the number of Fourier modes in the particular k bin, and (2) the errors in the different k bins are uncorrelated. Here, we use an ensemble of simulated 21-cm maps to analyse the error-covariance at various stages of reionization. We find that even at the very early stages of reionization ((x) over bar (HI) similar to 0.9), the error-variance significantly exceeds the Gaussian predictions at small length-scales (k > 0.5Mpc(-1)) while they are consistent at larger scales. The errors in most k bins (both large and small scales) are however found to be correlated. Considering the later stages ((x) over bar (HI) = 0.15), the error-variance shows an excess in all k bins within k >= 0.1Mpc(-1), and it is around 200 times larger than the Gaussian prediction at k similar to 1Mpc(-1). The errors in the different k bins are all also highly correlated, barring the two smallest k bins that are anti-correlated with the other bins. Our results imply that the predictions for different 21-cm experiments based on the Gaussian assumption underestimate the errors, and it is necessary to incorporate the non-Gaussianity for more realistic predictions.
引用
收藏
页码:2992 / 3004
页数:13
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