Statistics of the epoch of reionization 21-cm signal - I. Power spectrum error-covariance
File(s)stv2772.pdf (4.58 MB)
Published version
Author(s)
Mondal, R
Bharadwaj, S
Majumdar, S
Type
Journal Article
Abstract
The non-Gaussian nature of the epoch of reionization (EoR) 21-cm signal has a significant
impact on the error variance of its power spectrum P(k). We have used a large ensemble
of seminumerical simulations and an analytical model to estimate the effect of this nonGaussianity
on the entire error-covariance matrix Cij. Our analytical model shows that Cij
has contributions from two sources. One is the usual variance for a Gaussian random field
which scales inversely of the number of modes that goes into the estimation of P(k). The
other is the trispectrum of the signal. Using the simulated 21-cm Signal Ensemble, an ensemble
of the Randomized Signal and Ensembles of Gaussian Random Ensembles we have
quantified the effect of the trispectrum on the error variance Cii. We find that its relative
contribution is comparable to or larger than that of the Gaussian term for the k range 0.3 ≤ k
≤ 1.0 Mpc−1, and can be even ∼200 times larger at k ∼ 5 Mpc−1. We also establish that the
off-diagonal terms of Cij have statistically significant non-zero values which arise purely from
the trispectrum. This further signifies that the error in different k modes are not independent.
We find a strong correlation between the errors at large k values (≥0.5 Mpc−1), and a weak
correlation between the smallest and largest k values. There is also a small anticorrelation
between the errors in the smallest and intermediate k values. These results are relevant for the
k range that will be probed by the current and upcoming EoR 21-cm experiments.
impact on the error variance of its power spectrum P(k). We have used a large ensemble
of seminumerical simulations and an analytical model to estimate the effect of this nonGaussianity
on the entire error-covariance matrix Cij. Our analytical model shows that Cij
has contributions from two sources. One is the usual variance for a Gaussian random field
which scales inversely of the number of modes that goes into the estimation of P(k). The
other is the trispectrum of the signal. Using the simulated 21-cm Signal Ensemble, an ensemble
of the Randomized Signal and Ensembles of Gaussian Random Ensembles we have
quantified the effect of the trispectrum on the error variance Cii. We find that its relative
contribution is comparable to or larger than that of the Gaussian term for the k range 0.3 ≤ k
≤ 1.0 Mpc−1, and can be even ∼200 times larger at k ∼ 5 Mpc−1. We also establish that the
off-diagonal terms of Cij have statistically significant non-zero values which arise purely from
the trispectrum. This further signifies that the error in different k modes are not independent.
We find a strong correlation between the errors at large k values (≥0.5 Mpc−1), and a weak
correlation between the smallest and largest k values. There is also a small anticorrelation
between the errors in the smallest and intermediate k values. These results are relevant for the
k range that will be probed by the current and upcoming EoR 21-cm experiments.
Date Issued
2015-12-30
Date Acceptance
2015-11-23
Citation
Monthly Notices of the Royal Astronomical Society, 2015, 456 (2), pp.1936-1947
ISSN
0035-8711
Publisher
Oxford University Press
Start Page
1936
End Page
1947
Journal / Book Title
Monthly Notices of the Royal Astronomical Society
Volume
456
Issue
2
Copyright Statement
© 2015 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. The definitive publisher-authenticated version Rajesh Mondal, Somnath Bharadwaj, Suman Majumdar; Statistics of the epoch of reionization 21-cm signal – I. Power spectrum error-covariance, Monthly Notices of the Royal Astronomical Society, Volume 456, Issue 2, 21 February 2016, Pages 1936–1947 is available online at: https://dx.doi.org/10.1093/mnras/stv2772
Subjects
Science & Technology
Physical Sciences
Astronomy & Astrophysics
methods: statistical
cosmology: theory
dark ages, reionization
first stars
diffuse radiation
21 CM RADIATION
COSMIC REIONIZATION
INTERGALACTIC MEDIUM
PECULIAR VELOCITIES
HII-REGIONS
150 MHZ
FLUCTUATIONS
CONSTRAINTS
FOREGROUNDS
MATTER
astro-ph.CO
0201 Astronomical And Space Sciences
Notes
archiveprefix: arXiv keywords: methods: statistical, cosmology: theory, dark ages, reionization, first stars, diffuse radiation adsurl: http://adsabs.harvard.edu/abs/2016MNRAS.456.1936M adsnote: Provided by the SAO/NASA Astrophysics Data System