Measurements of one-point statistics in 21-cm intensity maps via foreground avoidance strategy

Author:

Kittiwisit Piyanat12ORCID,Bowman Judd D2,Murray Steven G2ORCID,Gehlot Bharat K23ORCID,Jacobs Daniel C2,Beardsley Adam P24

Affiliation:

1. Department of Physics and Astronomy, University of the Western Cape , Cape Town, 7535, South Africa

2. School of Earth and Space Exploration, Arizona State University , Tempe, AZ 85287-6004, USA

3. Kapteyn Astronomical Institute, University of Groningen , PO Box 800, NL-9700AV Groningen, the Netherlands

4. Physics Department, Winona State University , Pasteur 120, Winona, MN 55987, USA

Abstract

ABSTRACT Measurements of the one-point probability distribution function and higher-order moments (variance, skewness, and kurtosis) of the high-redshift 21-cm fluctuations are among the most direct statistical probes of the non-Gaussian nature of structure formation and evolution during re-ionization. However, contamination from astrophysical foregrounds and instrument systematics pose significant challenges in measuring these statistics in real observations. In this work, we use forward modelling to investigate the feasibility of measuring 21-cm one-point statistics through a foreground avoidance strategy. Leveraging the characteristic wedge-shape of the foregrounds in k-space, we apply a wedge-cut filtre that removes the foreground contaminated modes from a mock data set based on the Hydrogen Epoch of Re-ionization Array (HERA) instrument, and measure the one-point statistics from the image-space representation of the remaining non-contaminated modes. We experiment with varying degrees of wedge-cutting over different frequency bandwidths and find that the centre of the band is the least susceptible to bias from wedge-cutting. Based on this finding, we introduce a rolling filtre method that allows reconstruction of an optimal wedge-cut 21-cm intensity map over the full bandwidth using outputs from wedge-cutting over multiple sub-bands. We perform Monte Carlo simulations to show that HERA should be able to measure the rise in skewness and kurtosis near the end of re-ionization with the rolling wedge-cut method if foreground leakage from the Fourier transform window function can be controlled.

Funder

National Science Foundation

European Research Council

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 3 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. How informative are summaries of the cosmic 21 cm signal?;Astronomy & Astrophysics;2024-08

2. Aliasing from Galactic Plane Setting in Widefield Radio Interferometry;The Astrophysical Journal;2024-03-28

3. Skew spectrum and smoothed skewness of 21-cm signals from epoch of reionization;Monthly Notices of the Royal Astronomical Society;2023-05-12

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