Exploring One-point Statistics in HERA Phase I Data: Effects of Foregrounds and Systematics on Measuring One-point Statistics

Abstract Measuring one-point statistics in redshifted 21 cm intensity maps offers an opportunity to explore non-Gaussian features of the early Universe. We assess the impact of instrumental effects on measurements made with the Hydrogen Epoch of Reionization Array (HERA) by forward modeling observational and simulation data. Using HERA Phase I observations over 94 nights, we examine the second ( m 2 , variance) and third ( m 3 ) moments of images. We employ the DAYENU -filtering method for foreground removal and reduce simulated foreground residuals to 10% of the 21 cm signal residuals. In noiseless cosmological simulations, the amplitudes of one-point statistics measurements are significantly reduced by the instrument response and further reduced by wedge-filtering. Analyses with wedge-filtered observational data, along with expected noise simulations, show that systematics alter the probability distribution of the map pixels. A likelihood analysis based on the observational data shows m 2 measurements disfavor the cold reionization model characterized by inefficient X-ray heating, in line with other power spectra measurements. Small signals in m 3 due to the instrument response of the Phase I observation and wedge-filtering make it challenging to use these non-Gaussian statistics to explore model parameters. Forecasts with the full HERA array predict high signal-to-noise ratios for m 2 , m 3 , and S 3 assuming no foregrounds, but wedge-filtering drastically reduces these ratios. This work demonstrates conclusively that a comprehensive understanding of instrumental effects on m 2 and m 3 is essential for their use as a cosmological probe, given their dependence on the underlying model.

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Publication Details

Journal
The Astrophysical Journal
Published
2025-11-03
DOI
https://doi.org/10.3847/1538-4357/ae032e
Citations
2
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
2.31

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article

Exploring One-point Statistics in HERA Phase I Data: Effects of Foregrounds and Systematics on Measuring One-point Statistics

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2 citations
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Galaxies: Formation, Evolution, Phenomena
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article

Exploring One-point Statistics in HERA Phase I Data: Effects of Foregrounds and Systematics on Measuring One-point Statistics

Bradley Marero, Haoxuan Zheng, Eloy de Lera Acedo, Hans Nuwegeld, Honggeun Kim, Tashalee S. Billings, James Robnett, Piyanat Kittiwisit, M. F. Morales, Ziyaad Halday, Adrian Liu, Aaron Ewall‐Wice, Jacob Burba, Joshua Kerrigan, G. Bernardi, Nico Eksteen, Philip Bull, Joshua S. Dillon, Peter Sims, David R. DeBoer, J. Hickish, Tyrone Adams, Mathakane Molewa, Cresshim Malgas, Lourence Malan, Adam P. Beardsley, Steven Murray, N. Razavi‐Ghods, Adam Lanman, Keith Malgas, Hilton Swarts, Daniel Jacobs, Deepthi Gorthi, Tshegofalang Mosiane, Vincent MacKay, Richard F. Bradley, Eleanor Rath, Nicholas S. Kern, Matthew Kolopanis, Paul La Plante, C. L. Carilli, Zhilei Xu, Nicolas Fagnoni, Zachary E. Martinot, Nithyanandan Thyagarajan, Pieter van Wyngaarden, Bradley Greig, David MacMahon, Brian Glendenning, Jasper Grobbelaar, James Aguirre, Steven R. Furlanetto, Andrei Mesinger, Jacqueline N. Hewitt, B. J. Hazelton, Judd D. Bowman, Rushelle Baartman, Aaron R. Parsons, Kingsley Gale‐Sides, Steven Carey, Kai-Feng Chen, Craig Smith, Matt Dexter, John Ely
article en
2 citations

Abstract

Abstract Measuring one-point statistics in redshifted 21 cm intensity maps offers an opportunity to explore non-Gaussian features of the early Universe. We assess the impact of instrumental effects on measurements made with the Hydrogen Epoch of Reionization Array (HERA) by forward modeling observational and simulation data. Using HERA Phase I observations over 94 nights, we examine the second ( m 2 , variance) and third ( m 3 ) moments of images. We employ the DAYENU -filtering method for foreground removal and reduce simulated foreground residuals to 10% of the 21 cm signal residuals. In noiseless cosmological simulations, the amplitudes of one-point statistics measurements are significantly reduced by the instrument response and further reduced by wedge-filtering. Analyses with wedge-filtered observational data, along with expected noise simulations, show that systematics alter the probability distribution of the map pixels. A likelihood analysis based on the observational data shows m 2 measurements disfavor the cold reionization model characterized by inefficient X-ray heating, in line with other power spectra measurements. Small signals in m 3 due to the instrument response of the Phase I observation and wedge-filtering make it challenging to use these non-Gaussian statistics to explore model parameters. Forecasts with the full HERA array predict high signal-to-noise ratios for m 2 , m 3 , and S 3 assuming no foregrounds, but wedge-filtering drastically reduces these ratios. This work demonstrates conclusively that a comprehensive understanding of instrumental effects on m 2 and m 3 is essential for their use as a cosmological probe, given their dependence on the underlying model.

The Astrophysical JournalVol. 993(2)
National Science Foundation, National Aeronautics and Space Administration, Gordon and Betty Moore Foundation, Massachusetts Institute of Technology, Space Telescope Science Institute
Openalex Percentile: Top 10%
Galaxies: Formation, Evolution, Phenomena
2.31
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