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Impacts and Statistical Mitigation of Missing Data on the 21cm Power Spectrum: A Case Study with the Hydrogen Epoch of Reionization Array

Authors :
Chen, Kai-Feng
Wilensky, Michael J.
Liu, Adrian
Dillon, Joshua S.
Hewitt, Jacqueline N.
Adams, Tyrone
Aguirre, James E.
Baartman, Rushelle
Beardsley, Adam P.
Berkhout, Lindsay M.
Bernardi, Gianni
Billings, Tashalee S.
Bowman, Judd D.
Bull, Philip
Burba, Jacob
Byrne, Ruby
Carey, Steven
Choudhuri, Samir
Cox, Tyler
DeBoer, David R.
Dexter, Matt
Eksteen, Nico
Ely, John
Ewall-Wice, Aaron
Furlanetto, Steven R.
Gale-Sides, Kingsley
Garsden, Hugh
Gehlot, Bharat Kumar
Gorce, Adélie
Gorthi, Deepthi
Halday, Ziyaad
Hazelton, Bryna J.
Hickish, Jack
Jacobs, Daniel C.
Josaitis, Alec
Kern, Nicholas S.
Kerrigan, Joshua
Kittiwisit, Piyanat
Kolopanis, Matthew
La Plante, Paul
Lanman, Adam
Ma, Yin-Zhe
MacMahon, David H. E.
Malan, Lourence
Malgas, Cresshim
Malgas, Keith
Marero, Bradley
Martinot, Zachary E.
McBride, Lisa
Mesinger, Andrei
Mohamed-Hinds, Nicel
Molewa, Mathakane
Morales, Miguel F.
Murray, Steven G.
Nuwegeld, Hans
Parsons, Aaron R.
Pascua, Robert
Qin, Yuxiang
Rath, Eleanor
Razavi-Ghods, Nima
Robnett, James
Santos, Mario G.
Sims, Peter
Singh, Saurabh
Storer, Dara
Swarts, Hilton
Tan, Jianrong
van Wyngaarden, Pieter
Zheng, Haoxuan
Publication Year :
2024

Abstract

The precise characterization and mitigation of systematic effects is one of the biggest roadblocks impeding the detection of the fluctuations of cosmological 21cm signals. Missing data in radio cosmological experiments, often due to radio frequency interference (RFI), poses a particular challenge to power spectrum analysis as it could lead to the ringing of bright foreground modes in Fourier space, heavily contaminating the cosmological signals. Here we show that the problem of missing data becomes even more arduous in the presence of systematic effects. Using a realistic numerical simulation, we demonstrate that partially flagged data combined with systematic effects can introduce significant foreground ringing. We show that such an effect can be mitigated through inpainting the missing data. We present a rigorous statistical framework that incorporates the process of inpainting missing data into a quadratic estimator of the 21cm power spectrum. Under this framework, the uncertainties associated with our inpainting method and its impact on power spectrum statistics can be understood. These results are applied to the latest Phase II observations taken by the Hydrogen Epoch of Reionization Array, forming a crucial component in power spectrum analyses as we move toward detecting 21cm signals in the ever more noisy RFI environment.<br />Comment: 25 pages, 11 figures, submitted to ApJ

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.2411.10529
Document Type :
Working Paper