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This paper discusses the use of visibility correlations in radio-interferometric observations to study the distribution of neutral hydrogen (H I) from the dark ages to the present epoch. The authors propose a formalism that quantifies the statistical properties of fluctuations in redshifted 21-cm radiation, which provides insights into cosmological structure formation and the epoch of reionization. The study emphasizes the advantages of directly analyzing visibilities over traditional imaging techniques, al

Author
Purnendu Sheet
Language
EN