kNN CDF statistics detect 21cm-galaxy cross-correlations more effectively than two-point methods and distinguish reionization models at fixed ionized fraction even with noise and foregrounds.
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3 Pith papers cite this work. Polarity classification is still indexing.
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SARAS3 data sets T21 ≳ -277.6 mK at z=23.6 (3σ) in IDM models and finds no preference for IDM over CDM (Bayes factor ≈1.7).
Strong-feedback models with bright galaxies match JWST UVLF at z greater than or equal to 10 and predict an extended reionization from z approximately 16 to 6 that fits CMB optical depth within 2 sigma.
citing papers explorer
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Nearest Neighbour-Based Statistics for 21cm-Galaxy Cross-Correlations in the Epoch of Reionization
kNN CDF statistics detect 21cm-galaxy cross-correlations more effectively than two-point methods and distinguish reionization models at fixed ionized fraction even with noise and foregrounds.
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Implications of \textit{SARAS3} data for Coulomb-like interacting dark matter
SARAS3 data sets T21 ≳ -277.6 mK at z=23.6 (3σ) in IDM models and finds no preference for IDM over CDM (Bayes factor ≈1.7).
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Towards Reconciling Reionization with JWST: The Role of Bright Galaxies and Strong Feedback
Strong-feedback models with bright galaxies match JWST UVLF at z greater than or equal to 10 and predict an extended reionization from z approximately 16 to 6 that fits CMB optical depth within 2 sigma.