A proof-of-concept showing that large-scale 21-cm power spectrum and bispectrum, plus an independent measurement of the cosmic HI density, can constrain the parameters of the HI mass-halo mass relation at z=1.
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Probing the HI distribution at small scales using 21-cm Intensity Mapping at large scales
A proof-of-concept showing that large-scale 21-cm power spectrum and bispectrum, plus an independent measurement of the cosmic HI density, can constrain the parameters of the HI mass-halo mass relation at z=1.