A method to extract f(z) at the zeros of derivatives of fσ8(z) using only galaxy clustering and BAO data, without CMB or weak lensing inputs.
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Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys
A method to extract f(z) at the zeros of derivatives of fσ8(z) using only galaxy clustering and BAO data, without CMB or weak lensing inputs.