The dispersion model yields unbiased fσ8 inferences from cluster 2PCF multipoles down to 10 h^{-1} Mpc in Euclid DR1-like settings with photometric redshift errors.
Contribution of the hexadecapole10 For the investigation of the contribution ofℓ=4 we compare thefσ 8 posteriors with and without including it in the inference
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Testing template-fitting models for the multipoles of the two-point clustering of galaxy clusters
The dispersion model yields unbiased fσ8 inferences from cluster 2PCF multipoles down to 10 h^{-1} Mpc in Euclid DR1-like settings with photometric redshift errors.