Sebastian Bocquet's repositories
MiraTitanHMFemulator
Emulator for the halo mass function (HMF) from the Mira-Titan Universe suite of cosmological N-body simulations.
PosteriorAgreement
Quantify whether the difference between two posterior distributions is consistent with zero difference. Accepts samples from one- or multidimensional posterior distributions.
SPT_SZ_cluster_likelihood
SPT-SZ cluster cosmology likelihood code and data to reproduce Bocquet et al. 2019
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xshear
Measure the tangential shear around a set of lenses
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