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turboGL is a fast Mathematica code based on a stochastic approach to cumulative weak lensing. It can easily compute the lensing PDF relative to arbitrary halo mass distributions, selection biases, number of observations, halo profiles and evolutions, making it a useful tool to study how lensing depends on cosmological parameters and impact on observations.
CalPriorSNIa quickly computes the effective calibration prior on the absolute magnitude MB of Type Ia supernovae that corresponds to a given determination of H0.