https://github.com/xuod/NumCosmo/blob/master/NEWS
NcClusterMass * NcClusterMass object was adapted to NcmModel. * Now the parameters of the mass-observable (M-O) relation can be fitted. Therefore it is able to simultaneously fit both M-O and cosmological parameters (self-calibration). * The integrals of NcClusterMassVanderlinde and NcClusterMassBenson were optimized. Vanderlinde et al. http://arxiv.org/abs/1003.0003. Benson et al. http://arxiv.org/abs/1112.5435. Tinker Multiplicity Function: improvement * Tinker et al. multiplicity function, when dark matter halo mass is defined in terms of the critical density, is computed using a spline defined in the interval 200 <= Delta(z) <= 3200. * Improvement: This function was extended to Delta(z) > 3200. In this case the multiplicity function is computed using the fitting function given by Eqs.(B1 -- B4) in http://arxiv.org/abs/0803.2706. This extension was done properly to ensure the continuity of the multiplicity function.