The tables present average parameters of a Wigner-Seitz cell in an inner crust of a neutron star, considering nuclear mixtures that arise due to the nuclear statistical equilibrium conditions at the original crust formation. The four tables represent results of computations performed according to the Brussels-Montreal equation-of-state (EoS) models BSk22, BSk24, BSk25, and BSk26. For different mean number densities of baryons n_bar, each table gives an average number of protons in a Wigner-Seitz cell Z_cell, an average number of protons in a nuclear cluster at the center of a Wigner-Seitz cell Z_clust, an average number of nucleons (protons and neutrons) in a Wigner-Seitz cell A_cell, an average number of nucleons in a nuclear cluster at the center of a Wigner-Seitz cell A_clust, and the impurity parameter (the mean-square deviation of Z_clust from its average value) Q_imp.

Alexander Potekhin, palex(at)astro.ioffe.ru