  Our previous investigation of neutron-star crusts, based on the functional
BSk24, led to a substantial reduction of the pasta mantle when Strutinsky
integral and pairing corrections were added on top of the fourth-order extended
Thomas-Fermi method (ETF). Here, our earlier calculations are widened to a
larger set of functionals within the same family, and we find that the
microscopic corrections weaken significantly the influence of the symmetry
energy. In particular, the correlation observed at the pure ETF level between
the density for the onset of pasta formation and the symmetry energy vanishes,
not only for the $L$ coefficient but also for the symmetry-energy values at the
relevant densities. Moreover, the inclusion of microscopic corrections results
in a much lower abundance of pasta for all functionals.
