  This work is based on a bottom{-}up approach to the standard{-}model
effective field theory (SMEFT), resulting in an equiprobable space of Wilson
coefficients. The randomly generated Wilson coefficients of the SMEFT (in the
Warsaw basis) are treated as pseudo-data and, for each observable, the
corresponding probability density function is computed. The goal has been to
understand how large are the deviations from the SM once the SMEFT scale and
the range of the Wilson coefficients are selected. Correlations between
different observables are also discussed.
