  We consider solutions of the Einstein equations with cosmological constant
$\Lambda\neq 0$ admitting conformal compactification with smooth scri
$\mathscr{I^+}$. Metrics are written in the Bondi-Sachs coordinates and
expanded into inverse powers of the affine distance $r$. Unlike in the case
$\Lambda=0$ all free data are located on the scri. There are linear
differential constraints on the Bondi mass and angular momentum aspects. All
other components of metrics are defined in a recursive way.
