We present a detailed analysis of gravity in a partial Bondi gauge,
where only the three conditions g_{rr}=0=g_{rA}grr=0=grA
are fixed. We relax in particular the so-called determinant condition on
the transverse metric, which is only assumed to admit a polyhomogeneous
radial expansion. This is sufficient in order to build the solution
space, which here includes a cosmological constant, time-dependent
sources in the boundary metric, logarithmic branches, and an extra trace
mode at subleading order in the transverse metric. The evolution
equations are studied using the Newman–Penrose formalism in terms of
covariant functionals identified from the Weyl scalars, and we build the
explicit dictionary between this formalism and the tensorial Einstein
equations. This provides in particular a new derivation of the (A)dS
mass loss formula. We then study the holographic renormalisation of the
symplectic potential, and the transformation laws under residual
asymptotic symmetries. The advantage of the partial Bondi gauge is that
it allows to contrast and treat in a unified manner the Bondi–Sachs and
Newman–Unti gauges, which can each be reached upon imposing a further
specific gauge condition. The differential determinant condition leads
to the \LambdaΛ-BMSW
gauge, while a differential condition on g_{ur}gur
leads to a generalized Newman–Unti gauge. This latter gives access to a
new asymptotic symmetry which acts on the asymptotic shear and further
extends the \LambdaΛ-BMSW
group by an extra abelian radial translation. This generalizes results
which we have recently obtained in three dimensions.