  We briefly review how to compute the mass and angular momenta of rotating,
asymptotically anti-de Sitter spacetimes in Einstein-Gauss-Bonnet theory of
gravity using superpotentials derived from standard Noether identities. The
calculations depend on the asymptotic form of the metrics only and hence take
no account of the source of the curvature. When the source of curvature is a
black hole, the results can be checked using the first law of black hole
thermodynamics.
