  We investigate the expected radio emission from short GRBs, guided by the
observed distributions of their afterglow parameters. Our motivation is to
explore the radio signatures of the forward and reverse shock in a sGRB jet, as
well as the off-axis jet component and radio emission from the dynamical
ejecta. We estimate the fraction of GRBs detectable in the radio that may be
coincident with a GW signal from a neutron star (NS) merger. At the distance to
which aLIGO at design specification is sensitive to GWs from NS mergers, we may
detect up to 20 % of off-axis jet radio components of these events, and up to
about 10 % of events with radio emission from the tidal ejecta shocking with
the external medium. We discuss our results in light of the Next Generation
Very Large Array, expected to make significant progress in detecting radio
signals from sGRBs.
