  We present a kinematically-unbiased search to identify young, nearby low-mass
members of kinematic moving groups (MGs). Objects with both rotation periods
shorter than 5 days in the SuperWASP All-Sky Survey and X-ray counterparts in
the ROSAT All-Sky Survey were chosen to create a catalog of several thousand
rapidly-rotating, X-ray active FGK stars. These objects are expected to be
either young single stars or tidally-locked spectroscopic binaries. We obtained
optical spectra for a sub-sample of 146 stars to determine their ages and
kinematics, and in some cases repeat radial velocity (RV) measurements were
used to identify binarity. Twenty-six stars are found to have lithium
abundances consistent with an age of <=200 Myr, and show no evidence for
binarity and in most cases measurements of H-alpha and v\sin i support their
youthful status. Based on their youth, their radial velocities and estimates of
their 3-dimensional kinematics, we find 11 objects that may be members of known
MGs, 8 that do not appear associated with any young MG and a further 7 that are
close to the kinematics of the recently proposed "Octans-Near" MG, and which
may be the first members of this MG found in the northern hemisphere. The
initial search mechanism was ~18 per cent efficient at identifying
likely-single stars younger than 200 Myr, of which 80 per cent were early-K
spectral types.
