  Using the kinematically unbiased technique described in Binks, Jeffries &
Maxted (2015), we present optical spectra for a further 122 rapidly-rotating
(rotation periods < 6 days), X-ray active FGK stars, selected from the
SuperWASP survey. We identify 17 new examples of young, probably single stars
with ages of < 200 Myr and provide additional evidence for a new northern
hemisphere kinematic association: the Pisces Moving Group (MG). The group
consists of 14 lithium-rich G- and K-type stars, that have a dispersion of only
$\sim $3 kms$^{-1}$ in each Galactic space velocity coordinate. The group
members are approximately co-eval in the colour-magnitude diagram, with an age
of 30-50 Myr, and have similar, though not identical, kinematics to the
Octans-Near MG.
