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 km s ^ { -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 .