  To analyze the SACY (Search for Associations Containing Young stars) survey
we developed a method to find young associations and to define their high
probability members. These bona fide members enable to obtain the kinematical
and the physical properties of each association in a proper way. Recently we
noted a concentration in the UV plane and we found a new association we are
calling ASYA (All Sky Young Association) for its overall distribution in the
sky with a total of 38 bonafide members and an estimated age of 110 Myr, the
oldest young association found in the SACY survey. We present here its
kinematical, space and Li distributions and its HR diagram.
