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 .