Primary science goals

Primary science goals:

  1. Photometry of a sample (defined later) of open clusters basic physical parameters measured in a uniform way;
  2. Time domain study of variable objects in selected clusters: long time based line, high cadence and high duty cycle, high precision photometric observations;
     
    • A complete survey (defined later) of stellar variabilities along the main sequence (d Scu, b Cep & g Dor etc……) in selected open clusters;
    • A complete survey (defined later) of small and large amplitude red variables along the RGBs of selected open clusters;
    • A complete survey (defined later) of eclipsing binaries in selected clusters;
    • Looking for transit of exoplanet systems;
    • Looking for flare type variabilities in selected clusters;
    • Stellar rotation and spots activities;
    • ……
  3. Time domain study of selected field areas;