| Abstract |  | We describe an automated implementation of a Tokovinin Mass-Dimm unit on a 12" Meade RCX400 telescope, installed in the old 18-inch dome at Palomar Observatory. The system operates automatically every clear night. Results of the Free & Boundary seeing, height resolved MASS data, derived values including the Fried parameter and isoplanatic angle, are displayed in real time and stored in a data base, and can be compared with similar data from a nearby TMT-Halfmann Mass-Dimm system. These data provide useful feedback for observers, and can also be used to improve data analysis through enhanced PSF fitting.
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