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The Single-Mirror Small-Sized Telescope, or SST-1M, was originally developedas a prototype of a small-sized telescope for CTA, designed to form an arrayfor observations of gamma-ray-induced atmospheric showers for energies above 3TeV. A pair of SST-1M telescopes is currently being commissioned at theOndrejov Observatory in the Czech Republic, and the telescope capabilities formono and stereo observations are being tested in better astronomicalconditions. The final location for the telescopes will be decided based onthese tests. In this contribution, we present a data analysis pipeline calledsst1mpipe, and the performance of the telescopes when working independently andin a stereo regime.

Mono and stereo performance of the two SST-1M telescope prototypes