  Aims. A summary of the CoRoT brown dwarf investigations are presented.
Methods. Transiting brown dwarfs around solar like stars were studied by using
the photometric time-series of CoRoT, and ground based radial velocity
measurements. Results. CoRoT detected three transiting brown dwarfs around F
and G dwarf stars. The occurence rate of brown dwarfs was found to be 0.20 +/-
0.15% around solar-like stars which is compatible with the value obtained by
Kepler-data.
