  We provide the catalogue of all transit-like features, including false
alarms, detected by the CoRoT exoplanet teams in the 177 454 light curves of
the mission. All these detections have been re-analysed with the same softwares
so that to ensure their homogeneous analysis. Although the vetting process
involves some human evaluation, it also involves a simple binary flag system
over basic tests: detection significance, presence of a secondary, difference
between odd and even depths, colour dependence, V-shape transit, and duration
of the transit. We also gathered the information from the large accompanying
ground-based programme carried out on the planet candidates and checked how
useful the flag system could have been at the vetting stage of the candidates.
In total, we identified and separated 824 false alarms of various kind, 2269
eclipsing binaries among which 616 are contact binaries and 1653 are detached
ones, 37 planets and brown dwarfs, and 557 planet candidates. For the planet
candidates, the catalogue gives not only their transit parameters but also the
products of their light curve modelling, together with a summary of the outcome
of follow-up observations when carried out and their current status. Among the
planet candidates whose nature remains unresolved, we estimate that 8 +/- 3
planets are still to be identified. We derived planet and brown dwarf
occurrences and confirm disagreements with Kepler estimates: small-size planets
with orbital period less than ten days are underabundant by a factor of three
in the CoRoT fields whereas giant planets are overabundant by a factor of two.
These preliminary results would however deserve further investigations using
the recently released CoRoT light curves that are corrected of the various
instrumental effects and a homogeneous analysis of the stellar populations
observed by the two missions.
