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The BEST wide-angle telescope installed at the Observatoire de Haute-Provenceand operated in remote control from Berlin by the Institut fuerPlanetenforschung, DLR, has observed the CoRoT target fields prior to themission. The resulting archive of stellar photometric lightcurves is used tosearch for deep transit events announced during CoRoT's alarm-mode to aid infast photometric confirmation of these events. The "initial run" field of CoRoT(IRa01) has been observed with BEST in November and December 2006 for 12nights. The first "long run" field (LRc01) was observed from June to September2005 for 35 nights. After standard CCD data reduction, aperture photometry hasbeen performed using the ISIS image subtraction method. About 30,000lightcurves were obtained in each field. Transits of the first detected planetsby the CoRoT mission, CoRoT-1b and CoRoT-2b, were found in archived data of theBEST survey and their lightcurves are presented here. Such detections provideuseful information at the early stage of the organization of follow-upobservations of satellite alarm-mode planet candidates. In addition, no periodchange was found over ~4 years between the first BEST observation and lastavailable transit observations.

Pre-discovery observations of CoRoT-1b and CoRoT-2b with the BEST survey