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With only two functional reaction wheels, Kepler cannot maintain stablepointing at its original target field and entered a new mode of observationcalled K2. Our method is based on many years of experience in planet huntingfor the CoRoT mission. Due to the unstable pointing, K2 light curves presentsystematics that are correlated with the target position in the CCD. Therefore,our pipeline also includes a decorrelation of this systematic noise. Ourpipeline is optimised for bright stars for which spectroscopic follow-up ispossible. We achieve a maximum precision on 6 hours of 6 ppm. The decorrelatedlight curves are searched for transits with an adapted version of the CoRoTalarm pipeline. We present 172 planetary candidates and 327 eclipsing binarycandidates from campaigns 1, 2, 3, 4, 5 and 6 of K2. Both the planetarycandidates and eclipsing binary candidates lists are made public to promotefollow-up studies. The light curves will also be available to the community.

New planetary and EB candidates from Campaigns 1-6 of the K2 mission