Light curve of EPIC 201659529 as an example for our method for correcting the raw K2 LCs. Panel a: vdb-LC from which we extracted the detrending correction. Panel b: raw long-cadence LC extracted by us with the Kepler GO/lightkurve code from the MAST TPF using the aperture assigned as BESTAPER in the vdb-LC. Panel c: vdb-correction for the long-cadence data created by subtracting panel b from panel a. Panel d: corrected long-cadence LC. Panel e: raw short-cadence LC extracted by us analogously to the long-cadence LC of panel b using the aperture assigned as BESTAPER in the vdb-LC. Panel f: vdb-correction for the short-cadence data created by subtracting panel b from panel a and interpolating to all cadences. Panel g: corrected short-cadence LC.