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We present a simple phenomenological method for detrending of raw Kepler andMOST photometry, which is illustrated by means of photometric data processingof two periodically variable chemically peculiar stars, KIC 6950556 and HD37633. In principle, this method may be applied to any type of periodicallyvariable objects and satellite or ground based photometries. As a by product,we have identified KIC 6950556 as a magnetic chemically peculiar star with anACV type variability.

Fine detrending of raw Kepler and MOST photometric data of KIC 6950556 and HD 37633