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Strong variations of any kind and causes within a stellar light curve mayprohibit the detection of transits, particularly of faint or shallow transitscaused by small planets passing in front of the stellar disk. The success offuture space telescopes with the goal for finding small planets will be basedon proper filtering, analysis and detection of transits in perturbed stellarlight curves. The wavelet-based filter methods VARLET and PHALET, developed byRIU-PF, in combination with the transit detection software package EXOTRANSallow the extraction of (i) strong stellar variations, (ii) instrument causedspikes and singularities within a stellar light curve, (iii) already detectedplanetary or stellar binary transits in order to be able to search for furtherplanets or planets about binary stars. Once the light curve is filtered,EXOTRANS is able to search efficiently, effectively and precisely for transits,in particular for faint transits.

Wavelet-based filter methods to detect small transiting planets in stellar light curves