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We have performed a new search for DPVs of short period in the ASAS catalog(Pojmanski, G., 1997), focusing on those stars with orbital periods between 2to 3 days which also show variations in their brightness. From a total of 244objects, we have found another candidate to DPV, one whose mean brightness isgradually decreasing. By fitting a 3rd order polynomial to the mean magnitudeand then moving it to zero for a second analysis, a gradual decrease over 2500days was revealed. During the last 1000 days of this decrease, a 42% increasein the variation between the minimum and maximum values of the magnitude wasobserved. We determined the orbital period by using the PDM IRAF software(Stellingwerf 1978) and estimated the errors for the orbital period and longcycle by visual inspection of the light curves phased with trial periods nearthe minimum of the periodogram given by PDM.

TYC 5353-1137-1: an enigmatic Double Periodic Variable of semiregular amplitude