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We present the discovery of 1847 Mira candidates in the Local Group galaxyM33 using a novel semi-parametric periodogram technique coupled with a RandomForest classifier. The algorithms were applied to ~2.4x10^5 I-band light curvespreviously obtained by the M33 Synoptic Stellar Survey. We derive preliminaryPeriod-Luminosity relations at optical, near- & mid-infrared wavelengths andcompare them to the corresponding relations in the Large Magellanic Cloud.

The M33 Synoptic Stellar Survey. II. Mira Variables