10.3.2 Properties of the input data

The input data consisted of pre-processed and cleaned photometric time series in the $G$, $G_{\mathrm{BP}}$, and $G_{\mathrm{RP}}$ bands (see Section 10.2.3) that had at least five FoV transits in the $G$ band and were selected by the General Variability Detection work package (see Section 10.2.3). Additional information on $G_{\mathrm{BP}}$ and $G_{\mathrm{RP}}$ spectral shape components (Section 5.1.1) was available to better characterize specific classes. General time series statistics and period search results, pre-computed in preceding stages as described in Sections 10.2.3 and 10.2.3, provided further classification attributes. Astrometric parameters were also employed in both training and validation stages.