The short-timescale SOS work package aims to produce a list of suspected periodic
short-timescale candidates with periods between a few tens of minutes to one day.
This candidate list results from the analysis of Gaia time series (in $G$ CCD,
$G$ FoV, ${G}_{\mathrm{BP}}$ and ${G}_{\mathrm{RP}}$), for faint sources, with sufficient number of transits in the
$G$ band, and for which per-CCD time series showed a significant degree of
variability at the transit level and for the majority of the transits of the source.