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 CCD,
FoV, and ), for faint sources, with sufficient number of transits in the
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.