IPD parameter IPDgofha versus the mean G-band magnitude for our Galactic targets (large colour dots and circles) and stars located within 2 arcmins from them. Top: diagram colour-coded by the ratio G mean flux to its standard error (RFG). Bottom: our targets of interest are colour-coded by their faintest G-band magnitude as observed in their respective light curves. The targets with and without a published Gaia DR3 light curve are also indicated.