Notes. The first four columns describe the input sample and construction of subsamples. Columns 1 and 2: The name of the sample and the input samples for the search and the number of all targets in the catalog; Col. 3: number of oscillating targets within this sample that have a Gaia DR3 solution; Col. 4: number of targets in the magnitude limited sample within 4 ≤ G [mag] ≤ 13. The next 7 columns present the results of the search of the Non-Single-Star (NSS) catalog in Gaia DR3. Col. 5: gives the number of unique solutions returned by the ADQL query for the sample of oscillators with Gaia solutions (Col. 3); Col. 6: gives the number of alternative orbital solutions in case TBO contains multiple solutions; Col. 7: presents the binary detection fraction, calculated from the sample of all oscillating targets with a Gaia DR3 solution (Col. 3); Col. 8: presents the binary detection, calculated from the magnitude limited sample (Col. 4) and binaries within the magnitude limit; Col. 9: presents the number of systems hosting an oscillating component with inclination reported in TBO; Col. 10: number of sources with acceleration and non-linear solutions in TBO could point to longer-period binary systems. ^( ⋆ )Because the SB9 sample extends significantly further in period than the Gaia TBO sample, the magnitude limited sample for SB9 has been further corrected for a cut-off period of P ≤ 1100 days.