Notes. Each entry describes one star. We chose to include three identifiers to facilitate cross-identification: the TIC identifier, the Gaia DRЗ identifier, and an alternative identifier, most commonly the HD ID. The next 5 columns describe key stellar parameters: effective temperatւưe, surface gravity, luminosity, and associated uncertainty, the apparent magnitude in V band. The uncertainties for effective temperature and sւưface gravity are not included since these are fixed to 110 K and 0.2 dex (see Section 2.2). Next, 4 columns summarise the results obtained from our frequency analysis: the variability class if pulsations were detected, the range of frequencies excited for g and p modes, if applicable, and the number of excited radial orders identified. The variability classes are DS for δ Scuti, GD for γ Doradus, HY for hybrids, EB for eclipsing binaries, and OV for other variability. Lastly, information is provided on the potential binary nature of the system, the number of TESS sectors used for the analysis and whether the star is ap Puppis. The full table is available at the CDS.