We have analysed photometric data from a sample of pulsating stars observed by the Transiting Exoplanet Survey Satellite. By applying Fourier and prewhitening techniques, we extracted the significant frequencies for each star. We investigated the presence of rotationally split multiplets and evaluated frequency spacings using the Kolmogorov–Smirnov test. These analyses allow us to estimate stellar parameters such as the large frequency spacing, which in turn provides insights into the stellar mean densities. However, identifying clear multiplets and frequency spacings in ${\unicode{x03B4}}$ Scuti stars remains challenging due to the complexity of their oscillation spectra. Our rotationally-split mode findings are yet to be confirmed, while the K–S test revealed no convincing large frequency spacings that could be used toward mass estimation. We derived orbital periods for stars we identified to be in binary systems. We provide spectral type classifications to confirm the ${\unicode{x03B4}}$ Sct and/or ${\unicode{x03B3}}$ Dor nature of the stars we found. Out of 43 stars presented in this paper, 18 are identified as ${\unicode{x03B4}}$ Sct/${\unicode{x03B3}}$ Dor hybrids (including five candidates), 20 as ${\unicode{x03B4}}$ Sct stars, one as a ${\unicode{x03B3}}$ Dor star and four as binary systems without any signature of pulsation.