Gaia Data Release 3: Pulsations in main sequence OBAF-type stars
Context. The third Gaia data release provides photometric time series covering 34 months for about 10 million stars. For many of those stars, a characterisation in Fourier space and their variability classification are also provided. This paper focuses on intermediate- to high-mass (IHM) main sequence pulsators (M'a ¥''1.3'M') of spectral types O, B, A, or F, known as β Cep, slowly pulsating B (SP
