Recovery fraction of 152 transit injections into the β Pictoris dataset. Exoplanet signals with a S/N > 3.0 above other nights are considered recovered. We assume an impact parameter b = 0. The radii of Jupiter, Saturn and Neptune are indicated by the white dashed lines. As v_eq = 130 km s⁻¹, radial velocities outside of our range are (close-to) zero. Companions with radii R = R_Jup are almost fully recovered and a large fraction with radii R = R_Sat are recovered. The effects of stellar pulsation are seen by the fluctuations of the recovery fraction as a function of radial velocity.