Model dynamic spectra for an exoplanet-induced stellar emission. Abscissa is given in exoplanet’s years (i.e. orbital phase of the exoplanet) and stellar rotation (“* Rot”). In polarization dynamic spectra, black stands for northern emissions, white for southern emissions. a), b) Intensity and polarization dynamic spectra for an axisymmetric stellar magnetic field and 0° inclination (i.e. observer along the orbital plane). c), d) Intensity and polarization dynamic spectra for an axisymmetric stellar magnetic field and 15° inclination (i.e. observer’s direction 15° north of the orbital plane). e), f) Intensity and polarization dynamic spectra for a stellar magnetic field tilted by 15° relative to the rotation axis (perpendicular to the orbital plane) and 0° inclination. g), h) Intensity and polarization dynamic spectra for a stellar magnetic field tilted by 15° and 15° inclination.