PIMMS extends ZDI by adding a pulsation velocity map to reconstruct surface brightness, magnetic field, and velocity from spectropolarimetric data, with numerical tests showing accurate recovery on simulated pulsating hot stars.
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PIMMS: Pulsation-Informed Magnetic Mapping of Stars with Zeeman-Doppler Imaging I. Formalism and numerical tests
PIMMS extends ZDI by adding a pulsation velocity map to reconstruct surface brightness, magnetic field, and velocity from spectropolarimetric data, with numerical tests showing accurate recovery on simulated pulsating hot stars.