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Direct measurements of stellar magnetic fields across the HR diagram in the TESS era
Long-term blind spectropolarimetric monitoring can be ineffective in obtaining the final result — establishing the magnitude and topology of a stellar magnetic field. The high quality photometric data from TESS makes it possible to search for periodicity at different time intervals. For those who perform direct magnetic field measurements, this provides a reliable base for deep studying the magnetic field across the HR diagram, including its variability associated with different phenomenadoi:10.5281/zenodo.5542019 fatcat:rvyvaypvurgo7lopf6izkiqr7y