TESS asteroseismology of the known planet host star λ<SUP>2</SUP> Fornacis
Context. The Transiting Exoplanet Survey Satellite (TESS) is observing bright known planet-host stars across almost the entire sky. These stars have been subject to extensive ground-based observations, providing a large number of radial velocity measurements. Aims: The objective of this work is to use the new TESS photometric observations to
Nielsen, M. B. et al.
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2020