Host star and system parameters of the two evaporating exoplanet candidates.
|M⋆ [M⊙]||0.546 ± 0.044||H14|
|Pp [days]||0.6535538(1)||0.910022(5)||V14, R14|
Notes. From top to bottom: stellar effective temperature, stellar mass, stellar radius, stellar luminosity (derived from Teff,⋆ and R⋆), orbital period of the candidate planet, and corresponding semi-major axis (as given by Kepler’s third law). Numbers in brackets indicate the uncertainty on the last digit.
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