We report the confirmation of a sub-Saturn-size exoplanet, TOI-1194 b, with a mass of about RJ and the amplitude of the RV curve is
m s−1. TOI-1251 B is confirmed based on the multiband photometric and high-resolution spectroscopic data, whose orbital period is
days, radius is
RJ and amplitude of the RV curve is
m s−1.
Key words: planets and satellites: fundamental parameters – planets and satellites: gaseous planets – stars: fundamental parameters – stars: low-mass – methods: data analysis – techniques: photometric
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