Massive characterisation of subgiants and red giants with TESS (Kepler and Gaia)
TESS serves as a formidable tool for investigating stellar variability. Nonetheless, the adaptation of methodologies employed in other space missions, such as Kepler, to deduce long stellar rotation periods or solar-like stellar pulsations has been a challenge. The advent of multiple sectors of data for most stars every two years with the extended
García, Rafael A. et al.
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2024