Using a new but partly hand-tuned scaling relation, the authors predict that an extended TESS mission will detect activity-related p-mode frequency shifts in hundreds of main-sequence and early subgiant stars and thousands of evolved subgiant and red-giant stars.
Looking for activity cycles in late-type Kepler stars using time-frequency analysis
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Seismic Signatures of Stellar Magnetic Activity -- What Can We Expect from TESS?
Using a new but partly hand-tuned scaling relation, the authors predict that an extended TESS mission will detect activity-related p-mode frequency shifts in hundreds of main-sequence and early subgiant stars and thousands of evolved subgiant and red-giant stars.