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.
Minimax-robust forecasting of sequences with periodically stationary long memory multiple seasonal increments
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abstract
We introduce stochastic sequences $\zeta(k)$ with periodically stationary generalized multiple increments of fractional order which combines cyclostationary, multi-seasonal, integrated and fractionally integrated patterns. We solve the problem of optimal estimation of linear functionals constructed from unobserved values of stochastic sequences $\zeta(k)$ based on their observations at points $ k<0$. For sequences with known spectral densities, we obtain formulas for calculating values of the mean square errors and the spectral characteristics of the optimal estimates of functionals. Formulas that determine the least favorable spectral densities and minimax (robust) spectral characteristics of the optimal linear estimates of functionals are proposed in the case where spectral densities of sequences are not exactly known while some sets of admissible spectral densities are given.
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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.