An ensemble stacking method is proposed to detect composite oscillation power envelopes in K-dwarfs by averaging spectra from many similar stars observed by PLATO.
Predicting the detectability of oscillations in solar-type stars observed by Kepler
2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
abstract
Asteroseismology of solar-type stars has an important part to play in the exoplanet program of the NASA Kepler Mission. Precise and accurate inferences on the stellar properties that are made possible by the seismic data allow very tight constraints to be placed on the exoplanetary systems. Here, we outline how to make an estimate of the detectability of solar-like oscillations in any given Kepler target, using rough estimates of the temperature and radius, and the Kepler apparent magnitude.
fields
astro-ph.SR 2representative citing papers
This review summarizes the development, techniques, and open questions in asteroseismology of solar-type stars whose oscillations are stochastically excited by surface convection.
citing papers explorer
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Ensemble asteroseismology: An ensemble approach to detecting signatures of solar-like oscillations in K-dwarfs
An ensemble stacking method is proposed to detect composite oscillation power envelopes in K-dwarfs by averaging spectra from many similar stars observed by PLATO.
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Asteroseismology of solar-type stars
This review summarizes the development, techniques, and open questions in asteroseismology of solar-type stars whose oscillations are stochastically excited by surface convection.