T. L. Campante
Abstract
The upcoming NASA TESS mission will perform an all-sky survey for planets transiting bright nearby stars. In addition, its excellent photometric precision will enable asteroseismology of solar-type and red-giant stars. We apply a newly developed detection test along a sequence of stellar evolutionary tracks in order to predict the detectability of solar-like oscillations with TESS.
Keywords
Astrophysics - Solar and Stellar Astrophysics
Seismology of the Sun and the Distant Stars 2016 – Using Today’s Successes to Prepare the Future – TASC2 & KASC9 Workshop – SPACEINN & HELAS8 Conference
M.J.P.F.G. Monteiro, M.S. Cunha, J.M.T.S. Ferreira
EPJ Web of Conferences
Volume 160, Number 0100
2017 October
