Tiago L. Campante
Published 2016-10-20Version 1
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.
Comments: Submitted to EPJ Web of Conferences, to appear in the Proceedings of the joint TASC2/KASC9 workshop - SPACEINN & HELAS8 conference; 5 pages, 4 figures
Solar-Like Oscillations: Lessons Learned & First Results from TESS
Period-luminosity relations in evolved red giants explained by solar-like oscillations
FRA -- A new Fast, Robust and Automated pipeline for the detection and measurement of solar-like oscillations in time-series photometry of red-giant stars
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