2016/10/20 by T. L. Campante, Tiago L. Campante · 1 citation
Physics and Astronomy · #Asteroseismology #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Gamma-ray bursts and supernovae #Physics #Planet #Sky #Stars #Stellar, planetary, and galactic studies #astro-ph.SR
paper · pdf · doi:10.1051/epjconf/201716001006
Submitted to EPJ Web of Conferences, to appear in the Proceedings of the joint TASC2/KASC9 workshop - SPACEINN & HELAS8 conference; 5 pages, 4 figures
arxiv created 2016/10/20 · openalex created_date 2016/10/28 · openalex publication_date 2017/01/01 · arxiv updated 2017/11/08 · openalex updated_date 2026/08/05
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.