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The Asteroseismic Target List for Solar-like Oscillators Observed in 2 minute Cadence with the Transiting Exoplanet Survey Satellite

  • Authors: Mathew Schofield, William J. Chaplin, Daniel Huber, Tiago L. Campante, Guy R. Davies, Andrea Miglio, Warrick H. Ball, Thierry Appourchaux, Sarbani Basu, Timothy R. Bedding, Jørgen Christensen-Dalsgaard, Orlagh Creevey, Rafael A. García, Rasmus Handberg, Steven D. Kawaler, Hans Kjeldsen, David W. Latham, Mikkel N. Lund, Travis S. Metcalfe, George R. Ricker, Aldo Serenelli, Victor Silva Aguirre, Dennis Stello, and Roland Vanderspek

2019 The Astrophysical Journal Supplement Series 241 12.

  • Provider: AAS Journals

Caption: Figure 11.

Predicted asteroseismic yield for the first year of TESS science operations (Cycle 1). Panel (a): radius vs. effective temperature for all expected TESS detections (blue) and the detections for dwarfs and subgiants by Kepler (red). The blue dashed line marks the approximate radius limit above that oscillations can be confidently detected using FFI light curves. Black lines show evolutionary tracks. Panel (b): approximate V magnitude distribution of the expected TESS yield (blue) and the Kepler yield (red).

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