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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 7.

FOV from one of the ecliptic poles. The color bar represents how long a part of the sky will be observed by TESS. The dotted circles are lines of constant latitude (0°, 30°, and 60°). The center of the image has a latitude of 90°. The outer dotted circle at 0° latitude has labels for 0° and 180° longitude. The horizontal dotted line represents longitude values of 0° and 180°.

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