Figure 8 from The Asteroseismic Target List for Solar-like Oscillators Observed in 2 minute Cadence with the Transiting Exoplanet Survey Satellite

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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 8.

Example of what is calculated in order to determine whether a star lies inside ϕ_range. In this example, the star’s longitude (represented by the orange line) lies outside of the satellite’s FOV, as marked by the red dashed lines (Equation (7)).

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