Figure 1 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 1.

Comparison between effective temperatures from high-resolution spectroscopy (as listed in the PASTEL catalog) and the ATL photometric temperatures. The solid line shows the 1:1 relation. The horizontal lines of data points exist because the PASTEL catalog gives several effective temperatures for some stars. The residual median and scatter is 102 K and 146 K, respectively.

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