Figure 2 from Stellar Diameters and Temperatures. I. Main-sequence A, F, and G Stars

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Stellar Diameters and Temperatures. I. Main-sequence A, F, and G Stars

Authors: Tabetha S. Boyajian, Harold A. McAlister, Gerard van Belle, Douglas R. Gies, Theo A. ten Brummelaar, Kaspar von Braun, Chris Farrington, P. J. Goldfinger, David O'Brien, J. Robert Parks, Noel D. Richardson, Stephen Ridgway, Gail Schaefer, Laszlo Sturmann, Judit Sturmann, Yamina Touhami, Nils H. Turner, and Russel White

Boyajian et al. 2012 The Astrophysical Journal 746 101.

Provider: AAS Journals

Caption: Figure 2.

Top: plot showing the measured limb-darkened angular diameters vs. the SED angular diameters and the 1σ errors (black). Measurements for the 14 stars in common with this work are highlighted in color with red indicating a CHARA measurement presented in this paper and blue for a PTI measurement measured in van Belle & von Braun (2009). Bottom: plot showing the fractional difference between the SED and limb-darkened angular diameters. The dotted line shows an equal agreement of both measurements. See Section 3.2 and Tables 5 and 6 for details.

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