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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 4.

Example of SED fit for HD 142860. The (red) pluses indicate flux-calibrated photometry from the literature with corresponding errors ( y-direction) and bandwidth of the filter ( x-direction). The (black) crosses show the flux value of the spectral template integrated over the filter transmission for each point. The spectral template is plotted by a blue line. The lower panel shows the residuals. See Section 4 for details.

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