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A KELT–TESS Eclipsing Binary in a Young Triple System Associated with the Local “Stellar String” Theia 301

  • Authors: Joni-Marie C. Cunningham, Dax L. Feliz, Don M. Dixon, Joshua Pepper, Keivan G. Stassun, Robert J. Siverd, George Zhou, Daniel Bayliss, Thiam-Guan Tan, Phillip Cargile, David James, Rudolf B. Kuhn, and Marina Kounkel

2020 The Astronomical Journal 160 187.

  • Provider: AAS Journals

Caption: Figure 10.

Cross-correlation function for the spectrum taken on HJD 2456057.93945226, with the ANU 2.3 m echelle at R = 23,000. The CCF shown is the average CCF of the cross correlations from all echelle orders, excluding those with very low cross-correlation heights. The cross correlations are performed against RV standard star exposures taken on the same night. For clarity, the highest peak (presumed to correspond to higher mass, primary component in the eclipsing binary) has been shifted in this figure to be at 0 km s−1.

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