Figure 3 from A KELT–TESS Eclipsing Binary in a Young Triple System Associated with the Local “Stellar String” Theia 301

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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 3.

Phase-folded light curve of HD 54236A from KELT-South (black points) with the follow-up data from PEST overplotted (red points). Since the KELT-South data includes the flux from the unrelated high-proper-motion star HD 54262, the KELT-South data are multiplied by a factor of 3 to match the egress slope from the PEST data.

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