Figure 2 from Two “b”s in the Beehive: The Discovery of the First Hot Jupiters in an Open Cluster

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Two “b”s in the Beehive: The Discovery of the First Hot Jupiters in an Open Cluster

Authors: Samuel N. Quinn, Russel J. White, David W. Latham, Lars A. Buchhave, Justin R. Cantrell, Scott E. Dahm, Gabor Fűrész, Andrew H. Szentgyorgyi, John C. Geary, Guillermo Torres, Allyson Bieryla, Perry Berlind, Michael C. Calkins, Gilbert A. Esquerdo, and Robert P. Stefanik

Quinn et al. 2012 The Astrophysical Journal Letters 756 L33.

Provider: AAS Journals

Caption: Figure 2.

Orbital solutions for Pr0211 (left) and Pr0201 (right). The panels, from top to bottom, show the relative RVs, best-fit residuals, bisector span variations, and relative S index values. RV error bars represent the internal errors, and do not include astrophysical jitter, although 13 m s ⁻¹ jitter was assumed in the orbital fit. The solid curve shows the best-fit orbital solution. The orbital parameters are listed in Table 3.

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