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Meredith L. Rawls edited subsection_A_hint_of_a__.tex
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\subsection{A hint of a second set of oscillations}
\label{subsec_second_osc}
Given that the giants in KIC 9246715 are nearly twins, we test whether it is possible that we see only one set of oscillation modes because both stars are oscillating with virtually identical frequencies. \newrevise{The predicted $\nu_{\rm{max}}$
values for these} not-quite-identical stars are
%$115.47 \pm 4.46$ and $102.9 \pm 3.46 \ \mu\rm{Hz}$
$103.4\substack{+1.6 \\ -1.1}$ and $104.1\substack{+1.1 \\ -1.2} \ \mu\rm{Hz}$
for Star 1 and Star 2, respectively (from an inversion of Equations \ref{density} and \ref{gravity}), and the predicted $\Delta\nu_{\rm{obs}}$ are