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\section{Physical parameters of the RG/EBs}  \label{review}  \citet{gau16} and \citet{raw16} used JKTEBOP \citep{sou09} and the Eclipsing Light Curve (ELC) program \citep{oro00} to simultaneously fit a combination of light curves and radial velocity observations for at a  total of 17 RG/EBs. RG/EBs observed by \emph{Kepler}. \citet{fra13} did the same for KIC 8410637, which brings the total to 18.  For the 14 SB2  systems that have a radial velocity curve for both stars, this gives a full dynamic solution: orbital period $P_{orb}$, zeropoint, orbital inclination $i$, eccentricity and argument of periastron parameterized as  $e \sin \omega$, \omega$ and  $e \cos \omega$, component masses, component radii, and the effective  temperature ratio). ratio.  For the four SB1  systems that have a radial velocity curve for one star only, this allows the determination of SOME RATIOS BUT NOT ALL THE THINGS. XX of relative radii only and no component masses. Of  the XX systems 18 total systems, 14  have red giants that exhibit solar-like oscillations, which were analyzed in \citet{gau14,gau16} to derive global asteroseismic parameters. Also mention/review:  \begin{itemize}