a sample of 109 EB candidates selected from the @Kirk2016 catalog, and listed in Table \[ebsampletable\]. We utilize both optical and NIR spectroscopy to solve these EBs as double-lined spectroscopic binaries (SB2s), and combine these results with [*Kepler*]{} photometry to derive masses and radii with precisions of better than 3% for most of the sample, and as good as 1% for a subset. Here we present two objects in our sample. Our complete sample is restricted to EBs that are classified as fully detached and have $H<13$. Orbital periods range from a few days to more than one hundred days. The total sample size is comparable in number to the $M<2{\ensuremath{\mathit{\,M_\odot}}}$ members in and DEBCat (110 and 285 EBs, respectively), but we have included many EBs with low-mass primary or secondary components in order to substantially increase the population of well measured low-mass stars. One of the reasons the compilation from is so useful to the astronomical community is that their study homogenously re-computed orbital and stellar parameters from the compiled list of literature EBs. Our survey will intrinsically possess this quality, as our analysis applies a singular set of tools to a homogeneous data set.

In §2 we describe 