  We report the results of a search for candidate Li-rich giants among 569,738
stars of the SDSS DR10 dataset. With small variations, our approach is based on
that taken in an earlier search for EMP/CEMP stars and uses the same dataset.
As part of our investigation, we demonstrate a method for separating post-main
sequence and main sequence stars cooler than Teff ~ 5800 K using our feature
strength measures of the Sr II 4078, Fe I 4072, and Ca I 4227 lines. By taking
carefully selected cuts in a multi-dimensional phase space, we isolate a sample
of potential Li-rich giant stars. From these, using detailed comparison with
dwarf and giant MILES stars, and our own individual spectral classifications,
we identify a set of high likelihood candidate Li-rich giant stars. We offer
these for further study to promote an understanding of these enigmatic objects.
