  Detailed chemical abundances for five stars in two Galactic globular
clusters, NGC 5466 and NGC 5024, are presented from high resolution optical
(from the Hobby- Eberley Telescope) and infrared spectra (from the SDSS-III
APOGEE survey). We find [Fe/H] = -1.97 +/- 0.13 dex for NGC 5466, and [Fe/H] =
-2.06 +/- 0.13 dex for NGC 5024, and the typical abundance pattern for globular
clusters for the remaining elements, e.g., both show evidence for mixing in
their light element abundance ratios (C, N), and AGB contributions in their
heavy element abundances (Y, Ba, and Eu). These clusters were selected to
examine chemical trends that may correlate them with the Sgr dwarf galaxy
remnant, but at these low metallicities no obvious differences from the
Galactic abundance pattern are found. Regardless, we compare our results from
the optical and infrared analyses to find that oxygen and silicon abundances
determined from the infrared spectral lines are in better agreement with the
other alpha-element ratios and with smaller random errors.
