Two standard stars were also observed, RGB stars with previously published spectral analyses in each of the globular clusters M3 and M13. The signal to noise (S/N) for these seven targets ranged from 40 - (see Table \[table:obs\]).

IR spectra for four of the five targets in NGC 5466 and NGC 5024 are available in the APOGEE DR10 release[^4]. APOGEE H-band spectra, ranging from 15000-17000Å at a resolution R $\sim$ 20,000 with S/N $\ge$ 100. These spectra expand analysis of our main science targets to features at longer wavelengths. We have not analysed the APOGEE spectra of our M3 and M13 standard stars since there are no published results of their infrared spectral features for a comparison.

-3.0cm

  ---------------- -------------- -------------- ------------ ------------------- --------- ---------- --------------------
                                                                                   Red S/N   Blue S/N  
  Star              R.A. (J2000)   Dec. (J2000)     Date Obs.  Exp. Time (s)[^5]   @6250Å     @5500Å      $V_{hel.}$ (km/s)
  NGC 5024-22254    13 12 47.94    +18 06 32.1       May 2005       2700(1)          50         40        -57.57 $\pm$ 0.50
  NGC 5024-50371    13 13 17.36    +18 14 46.4     March 2007       3387(1)          75         55        -62.69 $\pm$ 0.24
  NGC 5466-9951     14 05 41.08    +28 29 48.2      June 2005       6350(2)          60         55        126.53 $\pm$ 1.10
  NGC 5466-1344     14 05 20.73    +28 29 42.0      