(ASPCAP[^11], García Pérez et al. 2014, in preparation) for Fe, C and N.

-3.5cm

[@lcccccccccc@]{} & & &\
(r)[2-5]{} (r)[6-8]{} (r)[9-11]{} Star & [^12] & $\log(g)$ & $v_t$ &$\mathrm{T}_{\mathrm{eff}}$& $\log(g)$ & $v_t$ &$\mathrm{T}_{\mathrm{eff}}$& $\log(g)$ & $v_t$\
& &Spect.& ($\pm$0.2 dex)& ($\pm$0.2 km s$^{-1}$)& ($\pm$75 K)& ($\pm$0.2 dex)& ($^{+0.4}_{-0.2}$km s$^{-1}$)& (K) & dex) & (km s$^{-1}$)\
NGC 5024-22254 &4511&4410 &1.21 &1.60 &- &- &- &4409 &1.37 &1.83\
NGC 5024-50371 &4444&4425 &1.06 &1.80 &- &- &- &4391 &1.26 &1.86\
NGC 5466-9951 &4595&4600 &1.44 &1.55 &- &- &- &4512 &1.75 &1.71\
NGC 5466-1344 &4512&4499 &1.27 &1.40 &- &- &- &4469 &1.62 &1.75\
NGC 5466-10186 &4571&4585 &1.29 &1.75 &- &- &- &- &- &-\
M3-C41303-2217 &4379&4538 &1.19 &1.55 &4436 &1.20 &1.60 &4319 &1.69 &1.73\
M13-III-18 &4298&4397 &1.02 &1.75 &4350 &1.00 &1.65 &4498 &2.25 &1.56\
\
\[table:inputParam\]

Stellar Parameter Uncertainties {#sec:teff}
-------------------------------

The uncertainties in $\mathrm{T}_{\mathrm{eff}}$ were found by assuming the derived individual [Fe$\;$[Roman[1]{}]{}]{} line abundances are distributed randomly about the mean; thus the standard deviation ($\sigma_{\mathrm{Fe}}$) in the mean abundance measures the scatter in the data. If $\mathrm{T}_{\mathrm{eff}}$ is adjusted such that the slope of the log(Fe) vs $\chi$ spans $\pm 1 \sigma$ over the range in excitation potentials ($\chi$), then $\Delta\mathrm{T}_{\mathrm{eff}}$ is found 