\begin{table}%t2
\caption{Comparison of $t_{\rm e}$(O~{\sc iii})$^a$ and $t_{\rm e}$(H$^+$)$^b$ for the sample galaxies.}\label{te}
%\centering
\small
\begin{tabular}{llcccc} 
\hline\hline
Galaxy          & {\it EW}(H$\beta$) & $t_{\rm e}$(O {\sc iii}) 
& $t_{\rm e}$(H$^+$) & 12 + log O/H 
& $C$(H$\beta$)$^c$ \\ 
\hline
SBS 0335-052E SE  & 382. & 1.98 $\pm$ 0.05 & 1.90 $\pm$ 0.10&  7.28 &  0.00   \\  
Pox 186           & 358. & 1.67 $\pm$ 0.02 & 2.00 $\pm$ 0.07&  7.75 &  0.08   \\  
HS 2236+1344a     & 343. & 2.05 $\pm$ 0.02 & 1.96 $\pm$ 0.06&  7.49 &  0.14   \\  
UM 461a           & 335. & 1.66 $\pm$ 0.02 & 1.77 $\pm$ 0.32&  7.76 &  0.22   \\  
J 104457.80+035313.1a      & 318. & 1.96 $\pm$ 0.02 & 1.91 $\pm$ 0.08&  7.44 &  0.31   \\  
Tol 1214-277      & 314. & 2.04 $\pm$ 0.03 & 1.92 $\pm$ 0.06&  7.50 &  0.14   \\  
UM 570            & 310. & 1.83 $\pm$ 0.02 & 1.83 $\pm$ 0.13&  7.72 &  0.14   \\  
CGCG 032-017       & 308. & 1.38 $\pm$ 0.01 & 1.48 $\pm$ 0.21&  8.09 &  0.27   \\ 
Pox 108           & 306. & 1.31 $\pm$ 0.02 & 1.31 $\pm$ 0.17&  8.11 &  0.08   \\  
UM 559            & 306. & 1.60 $\pm$ 0.02 & 1.55 $\pm$ 0.12&  7.72 &  0.06   \\    
SBS 0335-052E \#7  & 299. & 1.97 $\pm$ 0.06 & 1.91 $\pm$ 0.06&  7.21 &  0.14    \\ 
UM 442            & 289. & 1.30 $\pm$ 0.01 & 1.29 $\pm$ 0.09&  8.10 &  0.14    \\ 
Mrk 1329          & 288. & 1.05 $\pm$ 0.01 & 1.26 $\pm$ 0.06&  8.33 &  0.03   \\  
Mrk 1236a         & 283. & 1.21 $\pm$ 0.01 & 1.30 $\pm$ 0.08&  8.17 &  0.14   \\  
Tol 2146-391      & 277. & 1.63 $\pm$ 0.02 & 1.59 $\pm$ 0.32&  7.78 &  0.18   \\ 
CGCG 007-025a      & 274. & 1.58 $\pm$ 0.02 & 1.83 $\pm$ 0.27&  7.81 &  0.20   \\  
HS 2134+0400      & 262. & 2.02 $\pm$ 0.04 & 1.86 $\pm$ 0.20&  7.41 &  0.25    \\ 
J 001434.98-004352.0       & 260. & 1.39 $\pm$ 0.04 & 1.31 $\pm$ 0.28&  7.97 &  0.12    \\ 
J 232420.34-000625.0       & 249. & 1.41 $\pm$ 0.01 & 1.55 $\pm$ 0.22&  7.95 &  0.20   \\  
SBS 0335-052E \#3b    & 249. & 2.04 $\pm$ 0.03 & 2.07 $\pm$ 0.22&  7.31 &  0.45   \\  
J 125305.96-031258.9       & 248. & 1.38 $\pm$ 0.01 & 1.34 $\pm$ 0.21&  8.01 &  0.36   \\  
J 120122.30+021108.3       & 248. & 1.81 $\pm$ 0.03 & 1.70 $\pm$ 0.27&  7.49 &  0.09   \\  
SBS 0335-052E \#3a    & 246. & 2.02 $\pm$ 0.03 & 2.05 $\pm$ 0.22&  7.31 &  0.43   \\  
Tol 65a           & 244. & 1.76 $\pm$ 0.02 & 1.83 $\pm$ 0.17&  7.54 &  0.10   \\  
UM311             & 243. & 0.99 $\pm$ 0.01 & 1.00 $\pm$ 0.04&  8.36 &  0.22   \\  
J 130432.27-033322.1       & 233. & 1.08 $\pm$ 0.01 & 1.20 $\pm$ 0.08&  8.24 &  0.12   \\  
J 024815.95-081716.5a      & 233. & 1.32 $\pm$ 0.01 & 1.13 $\pm$ 0.19&  8.04 &  0.04   \\  
Pox 4a            & 220. & 1.39 $\pm$ 0.01 & 1.11 $\pm$ 0.23&  8.01 &  0.08   \\  
Pox 120a          & 215. & 1.53 $\pm$ 0.01 & 1.76 $\pm$ 0.22&  7.88 &  0.21   \\  
HS 2236+1344b     & 215. & 1.86 $\pm$ 0.02 & 1.80 $\pm$ 0.10&  7.58 &  0.22    \\ 
CGCG 007-025c      & 214. & 1.56 $\pm$ 0.02 & 1.49 $\pm$ 0.25&  7.78 &  0.02    \\ 
UM 462a           & 212. & 1.39 $\pm$ 0.01 & 1.45 $\pm$ 0.22&  8.00 &  0.52   \\  
J 230210.00+004938.8       & 212. & 1.80 $\pm$ 0.03 & 1.91 $\pm$ 0.09&  7.63 &  0.00   \\  
Tol 2138-405      & 208. & 1.39 $\pm$ 0.02 & 1.08 $\pm$ 0.12&  7.99 &  0.39   \\  
J 210455.31-003522.2N       & 203. & 2.01 $\pm$ 0.08 & 1.87 $\pm$ 0.18&  7.26 &  0.00   \\  
J 011340.44+005239.1       & 193. & 2.29 $\pm$ 0.30 & 2.55 $\pm$ 0.04&  7.17 &  0.00   \\  
J 013352.56+134209.3       & 178. & 1.74 $\pm$ 0.02 & 1.62 $\pm$ 0.33&  7.56 &  0.04   \\  
Pox 4b            & 177. & 1.43 $\pm$ 0.01 & 1.51 $\pm$ 0.18&  7.87 &  0.00   \\  
IC 4662a          & 172. & 1.27 $\pm$ 0.01 & 1.34 $\pm$ 0.19&  8.09 &  0.44   \\  
J 143053.50+002746.3       & 168. & 1.30 $\pm$ 0.01 & 1.21 $\pm$ 0.15&  8.07 &  0.15   \\  
IC 4662c          & 166. & 1.25 $\pm$ 0.01 & 1.25 $\pm$ 0.14&  8.16 &  0.33   \\  
Pox 120b          & 158. & 1.37 $\pm$ 0.02 & 1.18 $\pm$ 0.20&  7.99 &  0.14   \\  
g2252292-171050   & 158. & 1.59 $\pm$ 0.02 & 1.74 $\pm$ 0.24&  7.82 &  0.10    \\ 
UM 461b           & 147. & 1.58 $\pm$ 0.02 & 1.79 $\pm$ 0.23&  7.77 &  0.18   \\  
Mrk 1236c         & 147. & 1.22 $\pm$ 0.04 & 0.98 $\pm$ 0.03&  8.05 &  0.00   \\  
J 144805.36-011057.7       & 146. & 1.39 $\pm$ 0.01 & 1.44 $\pm$ 0.24&  8.00 &  0.21   \\  
IC 4662b          & 140. & 1.27 $\pm$ 0.01 & 1.32 $\pm$ 0.07&  8.10 &  0.14   \\  
J 223036.79-000636.9       & 133. & 1.71 $\pm$ 0.03 & 1.86 $\pm$ 0.30&  7.64 &  0.34   \\  
Pox 105           & 131. & 1.53 $\pm$ 0.02 & 1.49 $\pm$ 0.27&  7.85 &  0.04   \\  
UM 462d           & 130. & 1.45 $\pm$ 0.03 & 1.52 $\pm$ 0.26&  7.86 &  0.23   \\  
UM 462c           & 127. & 1.48 $\pm$ 0.02 & 1.11 $\pm$ 0.15&  7.88 &  0.00   \\  
J 024815.95-081716.5b      & 125. & 1.35 $\pm$ 0.04 & 1.36 $\pm$ 0.18&  7.99 &  0.00   \\  
CGCG 007-025b      & 122. & 1.58 $\pm$ 0.02 & 1.67 $\pm$ 0.19&  7.75 &  0.06    \\ 
J 162410.12-002202.5       & 122. & 1.20 $\pm$ 0.01 & 1.21 $\pm$ 0.15&  8.16 &  0.16   \\ 
UM 462e           & 112. & 1.59 $\pm$ 0.05 & 1.67 $\pm$ 0.26&  7.77 &  0.00   \\  
J 013452.00-003854.4       & 111. & 1.49 $\pm$ 0.15 & 1.53 $\pm$ 0.26&  7.85 &  0.16   \\  
SBS 0335-052W     & 109. & 1.97 $\pm$ 0.25 & 2.01 $\pm$ 0.25&  7.13 &  0.02   \\  
Tol 65b           &  96. & 1.69 $\pm$ 0.04 & 1.74 $\pm$ 0.31&  7.59 &  0.14   \\  
SBS 0335-052E \#4,5    &  89. & 2.11 $\pm$ 0.04 & 1.90 $\pm$ 0.13&  7.27 &  0.26   \\  
\hline
UM 462b           &  85. & 1.42 $\pm$ 0.02 & 1.44 $\pm$ 0.15&  7.92 &  0.21   \\  
CGCG 007-025d      &  69. & 1.68 $\pm$ 0.04 & 1.72 $\pm$ 0.27&  7.65 &  0.00   \\  
ESO 338-IG04      &  59. & 1.46 $\pm$ 0.02 & 1.44 $\pm$ 0.27&  7.90 &  0.02   \\  
Mrk 1236b         &  56. & 1.17 $\pm$ 0.02 & 1.14 $\pm$ 0.22&  8.12 &  0.07    \\ 
J 141454.13-020822.9       &  48. & 1.89 $\pm$ 0.01 & 1.98 $\pm$ 0.23&  7.32 &  0.08    \\ 
IC 4662d          &  44. & 1.25 $\pm$ 0.02 & 1.12 $\pm$ 0.28&  8.07 &  0.14    \\ 
J 010746.56+010352.0       &  40. & 1.56 $\pm$ 0.23 & 1.57 $\pm$ 0.25&  7.68 &  0.12    \\ 
g0405204-364859   &  23. & 2.08 $\pm$ 0.25 & 1.95 $\pm$ 0.21&  7.34 &  0.02    \\ 
J 104457.80+035313.1b      &  20. & 1.94 $\pm$ 0.21 & 1.81 $\pm$ 0.32&  7.45 &  0.14    \\ 
IC 4662e          &  10. & 1.31 $\pm$ 0.01 & 1.30 $\pm$ 0.23&  8.08 &  0.06    \\ 
\hline 
\end{tabular}
\parbox{13cm}{
$^a$ $t_{\rm e}$(O {\sc iii}) = $T_{\rm e}$(O {\sc iii})/10~000~K, derived from the [O~{\sc iii}] $\lambda$(4959+5007)/$\lambda$4363 emission line ratio. \\
$^b$ $t_{\rm e}$(H$^+$) = $T_{\rm e}$(H$^+$)/10~000, derived as the 
weighted mean temperature from the 10~best fits of the SED. \\
$^c$ Extinction coefficient is derived from observed hydrogen Balmer decrement.}
%\end{center}
\end{table}