\begin{table}%t1
\caption{TeV blazar data.}\label{tab1}
\small%\centerline
 {
\begin{tabular}{ l l l l l l l l l l l }
\hline
\hline
Source  & ~~~~~~$z$  & ~~~~~~~~$\alpha_\gamma$ & ~~~~~~~~$F_\gamma$ & CT & ~~~$\alpha_\gamma^{\rm corr}$ & 
~~~~~~ $F_\gamma^{\rm corr}$ 
&  $F_{5~{\rm GHz}}$ & $~~~~~~$$F_{\rm x}$ & ~~$F_{x,0}$  & Notes \\
      (1) & ~~~~ (2)  & ~~~~~~~ (3) & ~~~~~~~~(4) & (5)& ~~~~(6) & ~~~~~~~~(7) & ~~(8) & ~~~~~~(9) & ~~(10) & ~(11) 
\\
\hline
Mrk~421       &  ~~~0.031 & $2.33 \pm 0.08$ & 1.03($\pm$0.03)E-10 & M & ~~~2.15 & ~~~7.59E-11 & 0.730 & ~~~4.0E-10 & 
4.1E-11 & Al+07a \\
Mrk~501       &  ~~~0.034 & $2.28 \pm 0.05$ & 1.71($\pm$0.11)E-11 & M & ~~~2.08 & ~~~1.32E-11 & 1.400 & ~~~4.0E-10 & 3.0E-11 & Al+07b \\
              &           & $2.45 \pm 0.07$ & 3.84($\pm$1.00)E-12 & M & ~~~2.25 & ~~~4.73E-12 &       & ~~~1.7E-10 &         &        \\
PKS~2344+514  &  ~~~0.044 & $2.95 \pm 0.12$ & 1.21($\pm$0.10)E-11 & M & ~~~2.67 & ~~~1.67E-11 & 0.231 & $<$7.0E-11 & 1.7E-11 & Al+07c \\
Mrk~180       &  ~~~0.045 & $3.30 \pm 0.70$ & 8.46($\pm$3.38)E-12 & M & ~~~3.01 & ~~~1.23E-11 & 0.274 & $<$1.0E-10 & 5.0E-12 & Al+06a \\
1ES~1959+650  &  ~~~0.047 & $2.72 \pm 0.14$ & 3.04($\pm$0.35)E-11 & M & ~~~2.41 & ~~~4.63E-11 & 0.253 & ~~~1.4E-10 & 1.4E-11 & Al+06b \\
BL~Lacertae   &  ~~~0.069 & $3.60 \pm 0.50$ & 3.28($\pm$0.26)E-12 & M & ~~~3.12 & ~~~7.15E-12 & 2.490 & ~~~~~~ --- & 5.8E-13 & Al+07d \\
PKS~2005-489  &  ~~~0.071 & $4.00 \pm 0.40$ & 3.32($\pm$0.48)E-12 & H & ~~~3.50 & ~~~7.47E-12 & 1.190 & ~~~4.0E-11 & 0.9E-11 & Ah+05a \\
              &           &                 &                     &   &         &             &       &            &         & P+99 \\
RGB~J0152+017 &  ~~~0.080 & $2.95 \pm 0.36$ & 4.43($\pm$1.24)E-12 & H & ~~~2.38 & ~~~1.15E-11 & 0.050 & ~~~2.7E-12 & 9.1E-13 & Ah+08 \\
              &           &                 &                     &   &         &             &       &            &         & D+01 \\
PKS~2155-304  &  ~~~0.116 & $3.37 \pm 0.07$ & 2.89($\pm$0.18)E-11 & H & ~~~2.51 & ~~~1.36E-10 & 0.310 & ~~~2.7E-11 & 2.0E-11 & Ah+05b \\
1ES~1426+428  &  ~~~0.129 & $3.55 \pm 0.46$ & 2.53($\pm$0.43)E-11 & W & ~~~2.54 & ~~~1.47E-10 & 0.038 & ~~~2.0E-11 & 1.6E-11 & Hor+02 \\
              &           &                 &                     &   &         &             &       &            &         & S+97 \\
1ES~0229+200  &  ~~~0.139 & $2.50 \pm 0.19$ & 4.46($\pm$0.71)E-12 & H & ~~~1.46 & ~~~3.04E-11 & 0.046 & ~~~1.5E-11 & 8.8E-12 & Ah+07c \\
              &           &                 &                     &   &         &             &       &            &         &P+96 \\ 
              &           &                 &                     &   &         &             &       &            &         & D+05 \\
H~2356-309    &  ~~~0.165 & $3.09 \pm 0.24$ & 2.55($\pm$0.68)E-12 & H & ~~~1.84 & ~~~2.66E-11 & 0.065 & ~~~1.0E-11 & 2.4E-11 & Ah+06a \\
              &           &                 &                     &   &         &             &       &            &         & W+84 \\
1ES~1218+304  &  ~~~0.182 & $3.00 \pm 0.40$ & 1.01($\pm$0.26)E-11 & M & ~~~1.61 & ~~~1.39E-10 & 0.056 & ~~~~~~ --- & 1.5E-11 & Al+06c \\
1ES~1101-232  &  ~~~0.186 & $2.94 \pm 0.20$ & 4.35($\pm$0.69)E-12 & H & ~~~1.46 & ~~~6.08E-11 & 0.066 & ~~~5.1E-11 & 2.5E-11 & Ah+07a \\
1ES~0347-121  &  ~~~0.188 & $3.10 \pm 0.23$ & 3.86($\pm$0.73)E-12 & H & ~~~1.67 & ~~~5.77E-11 & 0.008 &~~~2.8E-11  & 6.0E-12 & Ah+07b \\
1ES~1011+496  &  ~~~0.212 & $4.00 \pm 0.50$ & 6.40($\pm$0.32)E-12 & M & ~~~2.37 & ~~~1.43E-09 & 0.636 & ~~~~~~ --- & ~~~ --- & Al+07e \\
PG~1553+113   & $>$0.25   & $4.20 \pm 0.30$ & 5.24($\pm$0.87)E-12 & M & $<$2.28 & $>$2.18E-10 & 0.286 & ~~~5.0E-11 & 1.4E-11 & Al+07f \\
\hline
\end{tabular}}
\medskip
Column~1: source name. \\
Column~2: source redshift. \\
Column~3: observed 0.2$-$2~TeV photon spectral index, and associated statistical uncertainty. The 
corresponding systematic uncertainties are typically $\sim$0.1 for HESS and $\sim$0.2 for MAGIC. \\
Column~4: observed $>$0.2 TeV flux (in erg~cm$^{-2}$~s$^{-1}$), and associated statistical uncertainty (from observed spectral normalization only). \\
Column~5: Cherenkov telescope (CT) or array with which the data in Col.~3 have been collected: symbols stand for H~$=$ HESS, M~$=$ MAGIC, W~$=$ Whipple. \\
Column~6: corrected 0.2$-$2 TeV photon spectral index. \\
Column~7: corrected $>$0.2 TeV flux. \\
Column~8: 5 GHz flux density (in Jy): data are from the NED, except for 1ES~0347-121 (Fossati et~al. \cite{Foss98}) and H~2356-309 (Costamante \& Ghisellini \cite{Costa02}). \\
Column~9: 2$-$10 keV flux (in erg cm$^{-2}$ s$^{-1}$): the data come from the papers listed in Col.~11 or from references quoted therein; when necessary, fluxes have been converted from {\it R}XTE/ASM count rates using the conversion 1~ct/s~$=$ 3.33E$-$10~erg~cm$^{-2}$~s$^{-1}$. \\
Column~10: minimum 2$-$10 keV flux (in erg cm$^{-2}$ s$^{-1}$). \\
Column~11: Reference for VHE $\gamma$-ray data, and for the baseline X-ray flux when the latter was not taken from the NED~-- 
Al+07a: Albert et~al. (\cite{Albe07a});
Al+07b: Albert et~al. (\cite{Albe07b});
Al+07c: Albert et~al. (\cite{Albe07c});
Al+06a: Albert et~al. (\cite{Albe06a});
Al+06b: Albert et~al. (\cite{Albe06b});
Al+07d: Albert et~al. (\cite{Albe07d});
Ah+05a: Aharonian et~al. (\cite{Ahar05a}); P+99: Perlman et~al. (\cite{Perl99}); 
Ah+08:  Aharonian et~al. (\cite{Ahar08}); D+01: Donato et~al. (\cite{Dona01}); 
Ah+05b: Aharonian et~al. (\cite{Ahar05b});
Hor+02: Horan et~al. (\cite{Hora02}); S+97: Sambruna et~al. (\cite{Samb97}); 
Ah+07c: Aharonian et~al. (\cite{Ahar07c}); P+96: Perlman et~al. (\cite{Perl96}); D+05: Donato et~al. (\cite{Dona05});
Ah+06a: Aharonian et~al. (\cite{Ahar06a}); W+84: Wood et~al. (\cite{Wood84}); 
Al+06c: Albert et~al. (\cite{Albe06c});
Ah+07a: Aharonian et~al. (\cite{Ahar07a});
Ah+07b: Aharonian et~al. (\cite{Ahar07b});
Al+07e: Albert et~al. (\cite{Albe07e});
Al+07f: Albert et~al. (\cite{Albe07f}).
\end{table}