\begin{table}%t1
\caption{\label{tab:pos_coincidence1}0FGL sources and LAT pulsars with spatially coincident VHE counterpart.}
%\centering
\par
%\renewcommand{\footnoterule}{}  
\begin{tabular}{cccccccccccc}
\hline\hline\noalign{\smallskip}
     LAT source        & Association\tablefootmark{a} & Class\tablefootmark{b} & $l$ & $b$ & Error\tablefootmark{c} & VHE $\gamma$-ray source & Association\tablefootmark{d} & $l$ & $b$ & Extension\tablefootmark{e} & References \\
               &  & & ($\degr$) & ($\degr$) & ($\degr$) & & & ($\degr$) & ($\degr$) & ($\degr$) & \\
    \hline
    \object{0FGL~J0534.6$+$2201} & Crab    & PSR & 184.56 & $-$5.76 & 0.05 & \object{HESS~J0534$+$220} & Crab nebula & 184.56 & $-$5.78 & PS & 1 \\
    \object{0FGL~J0835.4$-$4510} & Vela    & PSR & 263.56 & $-$2.77 & 0.04 & \object{HESS~J0835$-$455} & Vela~X & 263.86 & $-$3.09 & 0.43 & 2 \\
    \object{0FGL~J1418.8$-$6058} &         & PSR & 313.34 & 0.11 & 0.07 & \object{HESS~J1418$-$609} & \object{G313.3$+$0.1} (Rabbit) & 313.25 & 0.15 & 0.06 & 3 \\
    \object{PSR~J1420$-$6048}    &         & PSR & 313.5 & 0.2 & PS & \object{HESS~J1420$-$607} & \object{PSR~J1420$-$6048} & 313.56 & 0.27 & 0.07 & 3 \\
    \object{0FGL~J1709.7$-$4428} & \object{PSR~B1706$-$44} & PSR & 343.11 & $-$2.68 & 0.05 & \object{HESS~J1708$-$443}\tablefootmark{f} & \object{PSR~B1706$-$44}? & 343.04 & $-$2.38 & 0.29 & 4 \\
    \object{PSR~J1718$-$3825}    &         & PSR & 349.0 & $-$0.4 & PS & \object{HESS~J1718-385} & & 348.83 & $-$0.49 & 0.015 & 5 \\
    \object{0FGL~J1907.5$+$0602} &         & PSR & 40.14 & $-$0.82 & 0.08 & \object{HESS~J1908$+$063} & & 40.39 & $-$0.79 & 0.34 & 6 \\
    \object{0FGL~J2032.2$+$4122} &         & PSR & 80.16 & 0.98 & 0.09 & \object{TeV~J2032$+$4130} & & 80.23 & 1.10 & 0.10 & 7 \\
    \object{0FGL~J0617.4$+$2234} &         & SNR/PWN & 189.08 & 3.07 & 0.06 & \object{VER~J0616.9$+$2230} & \object{IC~443} & 189.08 & 2.92 & 0.16 & 8 \\
    \object{0FGL~J1615.6$-$5049} &         & SNR/PWN & 332.35 & $-$0.01 & 0.23 & \object{HESS~J1616$-$508} & \object{PSR~J1617$-$5055}? & 332.39 & -0.14 & 0.14 & 9 \\
    \object{0FGL~J1648.1$-$4606} &         & SNR/PWN & 339.47 & $-$0.71 & 0.18 & \object{Westerlund 1} region\tablefootmark{f,g} & & 339.55 & $-$0.40 & $\sim$0.9\tablefootmark{h} & 10 \\
    \object{0FGL~J1714.7$-$3827} &         & SNR/PWN & 348.53 & 0.1 & 0.13 & \object{HESS~J1714$-$385} & \object{CTB~37A} & 348.39 & 0.11 & 0.07 & 11 \\
    \object{0FGL~J1801.6$-$2327} &         & SNR/PWN & 6.54 & $-$0.31 & 0.11 & \object{HESS~J1801$-$233} & \object{W~28} & 6.66 & $-$0.27 & 0.17 & 12 \\
    \object{0FGL~J1834.4$-$0841} &         & SNR/PWN & 23.27 & $-$0.22 & 0.1 & \object{HESS~J1834$-$087} & \object{W~41} & 23.24 & $-$0.32 & 0.09 & 9 \\
    \object{0FGL~J1923.0$+$1411} & \object{W~51C}\tablefootmark{i} & SNR  & 49.13 & $-$0.4 & 0.08 & \object{HESS~J1923$+$141}\tablefootmark{f} & \object{W~51} & 49.14 & $-$0.6 & $\sim$0.15\tablefootmark{j} & 13 \\
    \object{0FGL~J1024.0$-$5754} &         & Unid & 284.35 & $-$0.45 & 0.11 & \object{HESS~J1023$-$575} & \object{Westerlund 2}? & 284.19 & $-$0.39 & 0.18 & 14 \\
    \object{0FGL~J1805.3$-$2138} &         & Unid & 8.54 & $-$0.17 & 0.19 & \object{HESS~J1804$-$216} & \object{W~30}/\object{PSR~J1803$-$2137}? & 8.40 & -0.03 & 0.20 & 9 \\
    \object{0FGL~J1839.0$-$0549} &         & Unid & 26.34 & 0.08 & 0.12 & \object{HESS~J1841$-$055} & & 26.8 & $-$0.2 & 0.42 & 15 \\
    \object{0FGL~J1844.1$-$0335} &         & Unid & 28.91 & $-$0.02 & 0.15 & \object{HESS~J1843$-$033}\tablefootmark{f} & & $\sim$29.08 & $\sim$0.16 & $\sim$0.2\tablefootmark{j} & 16 \\
    \object{0FGL~J1848.6$-$0138} &         & Unid & 31.15 & $-$0.12 & 0.16 & \object{HESS~J1848$-$018}\tablefootmark{f} & & 30.98 & $-$0.16 & 0.32 & 17 \\
    \object{0FGL~J0240.3$+$6113} & \object{LS~I~$+$61~303} & HMXB & 135.66 & 1.08 & 0.07 & \object{VER~J0240$+$612} & \object{LS~I~$+$61~303} & 135.70 & 1.08 & PS & 18 \\
    \object{0FGL~J1826.3$-$1451} & \object{LS 5039}      & HMXB & 16.89 & $-$1.32 & 0.11 & \object{HESS~J1826$-$148} & \object{LS~5039} & 16.90 & $-$1.28 & PS & 19 \\
    \hline
\end{tabular}
\tablefoot{
\tablefoottext{a}{Based on timing information.}
\tablefoottext{b}{Source class according to~\citet{bsl_lat}. PSR: pulsar; SNR/PWN: supernova remnant/PWN; HMXB: high-mass X-ray binary; Unid: unidentified sources. The classification of those sources as SNR/PWN is based on spatial coincidence only.}
\tablefoottext{c}{95\% positional error.}
\tablefoottext{d}{Based on spatial coincidence only.}
\tablefoottext{e}{An entry of ``PS'' indicates that the source is point-like with respect to the point spread function of the respective instrument.}
\tablefoottext{f}{These recent source discoveries are preliminary and they have been published in the referenced conference proceedings only.}
\tablefoottext{g}{The VHE emission has been detected by HESS towards the direction of the massive stellar cluster. The coordinates refer to the nominal position of \object{Westerlund~1}.}
\tablefoottext{h}{The extent of the source is not clear. The given value is estimated from the radial profile shown in Fig. 4 of the corresponding reference.}
\tablefoottext{i}{The association is based on a morphological study~\citep{lat_W51C}.}
\tablefoottext{j}{The extent of the source is not clear. The given value is estimated from the sky excess map in the corresponding reference.}
}\vspace{-2mm}
\tablebib{
(1)~\citet{hess_crab}; (2)~\citet{hess_velaX}; (3)~\citet{hess_kookaburra}; (4)~\citet{hess_1706}; (5)~\citet{hess_psr_1718_1809}; (6)~\citet{hess_1908+063}; (7)~\citet{hegra_TeV2032}; (8)~\citet{veritas_ic443};
(9)~\citet{hess_survey}; (10)~\citet{hess_westerlund1_1648}; (11)~\citet{CTB_37A}; (12)~\citet{hess_1801-233}; (13)~\citet{hess_w51}; (14)~\citet{hess_westerlund2_1023}; (15)~\citet{hess_dark}; (16)~\citet{hess_survey_2007}; (17)~\citet{hess_1848_HDGS}; (18)~\citet{veritas_LSI61}; (19)~\citet{hess_LS5039}.
}
\end{table}