\begin{table}%t1
\caption{\label{TELESCOP}Telescopes and detectors used for follow-up, recovery and secure orbits of NEAs. } 
%%\centering

\par
\begin{tabular}{lclccc}
\hline\hline\noalign{\smallskip}
Telescope & Aperture (m) & CCD & Pixels & FOV (arcmin) & Scale ($\arcsec$/pixel)\\
\hline\noalign{\smallskip}
Pic du Midi & 1.05 & THX7863 & $384\times288$ & $5.2\times3.9$ & 0.820 \\
Haute Provence & 1.20 & TK1024 & $1024\times1024$ & 11.$7\times11.7$ & 0.685\\
Cerro Armazones & 0.85 & SBIG ST-10 & $2184\times1472$ & $15.6\times8.3$ & 0.430 \\
Cerro Tololo & 1.0 & Y4KCam & $4096\times4096$ & $20\times20$ & 0.289 \\ 
Las Campanas & 1.02 & SIT\#3 & $2048\times3650$ & $15.1\times26.5$ & 0.435 \\
La Silla & 1.00 &  SBIG ST-10 & $2184\times1472$ & $3.3\times2.2$ & 0.090 \\
La Silla & 2.20 &  WFI mosaic & $8\times(2184\times1472)$ & $34\times33$ & 0.238\\
Vasile Urseanu, & & & & &  \\
Bucharest & 0.30 & TC273-home made & $640\times500$& $21.6\times16.9$ & 2.30 \\
York University & 0.60 & SBIG ST-9 & $512\times512$ & $4.3\times4.3$ & 0.505 \\
\hline 
\end{tabular}
\par
\tablefoot{The observatory is
given in the first column and the aperture in the second one. The CCD camera (third column), the pixel size (fourth column), the field of view  (FOV), and the scale (in $\arcsec$/pixel) are also presented.}
\end{table}