\begin{table}%t2
\caption{\label{tbl:obs2}{\it Herschel} observing geometries for our seven targets, including properties derived from ground-based visible observations and the obtained radiometric solutions.}
%\centering
\par
\begin{tabular}{lcccllll|cccc}
\hline \hline
\multicolumn{8}{c|}{} &\multicolumn{4}{c}{} \\[-6pt]
Target & $r$ [AU] & $\Delta$ [AU] & $\alpha$ $[^\circ]$ & $H_V$ [mag] & $\Delta_{\rm mag}$ & $P$ [h] & Ref. & $D^{\rm TPM}_{\rm eff}$ & $p^{\rm TPM}_V$ & $\Gamma$ & $\eta$ \\
\multicolumn{8}{c|}{} &\multicolumn{4}{c}{} \\[-8pt]
\hline
2003 AZ$_{84}$   & 45.376 & 44.889 & 1.11 & 3.83 $\pm$ 0.04 & 0.14 $\pm$ 0.03 & 6.79~h & 1, 2, 3       & 850--970 & 0.05--0.09 & 2--10 & 1.31		\\	
2001 YH$_{140}$  & 36.576 & 36.169 & 1.44 & 5.8 $\pm$ 0.2   & 0.13 $\pm$ 0.05 & 13.2~h & 4           & 300--390 & 0.06--0.10 & 0--10 & 1.2$^{\star}$  \\	
1997 CS$_{29}$   & 43.509 & 43.241 & 1.27 & 5.65 $\pm$ 0.09 & $<$0.08, $<$0.22 & --- & 5, 6, 7, 8   & 250--420 & 0.06--0.14 & 0--25 & 1.2$^{\star}$  \\	
2000 YW$_{134}$  & 44.125 & 43.833 & 1.25 & 4.88 $\pm$ 0.05 & $<$0.10 & --- & 9, 10                 &  $<$500 & $>$0.08   & 0--25 & ---		\\	
Typhon      & 17.943 & 18.376 & 2.84 & 7.68 $\pm$ 0.04 & 0.07 $\pm$ 0.01 & 9.67~h & 4, 11, 12   & 134--154 & 0.065--0.085 & 1--10 & 0.96		\\
2006 SX$_{368}$  & 11.972 & 12.271 & 4.48 & 9.5           & --- & --- & MPC                       & 70--80   & 0.05--0.06 & 0--40 & 1.2$^{\star}$  \\	
2005 TB$_{190}$  & 46.377 & 46.683 & 1.17 & 4.58 $\pm$ 0.22 & 0.12 $\pm$ 0.02 & 12.68~h & 13         & 335--410 & 0.15--0.24 & 0--25 & 1.2$^{\star}$  \\	
\hline
\end{tabular}
\tablefoot {$r$: Sun-target distance, $\Delta$: {\it Herschel}-target distance, $\alpha$: phase angle; $H_V$~magnitudes, lightcurve~$\Delta_{\rm mag}$, and the rotation period~$P$; references for the preceeding three columns, derived effective diameter~$D^{\rm TPM}_{\rm eff}$ in~[km] and geometric albedo~$p^{\rm TPM}_V$ values from  the TPM~analysis, the corresponding possible thermal inertias~$\Gamma$ [J~m$^{-2}$~s$^{-0.5}$~K$^{-1}$],  and the fitted NEATM $\eta$~value ($^{\star}$: for a fixed value).}\vspace{-2mm}
\tablebib {(1) Fornasier et~al. (\cite{fornasier04}); (2) DeMeo et~al. (\cite{demeo09});
(3) Perna et~al. (\cite{perna10});
(4) Thirouin et~al. (\cite{thirouin10});
(5) Sheppard \& Jewitt (\cite{sheppard02});
(6) Romanishin \& Tegler (\cite{romanishin99});
(7) Davies et~al. (\cite{davies00});
(8) Boehnhardt et~al. (\cite{boehnhardt01});
(9) Sheppard \& Jewitt (\cite{sheppard03});
(10) Doressoundiram et~al. (\cite{doressoundiram05});
(11) Rabinowitz et~al. (\cite{rabinowitz07});
(12) Tegler et~al. (\cite{tegler03});
(13) Thirouin et~al., in~prep.;
MPC: {\protect\url {http://www.cfa.harvard.edu/iau/lists/Centaurs.html}}}
\vspace{-3.5mm}\end{table}