\begin{table}%t1 
      \caption{\label{results}Results from long-term HESS observations of PKS~2005$-$489.}
         \small
           %\centering
\par
         \begin{tabular}{c c c c c c c c c c c c c}
            \hline\hline
            \noalign{\smallskip}
            Dark & MJD & MJD & Time & On & Off & $\alpha$ & Excess & Sig 
& $I$($>$400~GeV)\tablefootmark{a} 
& Crab\tablefootmark{b}  
& $\chi^2$~~(NDF\tablefootmark{c}) 
& $P$($\chi^2$)$^c$\\
            period & first & last & [h] & & & & &  [$\sigma$] & [10$^{-12}$~cm$^{-2}$~s$^{-1}$] & \% & & \\
            \noalign{\smallskip}
            \hline
            \noalign{\smallskip}
            06/2004 & 53171 & 53185 & 8.1  & 678 & 5877  & 0.0919 & 138 & 5.4 & $2.64\pm0.50$ & 3.0 & 7.2~~(10) & 0.71\\
            07/2004 & 53199 & 53205 & 1.5  & 105 & 985   & 0.0909 & 15  & 1.5 & $1.06\pm1.18$ & 1.2 & 1.4~~(1)  & 0.75\\
            09/2004 & 53255 & 53268 & 5.6  & 342 & 3171  & 0.0916 & 52  & 2.8 & $1.89\pm0.78$ & 2.1 & 2.1~~(5)  & 0.84\\
            10/2004 & 53285 & 53292 & 9.0  & 569 & 5065  & 0.0916 & 105 & 4.5 & $2.58\pm0.62$ & 2.9 & 1.5~~(4)  & 0.83\\
            07/2005 & 53582 & 53595 & 9.4  & 573 & 4504  & 0.0908 & 164 & 7.3 & $3.56\pm0.67$ & 4.0 & 9.2~~(9)  & 0.42\\
            08/2005 & 53609 & 53618 & 5.1  & 286 & 2159  & 0.0989 & 73  & 4.5 & $2.86\pm0.93$ & 3.2 & 4.6~~(4)  & 0.33\\
            09/2005 & 53639 & 53646 & 18.1 & 1072 & 9125 & 0.0928 & 225 & 7.1 & $2.93\pm0.46$ & 3.3 & 13.1~~(6) & 0.041\\
            06/2006 & 53908 & 53909 & 1.3  & 127 & 824   & 0.0938 & 50  & 4.9 & $4.72\pm1.32$ & 5.3 & 0.0~~(1)  & 0.97\\
            07/2006 & 53938 & 53940 & 4.4  & 397 & 2927  & 0.0901 & 133 & 7.3 & $4.33\pm0.70$ & 4.8 & 1.3~~(2)  & 0.52\\
            08/2006 & 53967 & 53977 & 8.4  & 500 & 4261  & 0.0913 & 111 & 5.1 & $2.74\pm0.57$ & 3.1 & 15.1~~(7) & 0.035\\
            09/2006 & 53995 & 54002 & 7.4  & 405 & 4116  & 0.0920 & 26  & 1.3 & $1.31\pm0.58$ & 1.5 & 6.0~~(5)  & 0.30\\
	    06/2007 & 54264 & 54270 & 5.3 & 333 & 3006 & 0.0924 & 55 & 3.1 & $1.02\pm0.60$ & 1.1 & 1.9~~(6) & 0.93\\
	    07/2007 & 54291 & 54304 & 4.4 & 309 & 2412 & 0.0964 & 76 & 4.5 & $2.51\pm0.70$ & 2.8 & 15.2~~(8) & 0.056\\
	    08/2007 & 54321 & 54329 & 1.8 & 93 & 849 & 0.0977 & 10 & 1.0 & $0.52\pm0.92$ & 0.6 & 2.9~~(3) & 0.41\\
	    09/2007 & 54345 & 54345 & 0.5 & 11 & 114 & 0.1000 & 0 & $-0.1$ & $<$$6.60$\tablefootmark{d} & $<$7.4 & $-$ & $-$ \\
            \noalign{\smallskip}
             2004 & 53171 & 53292 & 24.2 & 1694 & 15098 & 0.0917 & 310 & 7.7 & $2.37\pm0.33$ & 2.6 & 2.0~~(3) & 0.57\\
            2005 & 53582 & 53646 & 32.6 & 1931 & 15785 & 0.0930 & 462 & 11.0 & $3.09\pm0.35$ & 3.5 & 0.6~~(2) & 0.73\\
            2006 & 53908 & 54002 & 21.5 & 1429 & 12128 & 0.0914 & 320 & 8.8 & $2.84\pm0.34$ & 3.2 & 13.5~~(3) & 0.0037 \\
	    2007 & 54264 & 54345 & 12.0 & 746 & 6381 & 0.0947 & 141 & 5.3 & $1.50\pm0.40$ & 1.7 &  3.8~~(3) & 0.28\\
            \noalign{\smallskip} 
             Total & 53171 & 54345 & 90.3 & 5800 & 49392 & 0.0924 & 1233 & 16.7 & $2.57\pm0.18$ & 2.9 & 10.2~~(3) & 0.016 \\ 
             \hline
       \end{tabular}
       \tablefoot{\tablefoottext{a}{The integral flux above 400~GeV is calculated using the excess of events above an energy threshold, which differs
slightly from the observed excess.  The quoted error is statistical only and the
20\% systematic error on the observed flux is not shown.}
\tablefoottext{b}{The percentage is calculated relative to the HESS Crab Nebula flux above 400~GeV \citep{HESS_crab}.}
\tablefoottext{c}{The $\chi^2$, degrees of freedom (NDF), and corresponding $\chi^2$~probability $P$($\chi^2$) are given for fits of a constant to $I$($>$400~GeV) binned nightly within a dark period, or monthly within a year, or yearly within the total.}
\tablefoottext{d}{The upper limit is calculated
at a 99.9\% confidence level \citep{UL_tech}.}}
        \end{table}