\begin{table}%t1
\caption{\label{sandint1}Flux measurements of {\obj}.}
%\centering
\par
\begin{tabular}{lcr@{\hspace{5pt}}lr@{\hspace{5pt}}lr@{\hspace{5pt}}lr@{\hspace{5pt}}lr@{\hspace{5pt}}lrr}
\hline\hline \noalign{\smallskip}
Emission line          & $\lambda_0$ [\AA] &
      \multicolumn{2}{c}{PMAS$_{{\rm raw}}$} & \multicolumn{2}{c}{PMAS$_{{\rm corr.}}$} &
      \multicolumn{2}{c}{{\rR} (SPM1)} & \multicolumn{2}{c}{{\rR} (CFHT)} &
      \multicolumn{2}{c}{{\rJ}\tablefootmark{a}} & \multicolumn{1}{c}{{\rT}} & $I({\rm case~B})$\\[1.5pt]
\hline
\noalign{\smallskip}
{}[\ion{O}{iii}]  & 5006.84 &   3.36 & (0.33) &   3.48 & (0.35) &   2.7 & (1.3)  & 2.87   &(0.85) &  3 & (1) & 3.1 &       \\
{}[\ion{O}{iii}]  & 4958.92 &   1.27 & (0.29) &   1.33 & (0.30) &       &        &        &       &    &     &     &       \\
{\hb}             & 4861.32 & 100.00 & (0.49) & 100.00 & (0.49) & 100.0 & (2.1)  & 100.0\xx  & (1.7) & 100&     & 100 & 100.0 \\
\ion{He}{ii}    & 4685.65 &  78.72 & (0.62) &  82.11 & (0.64) &  76.1 & (2.3)  &  78.6\xx  & (1.5) & 77 & (3) &  92 &       \\
\ion{He}{ii}    & 4541.59 &   2.96 & (0.39) &   3.09 & (0.40)  \\       
H$\gamma$         & 4340.45 &  45.49 & (0.60) &  45.40 & (0.63) &  41.0 & (1.6)  &  42.05 & (0.98)& 39 & (3) &  56 &  47.6 \\
\ion{He}{ii}    & 4199.83 &   2.48 & (0.59) &   2.59 & (0.61)  \\
H$\delta$         & 4101.74 &  23.81 & (0.64) &  23.69 & (0.66) &  21.4 & (2.8)  &  20.6\xx  & (1.2) & 17 & (2) &  30 &  26.6 \\
H7                & 3970.07 &   9.70 & (0.73) &  10.11 & (0.76) &  10.0 & (2.5)  &   6.11 & (0.64)&  4 & (1) &  11 &  16.4 \\
H8                & 3889.06 &   8.63 & (0.89) &   9.00 & (0.93) &       &        &   2.92 & (0.73)&    &     &     &  10.8 \\
{}[\ion{Ne}{iii}] & 3868.80 & ${<}1$ &        & ${<}1$ &        &       &        &   1.04 & (0.52)& 15 & (7) &     &       \\
H9                & 3835.40 &   8.22 & (0.99) &   8.6\xx  & (1.0)  &       &        &        &       &    &     &     &   7.5 \\
H10               & 3797.91 &   3.4\xx & (1.2)  &   3.3\xx  & (1.2)  &       &        &        &       &    &     &     &   5.8 \\
$F$(\hb)\tablefootmark{b}      && 1.924  & (0.009)&        &        & 1.82  &(0.03)  &   2.55 & (0.03)&\multicolumn{2}{c}{1.47}     & 1.19 \\
\hline
\end{tabular}
\tablefoot {Errors are given in parentheses. The emission line names and the rest wavelength~$\lambda_0$, and Case~B line ratios for the Balmer lines to~{\hb}, are given in Cols.~1, 2, and~9. We present our raw values in Col.~3 and values corrected for the contribution of \ion{He}{ii} Pickering lines to the Balmer lines in Col.~4. Columns~5$-$8 give the values presented by {\rR} (SPM1), {\rR} (CFHT), {\rJ}, and \rT, respectively. \\
\tablefoottext{a}{The line ratios are corrected for an extinction value of $E(B-V)$~$=$ $0.03$ and for a~${\sim}5\%$ contribution of \ion{He}{ii}-lines to Balmer lines.}\\
\tablefoottext{b}{This is the total flux in emission measured for {\hb} in units of $10^{-14}$~\Fl, systematic errors are not considered in the error estimate.}}
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\end{table}