\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.}} %\vspace*{5mm} \end{table}