\begin{table}%t3 \caption{\label{tab:redshifts1138}Results of optical and near-IR spectroscopy in the MRC~1138$-$262\ field.} \small %\centerline { \begin{tabular}{r r r r r r r r l r r} \hline\hline\noalign{\smallskip} ID & RA(J2000) & Dec.(J2000) & $B_{\rm total}$ & $I_{\rm total}$ & $J_{\rm total}$ & $K_{\rm s, total}$ & $J-K_{\rm s}$ (1\farcs5) & Instr. & $z$ & Quality$^a$ \\ \hline 493 & 11 40 33.42 & $-$26 29 14.6 & $>$27 & $>$26.2 & 22.89 & 20.55 & 2.56 & FORS2 & ... & 4 \\ %slit 29 867 & 11 40 34.09 & $-$26 30 38.7 & $>$27 & 25.32 & $>$23.3 & 21.30 & 2.49 & FORS2 & ... & 4 \\ %slit 20 156 & 11 40 34.82 & $-$26 27 46.4 & $>$27 & $>$26.2 & $>$23.3 & 21.15 & 4.23 & FORS2 & ... & 4 \\ %slit 22 174 & 11 40 35.45 & $-$26 27 51.8 & 25.35 & 25.06 & $>$23.3 & $>$22 & 2.51 & FORS2 & ... & 3 \\ %slit 21 676 & 11 40 36.96 & $-$26 29 55.6 & $>$27 & $>$26.2 & 22.57 & 19.79 & 3.07 & FORS2 & ... & 4 \\ %slit 28 808 & 11 40 38.19 & $-$26 30 24.3 & $>$27 & 24.87 & 22.91 & 20.44 & 2.56 & FORS2 & ... & 4 \\ %slit 10 552 & 11 40 38.28 & $-$26 29 25.1 & $>$27 & 25.37 & 22.67 & 20.47 & 2.41 & MOIRCS & ... & 4 \\ 364 & 11 40 39.76 & $-$26 28 45.4 & 24.17 & 22.87 & 21.24 & 19.03 & 2.21 & MOIRCS & ... & 3 \\ 877 & 11 40 40.24 & $-$26 30 41.2 & 25.96 & 24.91 & 23.44 & 21.30 & 2.35 & FORS2 & ... & 3 \\ %slit 19 341 & 11 40 41.47 & $-$26 28 37.2 & $>$27 & 24.81 & 23.63 & 20.48 & 3.06 & FORS2 & 3.263 & 1 \\ %slit 08 147 & 11 40 43.48 & $-$26 27 44.1 & $>$27 & $>$26.2 & 21.98 & 20.04 & 2.43 & FORS2 & ... & 3 \\ %slit 23 369 & 11 40 43.46 & $-$26 28 45.2 & $>$27 & $>$26.2 & $>$23.3 & 21.30 & 3.83 & MOIRCS & ... & 4 \\ %NIC J-H=2.0 905 & 11 40 44.01 & $-$26 30 47.0 & $>$27 & $>$26.2 & 23.45 & 20.86 & 2.69 & MOIRCS & ... & 4 \\ 456 & 11 40 44.28 & $-$26 29 07.7 & $>$27 & 24.71 & 21.28 & 18.93 & 2.45 & FORS2 & ... & 3 \\ %slit 09 & & & & & & & & MOIRCS & 2.172 & 2 \\ %MIPS NIC J-H=1.7 464 & 11 40 46.09 & $-$26 29 11.5 & $>$27 & $>$26.2 & 21.54 & 19.06 & 2.41 & MOIRCS & 2.149 & 2 \\ %MIPS 558 & 11 40 46.52 & $-$26 29 27.1 & $>$27 & 24.71 & 21.64 & 19.03 & 2.55 & MOIRCS & ... & 4 \\ %NIC J-H=1.5 476 & 11 40 46.68 & $-$26 29 10.4 & $>$27 & 24.90 & 22.30 & 19.86 & 2.46 & FORS2 & ... & 3 \\ %slit 07 605 & 11 40 47.58 & $-$26 29 38.2 & $>$27 & $>$26.2 & $>$23.3 & 21.07 & 3.51 & FORS2 & ... & 4 \\ %slit 33 & & & & & & & & MOIRCS & ... & 4 \\ %NIC J-H=1.9 830 & 11 40 48.36 & $-$26 30 30.6 & $>$27 & 20.48 & 20.67 & 18.86 & 2.20 & MOIRCS & ... & 3 \\ 492 & 11 40 49.59 & $-$26 29 07.7 & $>$27 & 25.60 & 23.09 & 20.02 & 2.84 & FORS2 & ... & 4 \\ %slit 34 392 & 11 40 50.35 & $-$26 28 49.6 & $>$27 & $>$26.2 & 23.47 & 20.56 & 2.47 & FORS2 & ... & 4 \\ %slit 35 573 & 11 40 50.75 & $-$26 29 32.5 & $>$27 & 24.68 & 21.98 & 20.04 & 2.06 & MOIRCS & ... & 4 \\ %NIC J-H=1.2 601 & 11 40 51.30 & $-$26 29 38.5 & $>$27 & 23.45 & 21.27 & 19.05 & 2.35 & FORS2 & ... & 3 \\ %slit 12 506 & 11 40 53.13 & $-$26 29 18.1 & $>$27 & 23.55 & 21.33 & 19.01 & 2.38 & FORS2 & ... & 3 \\ %slit 13 165 & 11 40 54.01 & $-$26 27 48.1 & $>$27 & $>$26.2 & 23.35 & 20.85 & 2.59 & FORS2 & ... & 4 \\ %slit 32 241 & 11 40 54.77 & $-$26 28 03.6 & $>$27 & 25.44 & 23.16 & 20.78 & 2.76 & FORS2 & ... & 3 \\ %slit 14 223 & 11 40 55.99 & $-$26 28 02.9 & 26.13 & 24.30 & $>$23.3 & 21.36 & 2.37 & FORS2 & 3.455 & 1 \\ %slit 24 268 & 11 40 57.02 & $-$26 28 17.5 & $>$27 & 23.02 & 20.57 & 18.35 & 2.64 & FORS2 & ... & 3 \\ %slit 15 206 & 11 40 57.87 & $-$26 27 59.3 & $>$27 & 24.52 & 23.51 & 20.28 & 2.40 & FORS2 & ... & 3 \\ %slit 16 565 & 11 41 00.10 & $-$26 29 28.1 & $>$27 & $>$26.2 & 22.72 & 20.31 & 2.57 & FORS2 & ... & 4 \\ %slit 31 451 & 11 41 00.84 & $-$26 29 04.7 & $>$27 & $>$26.2 & $>$23.3 & 21.26 & 3.11 & FORS2 & ... & 4 \\ %slit 17 90 & 11 41 01.54 & $-$26 27 31.2 & $>$27 & 23.55 & 21.38 & 18.89 & 2.51 & FORS2 & ... & 3 \\ %slit 18 728 & 11 41 02.69 & $-$26 30 07.8 & $>$27 & $>$26.2 & 21.03 & 18.89 & 2.56 & FORS2 & ... & 4 \\ %slit 30 \hline ... & 11 40 43.85 & $-$26 31 26.4 & \multicolumn{5}{c}{Ly-$\alpha$ emitter candidate}& FORS2 & ... & 3 \\ ... & 11 40 50.68 & $-$26 31 00.0 & \multicolumn{5}{c}{Ly-$\alpha$ emitter candidate}& FORS2 & ... & 4\\ \hline\end{tabular}} \smallskip $^a$ Quality flags are the same as in Table~2. Limiting magnitudes are 5$\sigma$. \vspace*{4mm} \end{table}