\begin{table}%t1 \par \caption{\label{tab:oir}Optical-IR parameters and redshift of the sample.} \par %\centerline { \begin{tabular}{cccccccccccc} \hline\hline \multicolumn{1}{c} {ID}& \multicolumn{1}{c} {Name}& \multicolumn{1}{c} {$R$}& \multicolumn{1}{c} {$F_{3.6~\mu{\rm m}}$}& \multicolumn{1}{c} {$F_{4.5~\mu{\rm m}}$}& \multicolumn{1}{c} {$F_{5.8~\mu{\rm m}}$}& \multicolumn{1}{c} {$F_{8~\mu{\rm m}}$}& \multicolumn{1}{c} {$F_{24~\mu{\rm m}}$}& \multicolumn{1}{c} {Log($F_{24~\mu {\rm m}}$/$F_{\rm R}$)}& \multicolumn{1}{c} {Log($\lambda L_{5.8~\mu{\rm m}}$)}& \multicolumn{1}{c} {$z$}& \multicolumn{1}{c} {$z$-type} \\ (1) & (2) & (3) & (4) & (5) & (6) & (7) & (8) & (9) & (10) & (11) & (12) \\\hline 1 & J021559.46-045517.5 & 25.65 & 148.1 & 248.8 & 389.1 & 636.6 & 2364 & 4,2 & 45.14 & 1.007 & SP $^a$ \\ 2 & J021625.91-050425.1 & 24.39 & 14.31 & 34.45 & 106.5 & 400.0 & 2174 & 3.7 & 45.96 & 2.236 & PH $^h$ \\ 3 & J021656.59-051005.3 & 24.31 & 83.82 & 146.1 & 249.2 & 490.0 & 2083 & 3.7 & 45.12 & 1.080 & PH $^h$ \\ 4 & J021734.65-051718.2 & 26.36 & 59.84 & 111.0 & 222.1 & 419.7 & 1322 & 4.3 & 45.64 & 1.938 & PH $^h$ \\ 5 & J021743.09-044921.6 & 24.20 & 146 & 270.2 & 496.0 & 871.9 & 1508 & 3.5 & 45.13 & 1.042 & PH $^h$ \\ 6 & J021749.00-052306.9 & 22.36 & 375.6 & 714.2 & 1271 & 2317 & 8105 & 3.5 & 45.67 & 0.914 & SP $^a$ \\ 7 & J021754.45-043016.0 & 23.34 & 132.5 & 243.9 & 509.9 & 1055 & 2922 & 3.4 & 45.91 & 1.780 & PH $^h$ \\ 8 & J021912.66-043308.5 & 23.80 & 27.39 & 21.36 & $-$ & $-$ & 1471 & 3.3 & 44.42 & 0.754 & PH $^h$ \\ 9 & J021924.57-045300.0 & 25.26 & 30.38 & 42.14 & 67.16 & $-$ & 1473 & 3.9 & 45.62 & 1.979 & PH $^h$ \\ 10 & J021935.19-050528.4 & 22.70 & 159.8 & 142.5 & 151.1 & 328.6 & 4095 & 3.3 & 44.76 & 0.826 & SP $^b$ \\ 11 & J022003.58-045145.6 & 23.07 & 123 & 215.7 & 380.7 & 667.7 & 3374 & 3.4 & 45.28 & 1.080 & PH $^h$ \\ 12 & J022003.95-045220.4 & 24.22 & 48.1 & 77.87 & 177.6 & 436.7 & 2831 & 3.7 & 45.50 & 1.443 & PH $^h$ \\ 13 & J160623.44+542301.9 & 24.59 & 35.85 & 41.66 & 43.79 & 86.93 & 1546 & 3.6 & 45.05 & 1.466 &PH$^h$ \\ 14 & J160650.71+542510.1 & $>$24.30 & 290.2 & 258.2 & 193.1 & 818.8 & 1768 & $>$3.5 & 43.66 & 0.22 &SP$^c$ \\ 15 & J160700.62+542416.8 & 26.02 & 18.04 & 37.57 & 95.66 & 315.3 & 1937 & 4.2 & 44.35 & 0.63$_{-0.20}^{+0.20}$ &PH$^g$ \\ 16 & J160813.86+541942.4 & 25.09 & 63.38 & 130.0 & 270.4 & 531.2 & 2631 & 4.0 & 45.09 & 1 &PH$^g$ \\ 17 & J160816.15+545351.1 & 24.12 & 64.9 & 127.7 & 333.1 & 680.6 & 2147 & 3.5 & 44.75 & 0.70$_{-0.15}^{+0.15}$ &PH$^g$ \\ 18 & J160913.02+540509.7 & 25.31 & 61.84 & 136.9 & 292.7 & 581.3 & 1319 & 3.8 & 45.02 & 1 &PH$^g$ \\ 19 & J160913.28+542322.0 & 23.86 & 254.4 & 478.6 & 987.4 & 1966 & 4798 & 3.8 & 45.90 & 1.400 &PH$^h$ \\ 20 & J160933.78+535720.2 & 25.57 & 50.39 & 69.80 & 60.08 & 74.27 & 1373 & 3.9 & 44.43 & 1 &PH$^g$ \\ 21 & J160950.98+535836.3 & 23.95 & 131.9 & 236.4 & 406.9 & 752.3 & 1692 & 3.3 & 45.26 & 1.138 &PH$^h$ \\ 22 & J161007.17+540628.5 & 23.34 & 38.47 & 90.59 & 271.9 & 737.3 & 3284 & 3.4 & 45.95 & 1.871 &PH$^h$ \\ 23 & J161017.70+535124.1 & $>$24.80 & 17.48 & 37.81 & 80.36 & 260.6 & 1572 & $>$3.7 & 44.37 & 0.69$_{-0.20}^{+0.20}$ &PH$^g$ \\ 24 & J161017.93+542332.1 & 23.89 & 36 & 58.41 & 135.9 & 375.9 & 2273 & 3.5 & 44.42 & 0.63$_{-0.10}^{+0.10}$ &PH$^g$ \\ 25 & J161037.63+540603.5 & 24.88 & 12.05 & 12.63 & $-$ & 50.06 & 1724 & 3.7 & 46.58 & 3.77$_{-0.77}^{+0.48}$ &PH$^g$ \\ 26 & J161051.03+535330.5 & 25.39 & 13.26 & 20.86 & 57.56 & 197.4 & 1560 & 3.9 & 44.22 & 0.66$_{-0.15}^{+0.15}$ &PH$^g$ \\ 27 & J161052.74+543740.4 & 23.53 & 70.77 & 66.55 & 72.03 & 136.1 & 2646 & 3.4 & 45.21 & 1.410 &PH$^h$ \\ 28 & J161102.22+550551.6 & 24.10 & 71.53 & 73.24 & 121.4 & 350.9 & 2661 & 3.6 & 44.97 & 0.995 &PH$^h$ \\ 29 & J161204.84+544149.2 & 25.07 & 33.74 & 46.92 & 42.97 & 54.68 & 1808 & 3.8 & 45.98 & 2.58$_{-0.30}^{+0.40}$ &PH$^g$ \\ 30 & J161306.28+543959.7 & 24.91 & 23.5 & 54.15 & 170.7 & 548.9 & 2922 & 4.0 & 44.40 & 0.54$_{-0.10}^{+0.10}$ &PH$^g$ \\ 31 & J163723.94+410525.7 & 23.80 & 77.52 & 65.69 & 52.22 & 133.9 & 1856 & 3.3 & 44.94 & 1.24 &PH$^h$ \\ 32 & J104409.95+585224.7 & 23.56 & 64.27 & 150.4 & 390.9 & 1093 & 4134 & 3.6 & 46.41& 2.54 &SP$^d$ \\ 33 & J104528.29+591326.6 & 23.68 & 32.18 & 45.19 & 90.94 & 206.6 & 2462 & 3.4 & 45.98& 2.31 &SP$^e$ \\ 34 & J104837.82+572816.2 & 23.84 & 100.6 & 170.3 & 307.5 & 625.3 & 2355 & 3.5 & 45.53& 1.443 &PH$^h$ \\ 35 & J104847.14+572337.6 & 23.74 & 158.1 & 285.4 & 451.8 & 797.1 & 2590 & 3.5 & 45.42& 1.218 &PH$^h$ \\ 36 & J104954.96+584429.4 & 24.15 & 18.45 & 23.43 & 58.82 & 146.6 & 1378 & 3.3 & 44.27& 0.76$_{-0.10}^{+0.10}$ &PH$^g$ \\ 37 & J105604.84+574229.9 & 22.21 & 62.28 & 85.63 & 158.6 & 438.5 & 11~280& 3.5 & 45.59& 1.249 &PH$^h$ \\ 38 & J003314.61-432300.3 & 24.13 & 10.5 & 16.69 & 57.68 & 142.5 & 1648 & 3.4 & 44.46 & 0.87$_{-0.20}^{+0.20}$ & PH$^g$\\ 39 & J003316.92-431706.3 & 24.30 & 142.2 & 295.1 & 581.9 & 1059 & 2197 & 3.6 & 44.88 & 0.689 & SP$^f$\\ 40 & J003333.75-432326.9 & 24.41 & 48.02 & 73.56 & 161.1 & 225.4 & 1493 & 3.5 & 45.03 & 1.24$_{-0.20}^{+0.20}$ & PH$^g$\\ 41 & J003336.26-431731.7 & 24.65 & 18.66 & 34.14 & 82.01 & 259.0 & 2188 & 3.7 & 44.51 & 0.76$_{-0.10}^{+0.10}$ & PH$^g$\\ 42 & J003348.18-432822.3 & $>$26.63 & 16.17 & 40.72 & 98.36 & 346.5 & 1682 & $>$4.4 & 44.70 & 0.84$_{-0.05}^{+0.05}$ & PH$^g$\\ 43 & J003518.20-433414.6 & 25.19 & 12.06 & 16.96 & $-$ & 142.6 & 1745 & 3.9 & 45.38 & 1.69$_{-1.00}^{+0.40}$ & PH$^g$\\ 44 & J003641.47-432038.1 & 23.91 & 110 & 224.6 & 459.3 & 911.7 & 2746 & 3.6 & 45.25 & 1 & PH$^g$\\ \hline \end{tabular}} \par \medskip Column: (1) ID number; (2) name from SWIRE2 catalogue; (3) magnitude $R$; (4) 3.6 $\mu$m flux density in $\mu$Jy; (5) 4.5 $\mu$m flux density in $\mu$Jy; (6)~5.8~$\mu$m flux density in $\mu$Jy; (7) 8 $\mu$m flux density in $\mu$Jy; (8) 24 $\mu$m flux density in $\mu$Jy; (9) logarithm of $F_{24~\mu {\rm m}}$/$F_{\rm R}$ flux ratio; (10) logarithm of 5.8~$\mu$m luminosity in erg s$^{-1}$; (11) redshift; (12) type of redshift: SP spectroscopic redshift [$^a$ this work (see Sect.~2.3.1 for details); $^b$ Simpson et~al. (2006); $^c$ from Sloan Digital Sky Survey Data Release 2; $^d$ Polletta et~al. (\cite{Polletta2006}); $^e$ Weedman et~al. (2006a); $^f$ Feruglio et~al. (\cite{Feruglio2008})], PH photometric redshift [$^g$ this work (see Sect.~2.3 for details); $^h$ Rowan-Robinson et~al. (\cite{Rowan-Robinson2008}); $^i$ fixed value of $z$]. \vspace*{3mm} \end{table}