\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}