\begin{table}%[h]%Ta1
\par
\caption{\label{taba1}{AKARI} coordinates and flux densities of PAH-selexted galaxies in the S-cam field.}
\begin{tabular}{lccccccccccccccccccccc}
\hline\hline\noalign{\smallskip}
ID & Name & RA & Dec & 
\multicolumn{2}{c}{${2.4~\mu{\rm m}}$}& 
\multicolumn{2}{c}{${3.2~\mu{\rm m}}$} & 
\multicolumn{2}{c}{${4.1~\mu{\rm m}}$} & 
\multicolumn{2}{c}{${7.0~\mu{\rm m}}$} & 
\multicolumn{2}{c}{${9.0~\mu{\rm m}}$} & 
\multicolumn{2}{c}{${11~\mu{\rm m}}$}  &
\multicolumn{2}{c}{${15~\mu{\rm m}}$}  &
\multicolumn{2}{c}{${18~\mu{\rm m}}$}  &
\multicolumn{2}{c}{${24~\mu{\rm m}}$}  \\
\noalign{\smallskip}
& &  \multicolumn{2}{c}{[J2000]}  &
$f_\nu$ & $\Delta f_\nu$ & 
$f_\nu$ & $\Delta f_\nu$ & 
$f_\nu$ & $\Delta f_\nu$ & 
$f_\nu$ & $\Delta f_\nu$ & 
$f_\nu$ & $\Delta f_\nu$ & 
$f_\nu$ & $\Delta f_\nu$ & 
$f_\nu$ & $\Delta f_\nu$ & 
$f_\nu$ & $\Delta f_\nu$ & 
$f_\nu$ & $\Delta f_\nu$ \\
& & & &
$\mu$Jy & $\mu$Jy & 
$\mu$Jy & $\mu$Jy & 
$\mu$Jy & $\mu$Jy & 
$\mu$Jy & $\mu$Jy & 
$\mu$Jy & $\mu$Jy & 
$\mu$Jy & $\mu$Jy & 
$\mu$Jy & $\mu$Jy & 
$\mu$Jy & $\mu$Jy & 
$\mu$Jy & $\mu$Jy \\
(1) & (2) & (3) & (4)  & (5) & (6) & (7) & (8) &
(9) & (10) & (11) & (12) & (13) & (14) & (15) &
(16) & (17) & (18) & (19) & (20) & (21) & (22)\\
\hline
\noalign{\smallskip}
\multicolumn{21}{c}{PAH-selected galaxies at $z\sim 1$}  \\
 \noalign{\smallskip}
  1163 & J175331.44+662050.3 & 268.38102 &  66.34731 &    64.8 &     2.2 &    75.7 &     2.0 &    61.1 &     1.7 &    42.6 &    11.1 &    40.3 &     8.9 &   110.0 &    13.9 &   461.0 &    24.0 &   466.0 &    22.1 &   545.0 &    51.4  \\
  1637 & J175611.19+662419.4 & 269.04663 &  66.40540 &    38.8 &     2.2 &    43.1 &     1.8 &    35.1 &     1.5 &     3.6 &     6.5 &    22.4 &     8.8 &   107.0 &    14.3 &   262.0 &    18.7 &   198.0 &    18.8 &   254.0 &    41.2  \\
  1664 & J175342.76+662421.9 & 268.42817 &  66.40611 &    84.0 &     3.9 &    79.3 &     2.5 &    53.0 &     1.7 &    37.0 &     9.2 &    21.4 &     8.4 &   188.0 &    13.2 &   268.0 &    23.1 &   210.0 &    21.8 &   363.0 &    59.8  \\
  2043 & J175323.76+662623.2 & 268.34902 &  66.43978 &    47.0 &     2.8 &    47.3 &     2.3 &    30.3 &     1.6 &    40.1 &     8.6 &    22.2 &     8.3 &   105.0 &    12.8 &   187.0 &    20.0 &   122.0 &    19.4 &   148.0 &    64.7  \\
  2073 & J175636.92+662653.6 & 269.15387 &  66.44824 &    53.3 &     2.3 &    47.9 &     2.2 &    32.2 &     1.9 &    48.8 &     8.9 &     9.9 &    12.9 &   220.0 &    20.4 &   266.0 &    25.0 &   115.0 &    27.5 &   162.0 &    50.6  \\
  2437 & J175322.46+662905.7 & 268.34360 &  66.48493 &    69.3 &     3.7 &    95.4 &     3.2 &    82.0 &     2.2 &    77.9 &    10.7 &    38.9 &    10.2 &    90.0 &    15.6 &   499.0 &    25.2 &   426.0 &    22.6 &   547.0 &    61.0  \\
  2711 & J175346.89+663038.2 & 268.44540 &  66.51062 &    40.3 &     1.9 &    45.0 &     1.6 &    34.2 &     1.3 &    44.1 &     8.5 &    27.3 &    10.1 &    77.9 &    13.3 &   318.0 &    23.4 &   378.0 &    22.4 &   351.0 &    50.4  \\
  2836 & J175726.41+663114.3 & 269.36005 &  66.52066 &    70.8 &     2.5 &    87.4 &     2.3 &    80.9 &     2.0 &   113.0 &     8.7 &    67.0 &    10.2 &   106.0 &    14.2 &   588.0 &    32.3 &   627.0 &    30.6 &   545.0 &    72.8  \\
  2932 & J175336.29+663153.2 & 268.40124 &  66.53146 &    33.0 &     1.8 &    42.1 &     1.8 &    38.2 &     1.4 &    39.6 &     8.7 &    19.4 &     9.1 &    39.2 &    15.5 &   192.0 &    20.2 &   256.0 &    17.6 &   246.0 &    43.7  \\
  3033 & J175458.78+663227.3 & 268.74493 &  66.54094 &    54.3 &     2.9 &    69.0 &     2.3 &    64.1 &     1.9 &    56.1 &     9.6 &    26.4 &     8.7 &    86.7 &    12.8 &   327.0 &    23.1 &   257.0 &    19.5 &   539.0 &    49.5  \\
  4359 & J175629.33+664530.6 & 269.12221 &  66.75850 &    52.4 &     2.7 &    64.0 &     2.2 &    49.7 &     1.7 &    17.5 &     8.7 &    24.3 &     8.5 &   198.0 &    12.5 &   383.0 &    33.5 &   185.0 &    30.5 &   482.0 &   111.0  \\
  4856 & J175731.87+664245.6 & 269.38281 &  66.71269 &    60.3 &     2.0 &    63.5 &     1.8 &    50.9 &     1.5 &    43.4 &     8.0 &    39.2 &     9.4 &   105.0 &    11.1 &   400.0 &    25.7 &   326.0 &    25.4 &   387.0 &    72.1  \\
  4956 & J175412.75+664151.2 & 268.55316 &  66.69757 &    39.8 &     3.5 &    48.1 &     2.3 &    44.6 &     2.0 &    49.2 &    11.3 &    19.4 &    12.4 &    37.6 &    15.0 &   250.0 &    25.1 &   168.0 &    25.3 &   137.0 &    57.5  \\
  5545 & J175328.41+663813.9 & 268.36838 &  66.63721 &    57.5 &     2.4 &    81.8 &     2.2 &    93.9 &     2.0 &    82.8 &     8.4 &    70.8 &    11.1 &   160.0 &    16.0 &   853.0 &    27.0 &   780.0 &    24.6 &   725.0 &    54.4  \\
  6344 & J175416.38+665332.4 & 268.56829 &  66.89236 &    24.2 &     2.3 &    42.7 &     2.1 &    54.3 &     1.8 &    84.3 &     9.0 &    85.1 &     8.0 &   122.0 &    12.8 &   685.0 &    26.6 &   709.0 &    26.9 &   425.0 &    60.5  \\
  6452 & J175732.98+665210.6 & 269.38742 &  66.86962 &    27.7 &     1.9 &    39.2 &     1.7 &    40.0 &     1.5 &    39.0 &     9.0 &    39.7 &     8.2 &    30.4 &    10.7 &   431.0 &    34.1 &   358.0 &    37.1 &    83.3 &    83.7  \\
  6536 & J175456.40+665137.9 & 268.73504 &  66.86055 &    25.0 &     1.7 &    34.8 &     1.6 &    32.4 &     1.4 &    15.9 &     7.7 &    13.0 &     7.0 &    30.0 &    10.8 &   339.0 &    26.0 &   243.0 &    27.2 &   263.0 &    54.7  \\
  6650 & J175433.94+665123.1 & 268.64142 &  66.85642 &    33.6 &     2.0 &    49.3 &     1.7 &    43.1 &     1.5 &    22.5 &     7.3 &    23.3 &     8.6 &    42.1 &    11.3 &   290.0 &    23.9 &   267.0 &    19.1 &   228.0 &    48.9  \\
\hline
\noalign{\smallskip}
\multicolumn{21}{c}{PAH-selected galaxies at $z\sim 0.5$}  \\
\noalign{\smallskip}
  1174 & J175731.27+662050.0 & 269.38033 &  66.34723 &   116.0 &     3.3 &   112.0 &     2.5 &    79.1 &     1.9 &    49.4 &    10.4 &   189.0 &    13.0 &   416.0 &    17.8 &   514.0 &    30.4 &   538.0 &    33.9 &   620.0 &    60.7  \\
  1270 & J175526.98+662128.2 & 268.86244 &  66.35784 &    80.4 &     2.5 &    67.1 &     2.0 &    47.3 &     1.5 &    22.9 &     9.2 &   151.0 &    11.3 &   192.0 &    17.9 &   303.0 &    25.3 &   224.0 &    26.0 &   396.0 &    56.3  \\
  1321 & J175700.71+662141.3 & 269.25297 &  66.36148 &   142.0 &     3.3 &   112.0 &     2.5 &    79.7 &     1.9 &    58.4 &     9.0 &   328.0 &    12.3 &   501.0 &    18.9 &   485.0 &    24.6 &   594.0 &    23.6 &   841.0 &    56.7  \\
  1381 & J175650.63+662213.2 & 269.21097 &  66.37034 &    39.3 &     2.0 &    44.6 &     1.9 &    30.0 &     1.3 &    48.1 &     8.7 &   252.0 &    10.7 &   407.0 &    16.8 &   315.0 &    19.9 &   255.0 &    23.0 &   766.0 &    56.9  \\
  1451 & J175559.22+662245.6 & 268.99678 &  66.37935 &    85.1 &     2.6 &    70.8 &     2.1 &    52.9 &     1.7 &    23.3 &     8.1 &   102.0 &     8.9 &   226.0 &    14.3 &   262.0 &    23.8 &   227.0 &    20.2 &   186.0 &    42.2  \\
  1569 & J175600.05+662334.6 & 269.00021 &  66.39296 &    62.3 &     2.4 &    69.5 &     2.1 &    48.7 &     1.4 &    15.7 &     8.2 &   134.0 &     9.4 &   184.0 &    15.3 &   441.0 &    26.0 &   354.0 &    22.5 &   388.0 &    48.4  \\
  1642 & J175345.99+662357.8 & 268.44166 &  66.39940 &    48.4 &     3.7 &    55.4 &     3.5 &    39.2 &     2.3 &    35.4 &    10.4 &    93.8 &    10.1 &   306.0 &    15.6 &   325.0 &    26.9 &   406.0 &    25.0 &   403.0 &    56.1  \\
  1681 & J175640.43+662403.8 & 269.16847 &  66.40106 &    58.4 &     2.4 &    47.2 &     2.0 &    37.1 &     1.6 &    31.3 &     7.5 &   171.0 &     9.7 &   328.0 &    15.9 &   318.0 &    20.5 &   387.0 &    19.8 &   471.0 &    46.4  \\
  1726 & J175629.54+662444.9 & 269.12310 &  66.41249 &    81.9 &     2.5 &    64.9 &     2.0 &    42.2 &     1.5 &    27.4 &     7.9 &   175.0 &    13.1 &   313.0 &    14.8 &   236.0 &    20.9 &   329.0 &    19.7 &   238.0 &    49.0  \\
  1776 & J175631.43+662447.1 & 269.13098 &  66.41309 &   177.0 &     3.5 &   143.0 &     2.7 &   105.0 &     2.1 &    80.0 &     9.0 &   411.0 &    13.7 &   738.0 &    18.1 &   637.0 &    26.7 &   738.0 &    24.6 &   914.0 &    53.9  \\
  1901 & J175630.45+662550.4 & 269.12690 &  66.43068 &    55.6 &     2.1 &    42.7 &     1.6 &    30.0 &     1.2 &    13.0 &     8.3 &    94.5 &    14.1 &   237.0 &    20.3 &   147.0 &    19.7 &   143.0 &    23.9 &   222.0 &    50.2  \\
  1908 & J175518.76+662529.8 & 268.82820 &  66.42497 &   391.0 &     5.0 &   325.0 &     3.9 &   221.0 &     2.9 &   188.0 &    11.3 &   888.0 &    15.0 &  1540.0 &    21.9 &  1320.0 &    29.0 &  1370.0 &    26.3 &  1340.0 &    56.4  \\
  1934 & J175427.51+662545.6 & 268.61465 &  66.42934 &    87.7 &     2.5 &    67.0 &     2.1 &    57.8 &     1.7 &    18.2 &    10.6 &   329.0 &    12.6 &   543.0 &    17.5 &   414.0 &    23.7 &   518.0 &    23.6 &   520.0 &    48.0  \\
  2048 & J175415.43+662625.6 & 268.56430 &  66.44046 &   187.0 &     3.4 &   177.0 &     3.0 &   128.0 &     2.3 &    81.1 &     9.8 &   387.0 &    11.7 &   659.0 &    17.5 &   553.0 &    22.6 &   502.0 &    22.7 &   827.0 &    53.9  \\
  2111 & J175537.50+662702.4 & 268.90628 &  66.45067 &   133.0 &     2.9 &   105.0 &     2.3 &    73.7 &     1.7 &    72.6 &     9.0 &   276.0 &    12.1 &   722.0 &    18.1 &   581.0 &    25.0 &   562.0 &    24.1 &   437.0 &    48.2  \\
  2140 & J175641.58+662704.5 & 269.17325 &  66.45126 &   151.0 &     3.4 &   132.0 &     3.0 &   101.0 &     2.3 &   124.0 &     9.4 &   580.0 &    16.4 &   996.0 &    21.2 &   881.0 &    27.0 &  1040.0 &    27.0 &  1090.0 &    60.2  \\
  2256 & J175652.48+662736.3 & 269.21869 &  66.46011 &   200.0 &     3.6 &   181.0 &     2.9 &   121.0 &     2.2 &   139.0 &     9.1 &   778.0 &    20.0 &  1260.0 &    22.4 &  1030.0 &    29.2 &  1080.0 &    26.1 &   998.0 &    56.8  \\
  2626 & J175721.13+663009.3 & 269.33805 &  66.50260 &    37.8 &     1.8 &    35.0 &     1.4 &    26.2 &     1.2 &     2.3 &     6.7 &    94.8 &    10.9 &   143.0 &    14.7 &   229.0 &    27.7 &   236.0 &    29.4 &   201.0 &    70.6  \\
  2633 & J175352.59+662951.3 & 268.46913 &  66.49761 &    81.7 &     2.4 &    66.6 &     1.9 &    48.0 &     1.5 &    27.1 &     8.3 &   149.0 &    10.0 &   290.0 &    17.3 &   154.0 &    25.4 &   220.0 &    22.8 &   130.0 &    48.0  \\
  2675 & J175325.50+662957.2 & 268.35625 &  66.49923 &    69.9 &     2.2 &    63.7 &     1.8 &    38.9 &     1.3 &    28.1 &     8.6 &    85.0 &     8.4 &   235.0 &    13.7 &   414.0 &    25.1 &   291.0 &    22.5 &   453.0 &    53.9  \\
  2734 & J175723.08+663038.5 & 269.34619 &  66.51071 &    85.7 &     2.6 &    68.1 &     2.1 &    50.1 &     1.7 &    49.6 &     8.4 &   218.0 &    12.9 &   409.0 &    15.8 &   321.0 &    27.6 &   376.0 &    29.4 &   238.0 &    69.1  \\
  2833 & J175346.60+663101.8 & 268.44418 &  66.51717 &    43.2 &     2.0 &    34.0 &     1.6 &    27.3 &     1.4 &    11.7 &     8.1 &    65.8 &     8.7 &   184.0 &    15.4 &   190.0 &    22.1 &   196.0 &    20.8 &   210.0 &    45.9  \\
  2960 & J175327.78+663138.8 & 268.36579 &  66.52745 &    78.2 &     2.5 &    69.8 &     2.0 &    44.3 &     1.5 &    13.9 &     8.5 &    79.4 &    12.1 &   224.0 &    16.0 &   151.0 &    21.6 &   168.0 &    21.0 &   146.0 &    44.1  \\
\hline
  3110 & J175331.90+663231.9 & 268.38295 &  66.54220 &    65.1 &     2.3 &    61.9 &     1.9 &    40.7 &     1.5 &    13.4 &     8.0 &    63.3 &    10.7 &   230.0 &    19.0 &   149.0 &    20.4 &   184.0 &    22.8 &   218.0 &    46.7  \\
  3387 & J175345.13+663405.1 & 268.43805 &  66.56809 &    52.5 &     2.5 &    44.4 &     2.2 &    31.3 &     1.7 &     9.7 &     8.5 &    93.6 &    11.8 &   250.0 &    19.4 &   174.0 &    24.0 &   134.0 &    20.3 &    33.7 &    45.4  \\
  3953 & J175456.90+664818.7 & 268.73711 &  66.80520 &    93.2 &     2.7 &    84.9 &     2.3 &    62.1 &     1.8 &    11.5 &     8.2 &   180.0 &    10.4 &   311.0 &    14.1 &   305.0 &    27.3 &   294.0 &    21.9 &   256.0 &    50.3  \\
  4359 & J175629.33+664530.6 & 269.12221 &  66.75850 &    52.4 &     2.7 &    64.0 &     2.2 &    49.7 &     1.7 &    17.5 &     8.7 &    24.3 &     8.5 &   198.0 &    12.5 &   383.0 &    33.5 &   185.0 &    30.5 &   482.0 &   111.0  \\
  4438 & J175319.00+664419.7 & 268.32918 &  66.73881 &   118.0 &     2.9 &   103.0 &     2.3 &    68.0 &     1.7 &    20.2 &     7.2 &   150.0 &    10.3 &   215.0 &    13.4 &   218.0 &    20.9 &   245.0 &    19.1 &   308.0 &    49.1  \\
  4454 & J175335.34+664522.4 & 268.39727 &  66.75624 &    72.0 &     2.7 &    67.1 &     2.1 &    47.9 &     1.7 &    20.8 &     7.7 &    89.8 &    11.1 &   203.0 &    14.0 &   251.0 &    21.9 &   270.0 &    19.2 &   268.0 &    48.1  \\
  4653 & J175645.64+664334.9 & 269.19020 &  66.72637 &    82.1 &     3.2 &    74.2 &     2.4 &    51.6 &     2.2 &    37.6 &     8.1 &   296.0 &    10.1 &   463.0 &    12.9 &   333.0 &    27.8 &   347.0 &    23.3 &   465.0 &    64.4  \\
  4802 & J175328.00+664228.0 & 268.36667 &  66.70779 &    66.5 &     2.3 &    67.2 &     2.2 &    43.9 &     2.0 &     8.9 &     6.6 &    60.5 &     9.2 &   200.0 &    11.2 &   245.0 &    19.8 &   132.0 &    17.7 &   143.0 &    44.7  \\
  5339 & J175651.89+664003.0 & 269.21623 &  66.66751 &    50.0 &     2.4 &    45.8 &     2.2 &    28.8 &     2.1 &     7.8 &     9.7 &    60.2 &    10.5 &   217.0 &    13.2 &   209.0 &    32.0 &   216.0 &    29.5 &   247.0 &    62.9  \\
  5424 & J175534.22+663918.4 & 268.89262 &  66.65512 &    53.7 &     2.0 &    65.1 &     1.9 &    50.2 &     1.4 &    42.7 &    11.4 &   136.0 &    12.7 &   538.0 &    19.1 &   487.0 &    35.9 &   522.0 &    47.6 &  1010.0 &    96.6  \\
  5776 & J175328.61+663701.4 & 268.36922 &  66.61707 &    53.6 &     2.0 &    48.8 &     1.8 &    31.0 &     1.4 &     3.2 &     7.0 &    75.2 &    10.8 &   162.0 &    16.3 &   200.0 &    19.8 &   195.0 &    18.2 &   250.0 &    47.6  \\
  6363 & J175701.56+665331.4 & 269.25654 &  66.89206 &    54.1 &     2.4 &    61.1 &     2.3 &    39.0 &     1.7 &     4.4 &     7.4 &    86.4 &     9.8 &   197.0 &    13.2 &   270.0 &    25.6 &   278.0 &    30.6 &   507.0 &    86.5  \\
  6393 & J175402.88+665222.2 & 268.51203 &  66.87284 &   257.0 &     4.5 &   229.0 &     3.3 &   174.0 &     2.8 &   176.0 &    10.2 &   828.0 &    11.9 &  1420.0 &    17.9 &  1190.0 &    29.8 &  1400.0 &    28.7 &  1780.0 &    62.0  \\
  6427 & J175430.88+665249.1 & 268.62869 &  66.88033 &   141.0 &     3.1 &   132.0 &     2.7 &    89.1 &     2.1 &    65.5 &     7.9 &   342.0 &     9.4 &   630.0 &    14.9 &   636.0 &    26.4 &   537.0 &    22.1 &   653.0 &    50.6  \\
  6449 & J175542.96+665248.9 & 268.92901 &  66.88027 &    37.2 &     1.9 &    39.3 &     1.7 &    27.6 &     1.4 &     7.5 &     7.8 &    72.5 &     8.4 &   213.0 &    12.5 &   232.0 &    28.0 &   274.0 &    23.5 &   426.0 &    57.9  \\
\hline
\end{tabular}
\tablefoot{Galaxies with ambiguous optical identification are excluded. Column~(1): AKARI mid-IR~source ID. Columns~(2): Source Name. Columns~(3) and (4): AKARI $N2$-band J2000.0 RA and Dec. Columns~(5) through (22): IRC~flux densities and errors. }
\end{table}