\begin{table}%t1
\tiny
\caption{\label{z2LyaCandidatesTable}Combined data list of $z\sim 2.2$ LAE candidates in the north-east half of the GOODS-North field.}
\par
%\centering
\par
\begin{tabular}{ccccccccccccccccc}
\hline\hline\noalign{\smallskip}
\tablefootmark{1}ID&RA&Dec&\tablefootmark{2}$z_{\rm phot}$&\tablefootmark{3}$z_{\rm spec}$&\tablefootmark{4}$EW$(Ly$\alpha$)$_{\rm rest}$&\tablefootmark{5}OFF-ON&\tablefootmark{6}ON&\tablefootmark{7}$\log L($Ly$\alpha$)&\tablefootmark{8}$F_{24~\mu{\rm m}}$&\tablefootmark{9}$F_{100~\mu{\rm m}}$&\tablefootmark{10}$F_{160~\mu{\rm m}}$&\tablefootmark{11}$R_{\rm isoph.}$&\tablefootmark{12}$n$&\tablefootmark{13}$R-K_{\rm s}$&\tablefootmark{14}$F_{\nu}(24~\mu{\rm m}$)/$F_{\nu}$(R)&\tablefootmark{15}Sp.~T.\\
\hline
ALH00228&12:37:36.1&+62:10:58&2.15&--&159.50~$\pm$~14.36&1.259~$\pm$~0.052&23.502~$\pm$~0.108&43.02&0.192~$\pm$~0.005&0.120~$\pm$~0.031&0.336~$\pm$~0.029&--&--&3.33~$\pm$~0.06&77.38~$\pm$~2.45&AGN/C\\
ALH02515&12:37:34.3&+62:13:21&2.12&--&274.96~$\pm$~23.21&1.731~$\pm$~0.237&24.793~$\pm$~0.206&42.79&--&--&--&1.92&3.8&4.08~$\pm$~0.07&--&AGN/C\\
ALH03537&12:38:04.4&+62:14:26&2.12&--&161.72~$\pm$~14.52&1.270~$\pm$~0.157&24.517~$\pm$~0.222&42.61&0.013~$\pm$~0.003&--&--&--&--&4.96~$\pm$~0.06&15.48~$\pm$~3.94&AGN/C\\
ALH03930&12:37:04.3&+62:14:47&2.13&2.21&297.24~$\pm$~24.94&1.802~$\pm$~0.088&23.393~$\pm$~0.076&43.40&0.198~$\pm$~0.003&0.124~$\pm$~0.023&--&1.79&1.9&5.08~$\pm$~0.06&517.75~$\pm$~45.69&AGN/C\\
ALH04281&12:37:52.6&+62:15:07&2.22&--&202.84~$\pm$~17.66&1.461~$\pm$~0.319&24.328~$\pm$~0.263&42.86&--&--&--&1.70&1.9&3.91~$\pm$~0.07&--&AGN/C\\
ALH05262&12:37:48.3&+62:16:10&2.29&--&149.09~$\pm$~13.57&1.204~$\pm$~0.219&24.552~$\pm$~0.261&42.63&0.019~$\pm$~0.003&--&0.079~$\pm$~0.018&1.32&1.4&3.23~$\pm$~0.14&174.82~$\pm$~39.80&AGN/C\\
ALH06146&12:37:14.9&+62:17:00&2.17&2.13&165.52~$\pm$~14.81&1.289~$\pm$~0.174&24.901~$\pm$~0.359&42.49&0.014~$\pm$~0.003&--&--&0.64&0.8&4.32~$\pm$~0.07&48.95~$\pm$~12.63&AGN/C\\
ALH06822&12:37:43.2&+62:17:46&2.35&--&131.25~$\pm$~12.23&1.103~$\pm$~0.122&24.893~$\pm$~0.219&42.44&--&--&--&1.04&1.2&2.24~$\pm$~0.16&--&SF\\
ALH07181&12:37:30.7&+62:18:05&2.08&--&75.64~$\pm$~8.17&0.712~$\pm$~0.068&23.612~$\pm$~0.144&42.46&--&--&--&4.98&0.7&4.87~$\pm$~0.03&--&AGN/C\\
ALH07955&12:37:26.1&+62:18:57&2.16&--&96.76~$\pm$~9.68&0.877~$\pm$~0.099&23.872~$\pm$~0.205&42.57&--&--&--&2.74&1.2&4.26~$\pm$~0.05&--&SF\\
ALH08364&12:37:02.1&+62:19:25&2.30&--&117.16~$\pm$~11.18&1.017~$\pm$~0.163&24.456~$\pm$~0.343&42.53&0.037~$\pm$~0.003&--&--&1.78&0.7&3.97~$\pm$~0.06&72.09~$\pm$~8.56&AGN/C\\
ALH09289&12:37:41.6&+62:20:28&2.08&--&98.82~$\pm$~9.83&0.892~$\pm$~0.120&24.341~$\pm$~0.216&42.36&--&--&--&--&--&--&--&AGN/C\\
ALH09753&12:37:34.3&+62:20:56&2.12&--&104.77~$\pm$~10.27&0.934~$\pm$~0.151&24.133~$\pm$~0.208&42.50&--&--&--&1.85&1.7&4.50~$\pm$~0.06&--&AGN/C\\
ALH09821&12:37:42.4&+62:21:02&2.26&--&92.53~$\pm$~9.37&0.846~$\pm$~0.168&24.393~$\pm$~0.258&42.38&--&--&--&1.66&7.6&5.03~$\pm$~0.06&--&SF\\
ALH10766&12:37:36.4&+62:22:01&2.28&--&251.40~$\pm$~21.39&1.649~$\pm$~0.325&24.949~$\pm$~0.331&42.76&--&--&--&1.49&1.2&--&--&SF\\
ALH11687&12:37:18.4&+62:23:00&2.31&--&115.63~$\pm$~11.07&1.007~$\pm$~0.132&24.266~$\pm$~0.247&42.60&0.256~$\pm$~0.004&--&--&0.89&1.8&3.81~$\pm$~0.09&670.84~$\pm$~62.20&AGN/C\\
\hline
\end{tabular}
\tablefoot{\tablefoottext{1}{ID from ALHAMBRA survey data.}\\
\tablefoottext{2}{Photometric redshift.}\\
\tablefoottext{3}{Spectroscopic redshift from Barger et~al. (\cite{barger08}).}\\
\tablefoottext{4}{Rest-frame equivalent width (\AA) of Ly$\alpha$ emission line from OFF-ON color and relation in Fig.~\ref{filter}.}\\
\tablefoottext{5}{OFF-ON color.}\\
\tablefoottext{6}{ON-band magnitude.}\\
\tablefoottext{7}{Logarithm of Ly$\alpha$ luminosity (erg s$^{-1}$).}\\
\tablefoottext{8}{Wavelength flux density in 24~$\mu{\rm m}$ band from MIPS ($\times$10$^{-18}$~erg~cm$^{-2}$~s$^{-1}$~\AA$^{-1}$).}\\
\tablefoottext{9}{Wavelength flux density in 100~$\mu{\rm m}$ band from HERSCHEL-PACS ($\times$10$^{-18}$~erg~cm$^{-2}$~s$^{-1}$~\AA$^{-1}$).}\\
\tablefoottext{10}{Wavelength flux density in 160~$\mu{\rm m}$ band from HERSCHEL-PACS ($\times$10$^{-18}$~erg~cm$^{-2}$~s$^{-1}$~\AA$^{-1}$).}\\
\tablefoottext{11}{Isophotal (2-$\sigma$) radius in kpc.}\\
\tablefoottext{12}{S\'ersic index.}\\
\tablefoottext{13}{Observed $R-K_{\rm s}$~color.}\\
\tablefoottext{14}{Ratio of $24~\mu{\rm m}$ to $R$-band frequency flux densities.}\\
\tablefoottext{15}{Spectral type from templates of Polletta et~al. \cite{polletta07}: star-forming (SF) or AGN/Composite (AGN/C).}\\
}
\end{table}