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Table B.1:

Combined data list of $z\sim 2.2$ LAE candidates in the north-east half of the GOODS-North field.

1ID 		RA Dec 2 $z_{\rm phot}$ 3 $z_{\rm spec}$ 4EW(Ly$\alpha $) $_{\rm rest}$ 5OFF-ON 6ON 7$\log L($Ly$\alpha $) 8 $F_{24~\mu{\rm m}}$ 9 $F_{100~\mu{\rm m}}$ 10 $F_{160~\mu{\rm m}}$ 11 $R_{\rm isoph.}$ 12n 13 $R-K_{\rm s}$ 14 $F_{\nu}(24~\mu{\rm m}$)/$F_{\nu}$(R) 15Sp. T.
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

Notes. (1) ID from ALHAMBRA survey data.
(2) Photometric redshift.
(3) Spectroscopic redshift from Barger et al. (2008).
(4) Rest-frame equivalent width (Å) of Ly$\alpha $ emission line from OFF-ON color and relation in Fig. A.1.
(5) OFF-ON color.
(6) ON-band magnitude.
(7) Logarithm of Ly$\alpha $ luminosity (erg s-1).
(8) Wavelength flux density in 24  $\mu{\rm m}$ band from MIPS ($\times$10-18 erg cm-2 s-1 Å-1).
(9) Wavelength flux density in 100  $\mu{\rm m}$ band from HERSCHEL-PACS ($\times$10-18 erg cm-2 s-1 Å-1).
(10) Wavelength flux density in 160  $\mu{\rm m}$ band from HERSCHEL-PACS ($\times$10-18 erg cm-2 s-1 Å-1).
(11) Isophotal (2-$\sigma $) radius in kpc.
(12) Sérsic index.
(13) Observed $R-K_{\rm s}$ color.
(14) Ratio of $24~\mu{\rm m}$ to R-band frequency flux densities.
(15) Spectral type from templates of Polletta et al. 2007: star-forming (SF) or AGN/Composite (AGN/C).


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