Table 2: Photometric and spectroscopic properties of the 15 LAE candidates. The limits of the narrow-band photometry correspond to the limiting magnitude (3$\sigma $ in 2 $^{\prime \prime }$ diameter aperture).
No. RA Dec mag $_{\rm {810}}$ mag $_{\rm {815}}$ mag $_{\rm {823}}$ Flux $_{\rm {phot}}$ EW [Å] $z_{\rm {spec}}$ Flux $_{\rm {spec}}$
            [10-21 W m-2]     [10-21 W m-2]

1		 1:05:50.36 -25:46:31.30 >26.35 >26.46 25.03 $\pm$ 0.11 5.41 $\pm$ 0.55 >70.1 5.780 8.36 $\pm$ 0.83
2 1:05:51.06 -25:43:21.50 25.28 $\pm$ 0.16 24.75 $\pm$ 0.09 >26.48 5.02 $\pm$ 0.37 >99.5 - -
3 1:05:52.24 -25:47:10.24 >26.35 >26.46 25.12 $\pm$ 0.14 4.98 $\pm$ 0.64 > 61.8 5.770 2.41$\pm$ 0.49
4 1:05:52.45 -25:43:52.50 >26.35 >26.46 24.61 $\pm$ 0.10 7.97 $\pm$0.73 >131.5 -  
5 1:05:53.42 -25:44:26.42 >26.35 >26.46 24.88 $\pm$ 0.10 6.22 $\pm$ 0.57 >86.9 - -
6 1:05:54.94 -25:48:25.08 >26.35 >26.46 25.14 $\pm$ 0.15 4.89 $\pm$ 0.68 >60.1 5.787 8.17 $\pm$ 1.02
7 1:05:58.45 -25:42:41.17 24.73 $\pm$ 0.10 >26.46 >26.48 9.02 $\pm$ 0.83 >161.4 - -
8 1:05:59.27 -25:49:20.37 24.82 $\pm$ 0.11 >26.46 >26.48 8.30 $\pm$ 0.84 >138.0 5.627 4.79$\pm$ 0.56
9 1:06:01.46 -25:44:25.45 25.16 $\pm$ 0.13 >26.46 >26.48 6.07 $\pm$ 0.73 >80.7 - -
10 1:06:06.05 -25:43:17.68 >26.35 >26.46 25.69 $\pm$ 0.19 2.95 $\pm$ 0.52 >28.4 - -
11 1:06:07.82 -25:48:49.86 >26.35 >26.46 25.07 $\pm$ 0.13 5.22 $\pm$ 0.62 >66.3 5.758 1.13 $\pm$ 0.33
12 1:06:07.93 -25:43:17.47 >26.35 24.26 $\pm$ 0.05 >26.48 10.59 $\pm$ 0.49 >230.1 - -
13 1:06:08.88 -25:48:37.24 25.92 $\pm$ 0.13 24.83 $\pm$ 0.11 >26.48 6.26 $\pm$ 0.63 >88.4 5.679 4.37 $\pm$ 0.50
14 1:06:09.38 -25:48:20.32 >26.35 >26.46 25.00 $\pm$ 0.15 5.57 $\pm$ 0.77 >73.1 5.764 4.05 $\pm$ 0.54
15 1:06:16.29 -25:48:06.58 24.1 $\pm$ 0.05 >26.46 >26.48 16.12 $\pm$ 0.74 >872.4 5.640 11.99 $\pm$ 0.72


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