Table A.2: Candidate Ly$\alpha $ emitters with EW0 > 15 Å and $\Sigma > 3$.
ID Coordinates B EW0 $\Sigma $ $F_{\rm Ly\alpha}$
(1) (2) (3) (4) (5) (6)
28 11:40:50.8 -26:32:26.0 26.1 97.8 4.3 5.3
46 11:40:33.9 -26:32:13.4 25.5 31.6 3.7 3.4
54 11:40:37.1 -26:32:08.3 24.5 24.2 5.6 7.1
73 11:40:37.8 -26:31:55.5 25.7 34.5 3.6 3.1
127 11:40:48.2 -26:31:32.4 25.5 18.9 3.3 2.2
146 11:40:47.4 -26:31:22.6 25.6 26.0 3.5 2.6
184 11:40:36.6 -26:31:04.1 24.9 22.5 4.4 4.4
238 11:40:55.3 -26:30:43.5 26.5 97.5 3.7 3.4
286 11:40:47.9 -26:30:31.5 27.5 265.0 3.1 2.6
297 11:40:54.9 -26:30:29.8 27.5 497.6 3.8 3.4
301 11:40:45.2 -26:30:27.7 27.4 139.9 4.0 2.0
361 11:40:36.9 -26:30:08.8 25.0 23.6 3.8 4.3
365 11:40:58.1 -26:30:09.4 25.0 21.8 3.5 3.7
366 11:40:51.6 -26:30:08.0 25.0 29.5 4.1 5.0
417 11:40:45.3 -26:29:49.1 24.7 18.9 3.8 4.6
441 11:40:57.4 -26:29:38.3 24.9 83.9 4.9 13.5
465 11:40:48.0 -26:29:37.0 26.8 119.2 3.5 3.2
470 11:40:59.7 -26:29:35.0 25.8 49.9 4.2 3.9
479 11:40:51.0 -26:29:31.1 25.3 25.0 3.3 3.3
484 11:40:45.5 -26:29:30.0 27.5 96.6 3.0 1.4
a491 11:40:48.2 -26:29:09.5 21.6 108.4 68.3 341.9
a515 11:40:48.5 -26:29:07.3 22.7 48.9 23.9 64.3
522 11:40:49.4 -26:29:09.6 23.7 36.0 8.6 20.0
561 11:40:46.2 -26:29:03.2 27.5 9749.7 7.4 6.8
565 11:40:56.6 -26:26:13.6 25.3 28.2 3.0 3.9
674 11:40:46.0 -26:28:35.7 27.5 269.4 3.4 2.6
675 11:40:55.3 -26:28:24.3 26.8 117.8 3.9 3.1
703 11:40:43.7 -26:28:21.8 26.4 86.7 3.4 3.4
728 11:40:36.9 -26:28:03.3 23.7 20.2 7.1 11.9
739 11:40:57.4 -26:27:07.8 24.4 20.6 4.5 6.3
b778 11:41:02.4 -26:27:45.1 24.1 314.2 27.4 67.6
877 11:40:54.0 -26:28:01.1 25.3 31.6 3.4 4.3
891 11:40:59.1 -26:28:10.5 25.0 25.4 4.4 4.7
941 11:40:44.0 -26:28:33.5 25.6 32.0 3.1 3.3
942 11:40:49.8 -26:28:29.0 26.2 55.3 3.3 2.9
c968 11:40:39.8 -26:28:45.4 24.2 26.6 8.6 9.8
a971 11:40:47.8 -26:29:08.2 25.5 334.6 10.6 19.2
980 11:40:42.3 -26:28:51.3 26.3 113.1 3.7 4.7
1009 11:40:49.5 -26:29:11.1 25.1 57.1 5.9 8.5
1017 11:40:48.3 -26:29:01.7 24.2 68.2 8.7 21.5
Notes: (1) Catalog number; (2) right ascension and declination in J2000 coordinates; (3) B band magnitude; (4) rest frame equivalent width; (5) significance of excess flux; (6) continuum subtracted narrow band flux in 10-17 erg cm -2 s-1. Notes to individual objects: a Inside Ly$\alpha $ halo of PKS 1138-262, b QSO described in Sect. 5.4, c QSO discovered in Paper II.

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