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Table 1

LAEs behind AS1063, see Table A.1 for quality flags and a cross correlation with multiple images.

ID RA (J2000) Dec (J2000) z

NE-91 342.19238 –44.52505 2.9760
SW-49a 342.17505 –44.54102 3.1169c,e
SW-49b 342.17315 –44.53999 3.1169abcef
SW-50 342.16225 –44.53829 3.1160
SW-68a 342.18745 –44.53869 3.1166ah
SW-68b 342.17886 –44.53587 3.1166ah
NE-93a 342.18283 –44.52028 3.1690
NE-93b 342.19196 –44.52409 3.1690
SW-51 342.17402 –44.54124 3.2275
NE-94a 342.18935 –44.51871 3.2857
NE-94b 342.19615 –44.52291 3.2857
NE-96 342.19709 –44.52483 3.4514
NE-97 342.19100 –44.52679 3.7131
SW-52a 342.18150 –44.53936 4.1130c
SW-52b 342.17918 –44.53870 4.1130c
NE-98a 342.19015 –44.53093 5.0510
NE-98b 342.19085 –44.53566 5.0510
NE-99a 342.18378 –44.52122 5.2373
NE-99b 342.18874 –44.52276 5.2373
NE-100 342.19701 –44.52212 5.8940
SW-53a 342.18106 –44.53462 6.1074bcg
SW-53b 342.19088 –44.53747 6.1074bcg
NE-118c 342.18402 –44.53159 6.1074
NE-118d 342.18904 –44.53004 6.1074

SW-70a 342.18586 –44.53883 3.6065
SW-70b 342.17892 –44.53668 3.6065

Notes. The last galaxy, SW-70, is no LAE, but a Lyman Break galaxy with minimal Lyα emission, and is therefore not considered in the remainder of this paper. Previous redshift determinations by:

(a)

C16;

(c)

Paper I;

(†)

NE-118 is the same image family as SW-53 but located in the NE rather than the SW. To avoid confusion with object NE-53, we listed the objects with the NE-118 identifier.

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