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Table A.3.

Díaz-Santos et al. (2016) and Díaz-Santos et al. (2018) list of two spectroscopically confirmed and potential companions in order of i-band magnitude from brightest to faintest found through deep ALMA observations.

LBG candidates Ra Dec rmag rmagerr imag imagerr zmag zmagerr
U1 341.5319518 −5.4427905 24.02 0.01 23.41 0.01 22.87 0.01
C3 341.5315566 −5.4424653 25.84 0.05 24.48 0.03 24.43 0.05
C2 341.5326256 −5.4440949 25.51 0.04 24.67 0.03 24.52 0.05
Knot 341.5322715 −5.4439102 25.13 0.03 24.92 0.04 24.58 0.05
U3 341.5300995 −5.4454121 25.77 0.05 25.42 0.07 24.58 0.09
U2 341.5303579 −5.4416845 26.64 0.11 25.59 0.08 25.52 0.13

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