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Table 2.

New CANUCS systems of multiple images with spectroscopic redshifts.

Id RA Dec zniriss Class
C1.1 64.026343 −24.075524 2.91 [baseline=(X.base)] X) [draw, shape=circle, inner sep=0] g;
C1.2 64.038488 −24.083446 2.91

C2.1 64.037222 −24.082402 3.07 [baseline=(X.base)] X) [draw, shape=circle, inner sep=0] g;
C2.2 64.024868 −24.073494
C2.3 64.030749 −24.079544 3.07

C3.1 64.035827 −24.061968 [baseline=(X.base)] X) [draw, shape=circle, inner sep=0] g;
C3.2 64.042150 −24.065565
C3.3 64.046081 −24.070770 2.56

C4.1 64.035547 −24.081619 1.86 [baseline=(X.base)] X) [draw, shape=circle, inner sep=0] s;
C4.2 64.031217 −24.079546
C4.3 64.025491 −24.074159

Notes. Columns represent multiple-image IDs, their ICRS coordinates, NIRISS redshifts and their class (gold or silver, depending on their reliability). Grism redshift uncertainty is estimated as 0.005(1 + z) (see Sect. 2.2).

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