Notes. High-fidelity (F≥90%) candidate list extracted via blind search using LINESEEKER. ⁽¹⁾Identifier of ALMA 1.2-mm continuum-selected candidates. ⁽²⁾Right Ascension (ICRS). ⁽³⁾Declination (ICRS). ⁽⁴⁾Flux density extracted from the source peak pixel in the 1.2 mm tapered continuum image. ⁽⁵⁾Signal-to-noise ratio. ⁽⁶⁾Fidelity and its uncertainties estimated by LINESEEKER using negative detections and Poisson statistics. All sources have a NIR counterpart, as revealed in HST/WFC3 F140W image, therefore, the actual fidelity should be considered F = 1. ⁽⁷⁾High-confidence redshift measurement from MUSE spectroscopic data. ^(†)Tentative redshift estimate measured from low-quality MUSE spectrum. ⁽⁸⁾Redshift measurement derived from emission lines detected with ALMA (see, also, Table 2, and Appendix B). ⁽⁹⁾Emission line detected in either ALMA band 6 data cube or band 3 spectral scans. ⁽¹⁰⁾Apparent AB magnitude in HST/WFC3 F140W filter. All reported uncertainties correspond to 1σ.