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Table 1.

Main observational properties of the nine targets.

ID ID (Talia+21) RA Dec C20 Ks IRAC Ch 2
[hh:mm:ss] [dd:mm:ss] [mag] [mag]
RSN-41 COSMOSVLA3-49 09:58:17.869 +02:30:38.305 > 25.7 22.47 ± 0.04
RSN-84 COSMOSVLA3-106 09:58:43.440 +02:45:18.135 > 25.8 23.21 ± 0.07
RSN-121 COSMOSVLA3-152 09:59:14.234 +02:35:26.432 25.0 ± 0.3 22.54 ± 0.02
RSN-182 COSMOSVLA3-225 09:59:46.699 +02:48:41.215 > 25.0 23.29 ± 0.05
RSN-235 COSMOSVLA3-291 10:00:09.550 +01:42:50.834 > 26.2 23.40 ± 0.04
RSN-247 COSMOSVLA3-308 10:00:23.785 +01:41:59.273 24.9 ± 0.3 23.02 ± 0.03
RSN-298 COSMOSVLA3-370 10:00:57.970 +01:38:26.078 > 25.7 23.43 ± 0.04
RSN-361 COSMOSVLA3-442 10:01:28.390 +02:21:27.857 25.0 ± 0.3 23.84 ± 0.07
RSN-456 COSMOSVLA3-576 10:02:48.219 +02:24:30.629 > 25.7 22.97 ± 0.06

Notes. For each galaxy, we report the ID employed in Gentile et al. (2024) and throughout this paper. For completeness, we also report the original ID employed by Talia et al. (2021), which can be used to retrieve the observations from the ALMA science archive. Finally, we report the coordinates (of the radio counterpart, i.e., the counterpart with the higher spatial resolution) and a flag signaling whether each source has a counterpart in the COSMOS2020 catalog (Weaver et al. 2022).

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