Table A.1.
Known 92 GHz emitters in the field of Cl1449, after correcting for the primary beam.
| ID ( * ) | RA | Dec | Flux | Flux error |
|---|---|---|---|---|
| deg | deg | μJy | μJy | |
| A1+B1 ( * *) | 222.30882 | 8.94054 | 26.5 | 3.6 |
| A5 | 222.30963 | 8.93690 | 56.1 | 4.0 |
| 6 ( * *) | 222.30991 | 8.93779 | 11.6 | 3.8 |
| BRG | 222.31526 | 8.94785 | 255.2 | 8.5 |
| A2 ( * *) | 222.30710 | 8.93951 | 10.3 | 3.6 |
| A3 | 222.30488 | 8.93820 | 14.6 | 4.0 |
| A4 | 222.30648 | 8.93778 | 19.0 | 3.9 |
| 13 ( * *) | 222.30856 | 8.94199 | 5.7 | 3.6 |
| N7+S7 ( * *) | 222.31025 | 8.93985 | 4.1 | 3.6 |
Notes. ( * )Identifiers in C18, except for BRG which denotes a bright, low-redshift radio galaxy outside the field of the data discussed in that paper. Given the lower resolution of our ALMA data, some close sources in C18 were merged for the purpose of 92 GHz subtraction. ( * *)Confirmed cluster members.
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