Table A.1
Photometry of the 5σ ALMA detected sources combining HST, VLT, Spitzer and Herschel data.
| ID | F435W | F606W | F814W | F105W | F125W | F140W | F160W | K s | 3.6 μm | 4.5 μm | 5.8 μm | 8.0 μm | 24 μm | 100 μm | 160 μm | 250 μm | 350 μm | 500 μm |
|
|
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| A2744-ID01 | >29.04 | 28.24 | 27.52 | 26.41 | 25.63 | 25.01 | 24.44 | 23.07 | 22.22 | 21.83 | blended | blended | >18.7 | >15.4 | >14.5 | >13.8 | >13.4 | 13.39 |
| − | ±0.54 | ±0.14 | ±0.13 | ±0.12 | ±0.14 | ±0.12 | ±0.11 | ±0.05 | ±0.05 | − | − | − | − | − | − | − | ±0.26 | |
| A2744-ID02 | >28.49 | >29.75 | >30.09 | 26.09 | 25.32 | 24.61 | 24.17 | 24.21 | 22.66 | 22.30 | 21.13 | 21.04 | >18.3 | >15.4 | >14.5 | >13.7 | >13.3 | >13.6 |
| − | − | − | ±0.13 | ±0.12 | ±0.14 | ±0.12 | ±0.15 | ±0.50 | ±0.50 | ±0.50 | ±0.50 | − | − | − | − | − | − | |
| A2744-ID03 | >28.67 | 27.34 | 27.38 | 25.80 | 24.73 | 24.17 | 23.57 | 22.46 | >21.1 | >20.7 | >22.2 | >22.2 | >18.3 | >15.4 | >14.5 | >13.6 | >13.2 | >13.4 |
| − | ±0.22 | ±0.14 | ±0.13 | ±0.13 | ±0.12 | ±0.14 | ±0.06 | − | − | − | − | − | − | − | − | − | − | |
| A2744-ID04 | >28.51 | >27.8 | 23.99 | 22.93 | 22.49 | 22.24 | 21.97 | 21.28 | 20.63 | 20.25 | blended | blended | 18.26 | 13.38 | 12.36 | 12.76 | 12.53 | >12.92 |
| − | − | ±0.13 | ±0.13 | ±0.12 | ±0.14 | ±0.12 | ±0.09 | ±0.05 | ±0.05 | − | − | ±0.36 | ±0.06 | ±0.05 | ±0.21 | ±0.30 | − | |
| A2744-ID05 | >28.46 | >28.43 | >28.76 | 26.65 | 24.84 | 24.06 | 23.57 | 22.38 | 21.10 | 20.67 | blended | blended | >18.26 | >15.4 | >14.5 | >13.8 | >13.4 | >13.7 |
| − | − | − | ±0.13 | ±0.12 | ±0.14 | ±0.12 | ±0.08 | ±0.05 | ±0.05 | − | − | − | − | − | − | − | − | |
| A2744-ID06 | >29.81 | 26.75 | 25.77 | 23.57 | 22.81 | 22.39 | 22.08 | 21.06 | 20.65 | 19.87 | blended | blended | 17.54 | 14.74 | 14.24 | 12.32 | >12.61 | >12.95 |
| − | ±0.14 | ±0.22 | ±0.30 | ±0.12 | ±0.14 | ±0.12 | ±0.08 | ±0.05 | ±0.05 | − | − | ±0.19 | ±0.20 | ±0.28 | ±0.14 | − | − | |
| A2744-ID07 | >29.81 | >29.76 | >29.59 | 27.54 | 26.45 | 25.89 | 25.46 | 24.03 | 22.13 | 21.49 | blended | blended | 18.70 | >15.4 | >14.5 | >13.5 | >13.3 | >13.9 |
| − | − | − | ±0.15 | ±0.12 | ±0.14 | ±0.12 | ±0.20 | ±0.05 | ±0.05 | − | − | ±0.36 | − | − | − | − | − | |
|
|
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| M0416-ID01 | 22.72 | 22.53 | 22.22 | 22.09 | 21.86 | 21.65 | 21.46 | 20.82 | 20.06 | 19.95 | − | − | − | 14.12 | 13.41 | >13.6 | >13.4 | >13.4 |
| ±0.12 | ±0.12 | ±0.12 | ±0.12 | ±0.12 | ±0.12 | ±0.12 | ±0.05 | ±0.05 | ±0.05 | − | − | − | ±0.20 | ±0.23 | − | − | − | |
| M0416-ID02 | 26.15 | 24.96 | 24.20 | 23.17 | 22.52 | 22.23 | 22.01 | 21.12 | 21.04 | 20.55 | − | − | − | 14.78 | 13.67 | >13.6 | >13.4 | >13.5 |
| ±0.12 | ±0.12 | ±0.12 | ±0.12 | ±0.12 | ±0.12 | ±0.12 | ±0.05 | ±0.05 | ±0.05 | − | − | − | ±0.36 | ±0.29 | − | − | − | |
| M0416-ID03 | >29.30 | >29.20 | 27.02 | 24.25 | 23.67 | 23.35 | 23.22 | 21.89 | 20.52 | 20.63 | − | − | − | 14.39 | >13.9 | >13.5 | >13.4 | >13.6 |
| − | − | ±0.12 | ±0.12 | ±0.12 | ±0.12 | ±0.12 | ±0.05 | ±0.05 | ±0.05 | − | − | − | ±0.25 | − | − | − | − | |
| M0416-ID04 | 26.69 | 26.15 | 25.37 | 24.49 | 23.69 | 23.32 | 23.01 | 21.86 | 21.19 | 20.86 | − | − | − | >14.8 | >13.9 | >13.5 | >13.4 | >13.6 |
| ±0.12 | ±0.12 | ±0.12 | ±0.12 | ±0.12 | ±0.12 | ±0.12 | ±0.05 | ±0.05 | ±0.05 | − | − | − | − | − | − | − | − | |
|
|
||||||||||||||||||
| .M1149-ID01 | 24.21 | 23.38 | 22.48 | 21.46 | 21.03 | 20.83 | 20.66 | − | 19.56 | 19.41 | − | − | − | 15.21 | 14.13 | >13.3 | >13.4 | >13.7 |
| ±0.12 | ±0.12 | ±0.12 | ±0.12 | ±0.12 | ±0.12 | ±0.12 | − | ± 0.05 | ± 0.05 | − | − | − | ±0.30 | ±0.26 | − | − | − | |
Notes. AB magnitude photometry for the ALMA-FF sources. All the magnitudes have been aperture-corrected, are the observed magnitudes and represent the total flux associated with the source. Columns: (1) ID; (2), (3), (4), (5), (6), (7), (8) HST magnitudes measured on Frontier Fields images, with non-detections listed as 1 σ upper limits; (9) HAWK-I magnitudes; (10), (11), (12), (13), (14) IRAC and MIPS magnitudes, with non-detections listed as 1σ upper limits – if deblending was not possible, we adopt as an upper limit the flux measured at the position of the object; (15), (16), (17), (18), (19) Herschel magnitudes, with non-detections listed as 3σ upper limits, estimated by measuring the flux at the position of our objects.
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