Table 4
Multi-wavelength photometry of H1429−0028.
| Survey/ | Filter | Total | Foreg. | Backg.a |
| facility | [μJy] | [μJy] | [μJy] | |
|
|
||||
| SDSS | u | <4.9 |
|
|
| g | 5.9 ± 0.8 |
|
|
|
| r | 20.5 ± 1.1 |
|
|
|
| i | 35.3 ± 1.9 |
|
|
|
| z | 61.9 ± 7.4 |
|
|
|
| VIKING | Z | 52.7 ± 3.1 |
|
|
| Y | 78.8 ± 5.9 |
|
|
|
| J | 133.9 ± 6.7 |
|
|
|
| H | 192 ± 12 | 134.8 ± 8.4 | 6.4 ± 0.6b | |
| K s | 380 ± 12 | 224.7 ± 6.9 | 17.4 ± 1.5b | |
| HST | F110W | 98.8 ± 4.2 | 78.1 ± 3.5 | 2.6 ± 0.3b |
|
|
||||
| Survey/ | Filter | Total | Foreg. | Backg. |
| facility | [mJy] | [mJy] | [mJy] | |
|
|
||||
| Spitzer | 3.6 μm | 0.614 ± 0.003 |
|
|
| 4.5 μm | 0.673 ± 0.004 |
|
|
|
| WISE | 3.4 μm | 0.558 ± 0.014 |
|
|
| 4.6 μm | 0.653 ± 0.020 |
|
|
|
| 12 μm | 5.39 ± 0.15 |
|
|
|
| 22 μm | 6.22 ± 0.76 |
|
|
|
| Herschel | 100 μm | 821 ± 28 |
|
|
| 160 μm | 1164 ± 32 |
|
|
|
| 250 μm | 778 ± 6 |
|
|
|
| 350 μm | 467.0 ± 7.0 |
|
|
|
| 500 μm | 227.0 ± 8.0 |
|
|
|
| IRAM-30 | 1.2 mm | 10.3 ± 2.5 |
|
|
| ALMA | 1.28 mm | 5.86 ± 0.99 |
|
0.543 ± 0.098c |
| 2.8 mm | 0.54 ± 0.11 |
|
|
|
| JVLA | 7 GHz | 0.91 ± 0.08 | <0.03 | 0.175 ± 0.023c |
Notes. Upper limits are set at the 3σ level.
Estimated via direct analysis of high-resolution HST F110W, Keck AO H and Ks imaging and demagnified by μ = 7.9 ± 0.8 in the former and μ = 8.9 ± 0.7 in the Keck bands.
Assumed to be equal to the total flux and demagnified by μ = 10.8 ± 2 at 1.28 mm and μ = 5.2 ± 0.5 at 7 GHz (Table 3).
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