Table 1
Multi-wavelength SED of z1 (Col. 3) and Y5 (Col. 4).
| Band/instrument | λeff [μm] | z1 | Y5 |
|
|
|||
| I | 0.79 | < 3.6e-5 | < 3.6e-5 |
| z | 0.92 | < 1.4e-4 | < 1.4e-4 |
| Y | 1.02 | (2.0 ± 0.3)e-4 | < 6.3e-5 |
| J | 1.26 | (1.75 ± 0.05)e-3 | (6.9 ± 0.5)e-4 |
| H | 1.63 | (1.33 ± 0.07)e-3 | (9.3 ± 0.03)e-4 |
| Ks | 2.15 | (2.29 ± 0.06)e-3 | (1.77 ± 0.07)e-3 |
| IRAC | 3.6 | (6.98 ± 0.06)e-3 | (2.91 ± 0.11)e-3 |
| 4.5 | (10.20 ± 0.09)e-3 | (3.73 ± 0.10)e-3 | |
| 8.0 | (9.91 ± 0.96)e-3 | ||
| MIPS | 24 | 0.340 ± 0.040 | |
| PACS | 100 | < 3.3 | < 18 |
| 160 | 6.3 ± 2.0 | < 30 | |
| SPIRE | 250 | 19.4 ± 1.6 | 45.5 ± 1.6 |
| 350 | 15.7 ± 1.4 | 30.3 ± 1.2 | |
| 500 | 7.5 ± 1.7 | 19.4 ± 2.1 | |
| LABOCA | 870 | < 2.5 | 1.8 ± 1.0 |
| VLA | 2.1 × 105 | < 0.14 | < 0.14 |
Notes. Optical and IR photometry (rows 1–10) is taken from Laporte et al. (2011). Upper limits are 3σ. Rows 12–17 give the Herschel and LABOCA source flux. When the measured flux (not the estimated flux) is < 2.5σ the 3σ value is given as an upper limit. No entry indicates the lack of data. All fluxes are given in milli-Jansky.
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