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Table A.2.
Frequencies and luminosity for computing the spectral energy distribution of DES0141−54 from radio to X-ray.
| log(νrest) | log(νLν) | Survey |
|---|---|---|
| (Hz) | (erg s−1) | |
| (1) | (2) | (3) |
| 8.66 | 43.89 ± 0.18 | GLEAM |
| 8.70 | 43.87 ± 0.15 | GLEAM |
| 8.74 | 43.91 ± 0.13 | GLEAM |
| 8.77 | 43.88 ± 0.17 | GLEAM |
| 8.81 | 44.00 ± 0.10 | GLEAM |
| 8.84 | 43.93 ± 0.10 | GLEAM |
| 8.86 | 43.90 ± 0.10 | GLEAM |
| 8.89 | 43.89 ± 0.10 | GLEAM |
| 8.93 | 43.99 ± 0.08 | GLEAM |
| 8.96 | 43.99 ± 0.07 | GLEAM |
| 8.98 | 44.05 ± 0.06 | GLEAM |
| 9.00 | 44.07 ± 0.07 | GLEAM |
| 9.02 | 44.09 ± 0.07 | GLEAM |
| 9.03 | 44.14 ± 0.05 | GLEAM |
| 9.05 | 44.10 ± 0.06 | GLEAM |
| 9.07 | 44.13 ± 0.06 | GLEAM |
| 9.08 | 44.14 ± 0.03 | GLEAM |
| 9.09 | 44.14 ± 0.05 | GLEAM |
| 9.10 | 44.16 ± 0.05 | GLEAM |
| 9.12 | 44.16 ± 0.05 | GLEAM |
| 9.13 | 44.15 ± 0.05 | GLEAM |
| 9.70 | 44.59 ± 0.03 | SUMSS |
| 10.46 | 45.01 ± 0.08 | ATPMN |
| 10.46 | 45.05 ± 0.05 | AT20G |
| 10.46 | 45.10 ± 0.09 | PMN |
| 10.70 | 45.11 ± 0.05 | CRATES |
| 10.71 | 45.15 ± 0.16 | ATPMN |
| 10.71 | 45.19 ± 0.06 | AT20G |
| 11.08 | 45.35 ± 0.05 | AT20G |
| 14.59 | 45.47 ± 0.31 | WISE |
| 14.73 | 45.83 ± 0.08 | WISE |
| 15.16 | 45.90 ± 0.29 | VHS |
| 15.25 | 45.75 ± 0.32 | DES |
| 15.26 | 45.99 ± 0.15 | DES |
| 15.36 | 46.09 ± 0.12 | DES |
| 15.44 | 45.45 ± 0.17 | DES |
| 18.46 | 44.79 ± 0.15 | XMM |
Notes. Column (1): logarithm of the rest-frame frequency in Hz; Col. (2): logarithm of the rest-frame νLν in erg s−1 with their errors; Col. (3): reference survey. We report the XMM-Newton point at 2 keV rest-frame.
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