Table B.1.
Total flux density of Fornax A.
| Frequency | Flux density (this work) | Flux density (McK) | Flux density (PeR) | Telescope/Reference |
|---|---|---|---|---|
| [GHz] | [Jy] | [Jy] | [Jy] | [−] |
| 4.70 × 10−3 | 13500±20% ( * ) | Ellis & Hamilton (1966) | ||
| 1.83 × 10−2 | 3500±20% | Shain & Higgins (1954) | ||
| 1.97 × 10−2 | 4300±20% | Shain (1958) | ||
| 2.99 × 10−2 | 2120±10% | Finlay & Jones (1973) | ||
| 8.40 × 10−2 | 788 ± 158 | 950±20% | MWA | |
| 0.118 | 692 ± 138 | MWA | ||
| 0.154 | 642 ± 125 | 750±19% | MWA | |
| 0.189 | 519±5% ( * ) | Bernardi et al. (2013) | ||
| 0.200 | 533 ± 107 | MWA | ||
| 0.232 | 416±5% | VLA | ||
| 0.246 | 433±5% | VLA | ||
| 0.275 | 395±5% | VLA | ||
| 0.296 | 366±5% | VLA | ||
| 0.312 | 346±5% | VLA | ||
| 0.320 | 343 ± 17 | VLA | ||
| 0.328 | 345±5% | VLA | ||
| 0.344 | 335±5% | VLA | ||
| 0.356 | 318±3% | VLA | ||
| 0.382 | 313±3% | VLA | ||
| 0.392 | 309±3% | VLA | ||
| 0.400 | 140±10% ( * ) | McGee et al. (1955) | ||
| 0.403 | 309±3% | VLA | ||
| 0.408 | 259±10% | Cameron (1971) | ||
| 0.421 | 294±3% | VLA | ||
| 0.437 | 283±3% | VLA | ||
| 0.456 | 274±3% | VLA | ||
| 0.470 | 275±3% | VLA | ||
| 0.600 | 310±25% | Piddington & Trent (1956) | ||
| 0.843 | 169±9% | Jones & McAdam (1992) | ||
| 1.03 | 163 ± 8 | MeerKAT | ||
| 1.42 | 125±8% | VLA | ||
| 1.44 | 128 ± 6 | MeerKAT | ||
| 1.50 | 121 ± 6 | 117±10% | VLA | |
| 2.70 | 98±10% | Shimmins (1971) | ||
| 5.00 | 54±5% | Gardner & Whiteoak (1971) | ||
| 5.70 | 44 ± 2 | SRT | ||
| 5.90 | 44 ± 2 | SRT | ||
| 6.10 | 44 ± 2 | SRT | ||
| 6.30 | 44 ± 2 | SRT | ||
| 6.50 | 43 ± 2 | SRT | ||
| 6.70 | 41 ± 2 | SRT | ||
| 6.87 | 39 ± 1 | SRT | ||
| 22.5 | 14±5% | WMAP( † ) | ||
| 30.0 | 8.5 ± 1.3 | 11±7% | Planck | |
| 32.8 | 9.4±6% | WMAP | ||
| 40.4 | 6.6±9% | Planck | ||
| 44.0 | 4.6 ± 0.7 | 6.1±20% | WMAP | |
| 60.4 | 4.7±15% | WMAP | ||
| 70.0 | 2.9 ± 0.5 | 3.0±17% | Planck | |
| 100 | 0.9 ± 0.4 | 1.2±25% | Planck | |
| 143 | 0.3 ± 0.5 | 0.29±51% | Planck | |
| 217 | (0.7) | Planck |
Notes. Column (1) shows the frequencies at which we measure the flux density of Fornax A. Column (2) shows the flux densities measured in this work. Column (3) shows the flux densities shown in McKinley et al. (2015). Column (4) shows the flux densities shown in Perley & Butler (2017). Column (5) indicates the telescope used for the measurements, or the reference to the published fluxes. ( * )indicates flux densities that have not been included in the study of the SED. ( † )WMAP: Wilkinson Microwave Anisotropy Probe (Bennett et al. 2013).
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