Table A.1.
Far-IR to radio continuum fluxes for the nucleus of ESO 420-G13.
| Telescope/instrument | Frequency (Hz) | Flux (Jy) | Aperture | Ref. |
|---|---|---|---|---|
| PACS 70 μm | 4.2029 × 1012 | 17.1 ± 0.3 |
 |
(a) |
| PACS 100 μm | 2.9294 × 1012 | 20.8 ± 0.5 |
 |
(a) |
| PACS 160 μm | 1.8052 × 1012 | 16.2 ± 0.3 |
 |
(a) |
| SPIRE 250 μm | 1.19553 × 1012 | 6.43 ± 0.07 |
 |
(b) |
| SPIRE 350 μm | 8.56739 × 1011 | 2.44 ± 0.05 |
 |
(b) |
| SPIRE 500 μm | 5.87111 × 1011 | 0.76 ± 0.03 |
 |
(b) |
| ALMA 241 GHz | 2.41108 × 1011 | >1.7 × 10−3 | ∼27″ | (c) |
| ALMA 241 GHz | 2.41108 × 1011 | (340 ± 60)×10−6 |
 |
(c) |
| ALMA 227 GHz | 2.26605 × 1011 | >1.3 × 10−3 | ∼27″ | (c) |
| ALMA 227 GHz | 2.26605 × 1011 | (250 ± 40)×10−6 |
 |
(c) |
| VLA 1.4 GHz | 1.425 × 109 | (65 ± 2)×10−3 |
 |
(d) |
| SUMSS 843 MHz | 8.43 × 108 | (85 ± 3)×10−3 | – | (e) |
Notes. Flux measurements other than ALMA have been compiled from the literature and the NED database. The columns in the table correspond to the facility that was used for the continuum measurement, the observed frequency, the continuum flux density, the angular resolution of the observations, and the corresponding reference for the measurements. The largest angular scale in the ALMA maps is 
, thus the measured flux should be considered as a lower limit to the integrated flux within the FOV (27″).
References.
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