Table A.1.
Flux densities for known stellar sources from FULL9 dataset.
| Source | FluxFull9 | FluxDo10 | Notes |
|---|---|---|---|
| WR A | 0.48 ± 0.04 | 0.5 ± 0.06 | |
| 1.34 ± 0.09 | – | ||
| WR D | 0.34 ± 0.06 | – | |
| WR B | 3.24 ± 0.06c | – | Crowded |
| 9.50± 0.18t | 4.3 ± 0.4r | ||
| WR I | 0.45 ± 0.03 | – | Isolated |
| WR V | – | 0.4 ± 0.06 | Crowded |
| WR L | 0.40 ± 0.04 | 0.4 ± 0.06 | Isolated |
| WR S | 0.08 ± 0.03 | 0.3 ± 0.06 | |
| WR E | 0.11 ± 0.02 | – | Isolated |
| WR F | 0.34 ± 0.03 | 0.3 ± 0.06 | Isolated |
| WR M | 0.16 ± 0.04 | – | |
| W16a | 1.79 ± 0.09 | 1.6 ± 0.3 | Crowded |
| W12a | 1.66 ± 0.04c | – | |
| 3.28 ± 0.08 | 2.9 ± 0.3r | ||
| W4a | 1.79 ± 0.04c | 0.8 ± 0.08 | |
| 4.19 ± 0.11t | 2.2 ± 0.2r | ||
| W32 | 0.16 ± 0.04 | 0.4 ± 0.06 | Crowded |
| W265 | 0.94 ± 0.06c | – | Isolated |
| 2.72 ± 0.16t | 2.3 ± 0.3r | ||
| W237 | 1.26 ± 0.04c | 1.8 ± 0.2 | Isolated |
| 7.01 ± 0.22t | 5.6 ± 2.2r | ||
| W75 | 0.26 ± 0.04 | 0.3 ± 0.06 | Isolated |
| W20 | 2.39 ± 0.05c | – | |
| 16.62 ± 0.27t | 3.8 ± 0.4r | ||
| W26 | 152.15 ± 0.33 | 20.1 ± 2.0r | |
| W17 | 0.98 ± 0.05 | – | Crowded |
| 1.27 ± 0.07 | 1.7 ± 0.2 | ||
| W243 | 1.65 ± 0.05 | 1.5 ± 0.2 | Isolated |
| W9 | 30.47 ± 0.09c | 24.9 ± 2.5 | Crowded |
| 80.8 ± 0.5t | 30.5 ± 3.0r | ||
| D09-R1 | 1.20 ± 0.04c | 0.7 ± 0.07 | Crowded |
| 4.66 ± 0.14t | 6.5 ± 1.2r | ||
| D09-R2 | 0.88 ± 0.08 | 0.7 ± 0.06 | Crowded |
| W15 | 0.84 ± 0.10 | 0.6 ± 0.06 | |
Notes. Fluxes are taken from FULL9 dataset, measured with SEAC, assuming σf = 3, σs = 5, with consideration of segmentation where necessary. Flux densities are given in mJy. Core and total flux densities are given for relevant sources, noted by c, t respectively. Flux density values are compared to fluxes found in D10, at 8.6 GHz, where the superscript r refers to objects that were found to be spatially resolved.
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