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Table 3.
Measured fluxes of circumnuclear dust components.
| λ | Fpolar | Fdisk | Funres. | fpolar | fdisk | funres. |
|---|---|---|---|---|---|---|
| [μm] | [Jy] | [Jy] | [Jy] | [%] | [%] | [%] |
| 8.5 ± 0.2 | 1.84 ± 0.07 | 0.46 ± 0.03 | 0.39 ± 0.01 | 42.5 ± 1.5 | 10.5 ± 0.6 | 9.0 ± 0.2 |
| 8.9 ± 0.2 | 1.18 ± 0.08 | 0.29 ± 0.04 | 0.36 ± 0.01 | 37.4 ± 2.5 | 9.2 ± 1.1 | 11.3 ± 0.4 |
| 9.7 ± 0.2 | 1.40 ± 0.16 | 0.28 ± 0.06 | 0.28 ± 0.02 | 48.6 ± 5.6 | 9.8 ± 2.1 | 9.6 ± 0.7 |
| 10.5 ± 0.3 | 3.28 ± 0.34 | 0.60 ± 0.09 | 0.29 ± 0.02 | 64.7 ± 6.6 | 11.8 ± 1.7 | 5.6 ± 0.4 |
| 11.3 ± 0.3 | 5.42 ± 0.42 | 1.00 ± 0.11 | 0.49 ± 0.03 | 63.9 ± 4.9 | 11.8 ± 1.3 | 5.7 ± 0.3 |
| 12.0 ± 0.2 | 7.79 ± 0.58 | 1.61 ± 0.17 | 0.77 ± 0.04 | 64.0 ± 4.8 | 13.2 ± 1.4 | 6.3 ± 0.3 |
| 12.7 ± 0.2 | 9.44 ± 0.93 | 2.04 ± 0.28 | 0.96 ± 0.07 | 61.5 ± 6.1 | 13.3 ± 1.8 | 6.3 ± 0.4 |
Notes. Aperture fluxes (left) and fractions of the total photometric flux (right) for the polar emission, disk, and unresolved component in each image reconstruction. Fractional values do not sum to 100% because some of the total flux is resolved out by the ≥30 m baselines.
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