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Table 2
Flux densities for AME-G160.26 − 18.62 in the Perseus molecular cloud and residual fluxes when free-free, CMB and thermal dust components are removed.
| Frequency | Flux density | Flux density residual |
| [GHz] | [Jy] | [Jy] |
|
|
||
| 0.408 | 9.7 ± 3.3 | 0.2 ± 3.4 |
| 0.82 | 9.4 ± 4.7 | 0.5 ± 4.8 |
| 1.42 | 8.0 ± 1.7 | − 0.5 ± 1.8 |
| 10.9 | 16.1 ± 1.8 | 9.4 ± 2.0 |
| 12.7 | 20.0 ± 2.2 | 13.3 ± 2.4 |
| 14.7 | 28.4 ± 3.1 | 21.8 ± 3.3 |
| 16.3 | 35.8 ± 4.0 | 29.3 ± 4.2 |
| 22.8 | 39.8 ± 4.2 | 33.4 ± 4.5 |
| 28.5 | 38.1 ± 4.0 | 31.5 ± 4.4 |
| 33.0 | 36.7 ± 3.9 | 29.7 ± 4.4 |
| 40.9 | 30.8 ± 3.3 | 22.6 ± 4.0 |
| 44.1 | 28.5 ± 3.2 | 19.6 ± 4.0 |
| 61.3 | 27.4 ± 3.4 | 10.9 ± 6.4 |
| 70.3 | 32.2 ± 3.9 | 8.9 ± 9.0 |
| 93.8 | 63.0 ± 7.8 | 7 ± 21 |
| 100 | 78 ± 15 | 10 ± 29 |
| 143 | 202 ± 22 | − 25 ± 80 |
| 217 | 1050 ± 130 | 120 ± 320 |
| 353 | 3860 ± 470 | − 600 ± 1400 |
| 545 | 15300 ± 2100 | −800 ± 4900 |
| 857 | 48700 ± 6100 | −1000 ± 14000 |
| 1250 | 93000 ± 13000 | −2400 ± 28000 |
| 2143 | 117000 ± 15000 | 7000 ± 35000 |
| 2997 | 53600 ± 6700 | −2000 ± 20000 |
Notes. The fitted spinning dust model consists of two components.
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