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Table 2
Fitted 353GHz dust power spectra of the Planck data and of the dust model over SGC34, for which the mean dust intensity ⟨ D353 ⟩ is 54 ± 3kJysr-1.
| Parameter | Planck 353GHz data | Dust model |
|
|
||
| α EE | −2.37 ± 0.29 | −2.02 ± 0.26 |
| α BB | −2.33 ± 0.42 | −2.48 ± 0.38 |
| α TE | −2.07 ± 0.58 | −2.48 ± 0.25 |
|
|
||
| Assuming a common power law exponent αXX = −2.3 | ||
|
2.78 | 5.17 |
|
2.07 | 0.46 |
|
2.75 | 0.94 |
|
|
||
AEE [ ] |
17.21 ± 1.82 | 16.66 ± 1.59 |
| ABB [] |
8.85 ± 1.36 | 9.31 ± 1.23 |
| ATE [] |
36.95 ± 8.17 | 27.37 ± 2.76 |
|
|
||
| ⟨ ABB/AEE ⟩ | 0.51 ± 0.10 | 0.56 ± 0.09 |
| ⟨ ATE/AEE ⟩ | 2.18 ± 0.54 | 1.64 ± 0.23 |
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