Table 4
Spectral fits of the mean microwave dust SED.
Model parameters | |||||||
AME | |||||||
Analytical model | Greybody | ||||||
|
BB | ||||||
Model | Tb(23 GHz) | ν p | − m60 | τ BB | σH(353 GHz) | β mm | χ2/ d.o.f. |
|
|||||||
1 ............... | 13.0 ± 1.1 × 10-20 | 11 ± 7 | 1.4 ± 0.7 | ... | 7.4 ± 0.23 × 10-27 | 1.52 ± 0.03 | 0.27 |
2 ............... | 12.6 ± 1.2 × 10-20 | 19 ± 6 | 2.2 ± 1.0 | 2.4 ± 0.51 × 10-28 | 7.3 ± 0.24 × 10-27 | 1.65 | 0.42 |
|
|||||||
SPDUST spectra | |||||||
|
|||||||
AWNM(23 GHz) | ACNM(41 GHz) | ν shift | |||||
|
|||||||
3 ............... | 12.8 ± 1.3 × 10-20 | 0.88 ± 0.26 × 10-20 | 25 ± 3 | ... | 7.4 ± 0.26 × 10-27 | 1.50 ± 0.04 | 0.21 |
4 ............... | 12.2 ± 1.2 × 10-20 | 0.71 ± 0.25 × 10-20 | 24.5 ± 3 | 2.4 ± 0.54 × 10-28 | 7.3 ± 0.26 × 10-27 | 1.65 | 0.34 |
Notes. Tb(23 GHz) ≡ Brightness temperature, in μK cm2 H-1, of AME at 23 GHz for models 1 and 2. νp and − m60 ≡ Peak frequency in gigahertz and slope at 60 GHz of AME spectrum in Eq. (10) for models 1 and 2. AWNM and ACNM ≡ Maximum brightness temperature of WNM and CNM SPDUST spectra, in μK cm2 H-1, for models 3 and 4. νshift ≡ Frequency shift in gigahertz of the CNM SPDUST spectrum for models 3 and 4. τBB ≡ Specific opacity of the blackbody component, in cm2H-1, for models 2 and 4. σH(353 GHz) ≡ Specific dust opacity at 353 GHz of greybody in cm2H-1. βmm ≡ Spectral index of the greybody component. The spectral index is fixed to 1.65 for models 2 and 4. The temperature is 19.8 K for the greybody and blackbody components for all models. χ2/ DOF ≡χ2 of the fit per degree of freedom.
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