Table 2
Mean microwave SED from Hi correlation.
| Frequency [GHz] | |||||||||||||
| Experiment | |||||||||||||
| 23 | 28.4 | 33 | 41 | 44.1 | 61 | 70.4 | 94 | 100 | 143 | 217 | 353 | ||
| Quantity | WMAP | LFI | WMAP | WMAP | LFI | WMAP | LFI | WMAP | HFI | HFI | HFI | HFI | |
|
|
|||||||||||||
| ϵH(ν) [μKRJ (1020 H cm-2)-1] ................... | 17. | 9.6 | 6.7 | 3.7 | 3.0 | 2.0 | 1.7 | 1.8 | 2.1 | 3.2 | 6.0 | 10.4 | |
| σstat [μKRJ (1020 H cm-2)-1] ................... | 1.4 | 0.92 | 0.60 | 0.38 | 0.31 | 0.23 | 0.17 | 0.26 | 0.087 | 0.12 | 0.19 | 0.31 | |
 [μKRJ (1020 H
cm-2)-1] ................... |
14. | 7.8 | 5.4 | 3.1 | 2.5 | 1.9 | 1.6 | 1.6 | 2.2 | 3.2 | 6.0 | 10.3 | |
 [μKRJ (1020 H
cm-2)-1] ................... |
1.2 | 0.72 | 0.64 | 0.42 | 0.34 | 0.27 | 0.20 | 0.27 | 0.11 | 0.12 | 0.19 | 0.31 | |
| u c K ...................................... | 1.01 | 0.92 | 1.03 | 1.04 | 1.06 | 1.10 | 1.15 | 1.26 | 1.26 | 1.69 | 2.99 | 13.3 | |
Notes.
ϵH and
Mean dust emissivity expressed as
monochromatic brightness at the reference frequencies from the correlation of the maps
with the Galactic Hi template alone, and with both the Galactic Hi template
and the 408 MHz map,
respectively. Not colour corrected. σstat and
Statistical uncertainty
(1σ) of
the brightness temperatures Tb and
. ucK ≡ Unit
conversion factors from brightness (Rayleigh-Jeans) to thermodynamic (CMB)
temperature. For WMAP the conversion factors are computed at the
reference frequency, while for Planck, they are computed assuming a
constant νIν
within the spectral band.
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