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Table 1

Mean SED of dust emissivity from Hi correlation.

Frequency [GHz]
Experiment

70 94 100 143 217 353 545 857 1249 2143 2997
Quantity LFI WMAP HFI HFI HFI HFI HFI HFI DIRBE DIRBE DIRBE

ϵH(ν) [MJy sr-1(1020 H cm-2)-1] ... 0.00027 0.00045 0.00067 0.0020 0.0086 0.039 0.14 0.43 0.84 1.1 0.63
σstat [MJy sr-1(1020 H cm-2)-1] .... 2.8 × 10-5 8.9 × 10-5 2.8 × 10-5 7.9 × 10-5 3.0 × 10-4 0.0013 0.0045 0.013 0.027 0.048 0.022
photunc [%] ............. 0.5 0.2 0.5 0.5 0.5 1.2 10.0 10.0 11.6 10.6 13.6
σtot [MJy sr-1(1020 H cm-2)-1] .... 2.8 × 10-5 8.9 × 10-5 2.8 × 10-5 7.9 × 10-5 3.0 × 10-4 0.0014 0.015 0.045 0.10 0.13 0.088
cc ...................... 0.96 0.98 1.09 1.02 1.12 1.11 1.10 1.02 1.00 0.94 0.92
uc ..................... 7.54 4.63 4.10 2.69 2.07 3.48 ... ... ... ... ...

Notes. ϵH(ν) ≡ Mean dust emissivity ϵH(ν) expressed as monochromatic brightness at the reference frequencies, derived from correlation of the maps with the Galactic Hi template. Not colour corrected. σstat Statistical uncertainty (1σ) of the mean emissivities. photunc (%) ≡ Uncertainties of the absolute calibration [%] from Planck Collaboration I (2014), Bennett et al. (2013), and Hauser et al. (1998). σtot Total uncertainty combining statistical and photometric uncertainties [MJy sr-1 per 1020 H cm-2]. cc ≡ Colour-correction factors in Eq. (8) computed with the greybody parameters listed in Table 3. uc ≡ Unit conversion factors from MJy sr-1 to thermodynamic (CMB) temperatures in mK.

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