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Table 1

Sources of the data sets used in this paper, as well as their frequency, wavelength, resolution, calibration uncertainty, and rms on 5 scales (for data with 5 resolution or better only; see later).

Source ν [GHz] λ [mm] Res. Unc. σ (5, Jy) Analysis Reference

Haslam 0.408 734? 60.́ 10% ... L Haslam et al. (1982)
Dwingeloo 0.820 365? 72.́ 10% ... L Berkhuijsen (1972)
Reich 1.4 214? 35.́ 10% ... L Reich et al. (2001)
WMAP 9-year 22.8 13? 49.́ 3% ... L Bennett et al. (2013)
Planck 28.4 10.5 32.́24 3% ... L Planck Collaboration II (2014)
WMAP 9-year 33.0 9.0 40.́ 3% ... L Bennett et al. (2013)
WMAP 9-year 40.7 7.4 31.́ 3% ... L Bennett et al. (2013)
Planck 44.1 6.8 27.́01 3% ... L Planck Collaboration II (2014)
WMAP 9-year 60.7 4.9 21.́ 3% ... L Bennett et al. (2013)
Planck 70.4 4.3 13.́25 3% ... L Planck Collaboration II (2014)
WMAP 9-year 93.5 3.2 13.́ 3% ... L Bennett et al. (2013)
Planck 100? 3.0 9.́65 3% ... L Planck Collaboration VI (2014)
Planck 143? 2.1 7.́25 3% ... L Planck Collaboration VI (2014)
Planck 217? 1.38 4.́99 3% 0.015 LH Planck Collaboration VI (2014)
Planck 353? 0.85 4.́82 3% 0.05 LH Planck Collaboration VI (2014)
Planck 545? 0.55 4.́68 7% 0.13 LH Planck Collaboration VI (2014)
Herschel SPIRE PLW 600? 0.50 0.́59 4% 0.09 H Fritz et al. (2012)
Planck 857? 0.35 4.́33 7% 0.31 LH Planck Collaboration VI (2014)
Herschel SPIRE PMW 857? 0.35 0.́40 4% 0.23 H Fritz et al. (2012)
Herschel SPIRE PSW 1200? 0.25 0.́29 4% 0.29 H Fritz et al. (2012)
COBE-DIRBE 1249? 0.240 40.́ 13% ... L Hauser et al. (1998)
ISO 1763? 0.175 1.́3 10% 0.8 H Haas et al. (1998)
Spitzer MIPS B3 1870? 0.16 0.́63 12% 0.53 H Gordon et al. (2006), Bendo et al. (2012b)
Herschel PACS 1874? 0.16 0.́22 4% 2.4 H Fritz et al. (2012)
COBE-DIRBE 2141? 0.14 40.́ 13% ... L Hauser et al. (1998)
COBE-DIRBE 2997? 0.10 40.́ 13% ... L Hauser et al. (1998)
Herschel PACS 2998? 0.10 0.́21 4% 2.5 H Fritz et al. (2012)
IRAS (IRIS) B4 3000? 0.10 4.́3 13% 0.37 LH Miville-Deschênes & Lagache (2005)
Spitzer MIPS B2 4280? 0.07 0.́3 10% 0.12 H Gordon et al. (2006), Bendo et al. (2012b)
COBE-DIRBE 5000? 0.06 40.́ 13% ... L Hauser et al. (1998)
IRAS (IRIS) B3 5000? 0.06 4.́0 13% 0.12 LH Miville-Deschênes & Lagache (2005)
IRAS (IRIS) B2 12 000? 0.025 3.́8 13% 0.06 LH Miville-Deschênes & Lagache (2005)
Spitzer MIPS B1 12 490? 0.024 0.́1 4% 0.012 H Gordon et al. (2006), Bendo et al. (2012b)
IRAS (IRIS) B1 25 000? 0.012 3.́8 13% 0.04 LH Miville-Deschênes & Lagache (2005)
Spitzer IRAC 83 000? 0.0036 1.̋7 3% ... H Barmby et al. (2006), Spitzer Science Center (2012)

DRAO H i 1.4 ... 0.́37 5% ... H Chemin et al. (2009)
IRAM CO 115. ... 0.́38 15% ... H Nieten et al. (2006)

Notes. The Analysis column indicates whether the data set has been used in the 5 high-resolution (H) and/or 1° low-resolution (L) analysis. The first part of the table describes the continuum data sets, and the second part describes the spectral line data sets.

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