Table 6: Cross-correlation results of CMB data with dust. Available cross-correlation coefficients of CMB data sets with dust templates at 100  m.

Experiment Frequency (GHz) K/(MJy·sr−1) References

COBE DMR 31.5 20 Kogut et al. [37]
COBE DMR 31.5 30 Kogut et al. [37]
COBE DMR 53.0 20 Kogut et al. [37]
COBE DMR 53.0 30 6.4 ± 3.4 Kogut et al. [37]
COBE DMR 90.0 20 Kogut et al. [37]
COBE DMR 90.0 30 Kogut et al. [37]

Saskatoon (Ka band) 30.0 NCP De Oliveira-Costa et al. [25, 26]
Saskatoon (Q band) 40.0 NCP De Oliveira-Costa et al. [25, 26]

19 GHz survey 19.0 20 De Oliveira-Costa et al. [27, 28]
19 GHz survey 19.0 30 De Oliveira-Costa et al. [27, 28]

OVRO 14.5 NCP Leitch et al. [1, 2]
OVRO 32.0 NCP Leitch et al. [1, 2]

PYTHON V 40.3 Coble et al. [38]

Tenerife 10.0 20 De Oliveira-Costa et al. [29, 30]
Tenerife 10.0 30 De Oliveira-Costa et al. [29, 30]
Tenerife 10.0 40 De Oliveira-Costa et al. [29, 30]
Tenerife 15.0 20 De Oliveira-Costa et al. [29, 30]
Tenerife 15.0 30 De Oliveira-Costa et al. [29, 30]
Tenerife 15.0 40 De Oliveira-Costa et al. [29, 30]

Tenerife 10.0 20 Mukherjee et al. [39]
Tenerife 10.0 30 Mukherjee et al. [39]
Tenerife 10.0 40 Mukherjee et al. [39]
Tenerife 15.0 20 Mukherjee et al. [39]
Tenerife 15.0 30 Mukherjee et al. [39]
Tenerife 15.0 40 Mukherjee et al. [39]

South Pole 94 30.0 40 Hamilton and Ganga [40]
South Pole 94 40.0 40 Hamilton and Ganga [40]