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Table 2

Results from fitting Eq. (1) to the colour ratio data, including the covariance terms between the fitted parameters.

Ratio α A1 A2 ESF/ETotal Cov(α, A1) Cov(α, A2) Cov(A1, A2) C(3.6) C(24)
SP545/SP353 0.071 ± 0.01 ... 1.25 ± 0.01 0 ... −4.7 × 10-5 ... 0.85 0.51
SP857/SP545 0.103 ± 0.018 ... 1.10 ± 0.01 <0.13 ... −9.3 × 10-5 ... 0.86 0.71
SH857/SH600 0.085 ± 0.009 2.40 0.77 ± 0.04 0.19 ± 0.12 −0.0069 5.7 × 10-5 −0.096 0.88 0.57
SH1200/SH857 0.108 ± 0.008 2.04 0.54 ± 0.04 0.22 ± 0.09 −0.0048 8.3 × 10-5 −0.058 0.90 0.61
SH1874/SH1200 0.180 ± 0.013 1.82 0.06 ± 0.05 0.23 ± 0.08 −0.0063 0.00022 −0.047 0.85 0.61
SH3000/SH1870 0.30 ± 0.03 0.69 −0.95 ± 0.04 0.44 ± 0.07 −0.0039 0.00036 −0.0076 0.66 0.62
SS4280/SH3000 0.37 ± 0.04 0.077 −1.35 ± 0.02 0.85 ± 0.04 −0.00049 0.00015 −0.00052 0.34 0.65
SP545/SP353 0.063 ± 0.014 ... 1.27 ± 0.01 0 ... −5.0 × 10-5 ... 0.85 0.52
SP857/SP545 0.102 ± 0.018 ... 1.10 ± 0.01 <0.15 ... −9.3 × 10-5 ... 0.86 0.71
SH857/SH600 0.095 ± 0.009 2.40 0.77 ± 0.04 0.19 ± 0.12 −0.0075 6.1 × 10-5 −0.093 0.88 0.57
SH1200/SH857 0.108 ± 0.008 2.04 0.54 ± 0.04 0.22 ± 0.09 −0.0048 8.3 × 10-5 −0.058 0.90 0.61
SH1874/SH1200 0.180 ± 0.013 1.82 0.06 ± 0.05 0.23 ± 0.08 −0.0063 0.00022 −0.047 0.85 0.61
SH3000/SH1870 0.30 ± 0.03 0.69 −0.95 ± 0.04 0.44 ± 0.07 −0.0039 0.00036 −0.0076 0.66 0.62
SS4280/S H3000 0.37 ± 0.04 0.077 −1.35 ± 0.02 0.85 ± 0.04 −0.00049 0.00015 −0.00052 0.34 0.65
SP545/SP353 0.071 ± 0.014 ... −0.28 ± 0.18 0 ... −4.9 × 10-5 ... 0.85 0.38
SP857/SP545 0.101 ± 0.017 ... 0.36 ± 0.69 <0.13 ... 0.00421 ... 0.86 0.60
SH857/SH600 0.085 ± 0.009 1.71 0.80 ± 0.05 0.16 ± 0.11 −0.0056 1.4 × 10-4 −0.074 0.88 0.46
SH1200/SH857 0.109 ± 0.009 1.27 0.59 ± 0.05 0.21 ± 0.09 −0.0048 1.8 × 10-4 −0.054 0.90 0.50
SH1874/SH1200 0.183 ± 0.014 1.05 0.16 ± 0.05 0.24 ± 0.08 −0.0047 0.00041 −0.027 0.85 0.51
SH3000/SH1870 0.31 ± 0.03 0.38 −0.77 ± 0.05 0.44 ± 0.06 −0.0021 0.00076 −0.0049 0.66 0.56
SS4280/SH3000 0.39 ± 0.05 0.055 −1.34 ± 0.04 0.81 ± 0.04 −0.00030 0.00013 −0.00046 0.34 0.41

Notes. Upper limits are 1σ. The last two columns are the correlation coefficients (C) from Fig. 7. Top: using SMICA CMB subtraction. Middle: using NILC CMB subtraction. Bottom: using the combination of 24 μm and FUV emission as the star-formation tracer, with SMICA CMB subtraction. Planck data are marked by “P,” Herschel data by “H,” and Spitzer data by “S.”

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