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Table 4

Coefficients to estimate ki at 24 μm, 70 μm, 100 μm, and for TIR from luminosities in the NIR: ki = a + b × colour, with the colour in AB magnitudes.

IR band Colour a b σ ab Δki

24 FUVJ 16.429 ± 0.265 −2.122 ± 0.066 −0.017 0.000 ± 1.393
24 FUVH 16.236 ± 0.248 −2.005 ± 0.059 −0.014 0.000 ± 1.446
24 FUVK 15.332 ± 0.215 −1.923 ± 0.055 −0.011 0.000 ± 1.404
24 FUV3.6 15.044 ± 0.227 −2.169 ± 0.068 −0.015 0.000 ± 1.405

70 FUVJ 2.272 ± 0.145 −0.177 ± 0.035 −0.005 0.000 ± 0.339
70 FUVH 2.247 ± 0.143 −0.164 ± 0.033 −0.005 0.000 ± 0.340
70 FUVK 2.194 ± 0.132 −0.162 ± 0.033 −0.004 0.000 ± 0.340
70 FUV3.6 2.109 ± 0.122 −0.166 ± 0.035 −0.004 0.000 ± 0.347

100 FUVJ 1.770 ± 0.120 −0.163 ± 0.029 −0.003 0.000 ± 0.180
100 FUVH 1.752 ± 0.118 −0.153 ± 0.027 −0.003 0.000 ± 0.180
100 FUVK 1.695 ± 0.107 −0.149 ± 0.027 −0.003 0.000 ± 0.179
100 FUV3.6 1.632 ± 0.101 −0.157 ± 0.030 −0.003 0.000 ± 0.190

TIR FUVJ 1.012 ± 0.099 −0.098 ± 0.024 −0.002 0.000 ± 0.039
TIR FUVH 0.998 ± 0.097 −0.092 ± 0.023 −0.002 0.000 ± 0.043
TIR FUVK 0.961 ± 0.088 −0.089 ± 0.022 −0.002 0.000 ± 0.043
TIR FUV3.6 0.943 ± 0.083 −0.099 ± 0.025 −0.002 0.000 ± 0.041

Notes. The uncertainties on each coefficient are indicated along with the covariance σab. The last column indicates the mean offset and standard deviation between the measured ki and the estimation from the fit. The fitting procedure is carried out using the odr module of the python scipy package.

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