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Table 27.

MIR luminosity data.

Source W1 δW1 W2 δW2 W3 δW3 W4 δW4 log L12 μm
m3.4 μm m4.6 μm m12 μm m22 μm
H011A 11.575 0.006 10.301 0.006 6.232 0.006 2.786 0.006 44.19
L024A 12.188 0.009 11.417 0.010 6.949 0.008 3.591 0.011 44.24
L084B 11.810 0.006 10.644 0.007 6.880 0.007 3.795 0.010 44.88
L097A 11.423 0.006 11.064 0.007 6.736 0.006 4.270 0.010 43.92
L115A 11.580 0.006 11.405 0.008 7.863 0.011 4.870 0.017 43.63
L115B 11.200 0.006 10.850 0.006 6.843 0.007 4.485 0.012 44.05
L125B 12.172 0.008 11.679 0.014 7.170 0.008 4.055 0.011 43.77
L127A 12.744 0.009 12.410 0.016 8.006 0.013 4.530 0.015 43.53
L127B 12.267 0.009 11.676 0.011 7.200 0.008 4.327 0.013 43.88
L156A 11.196 0.006 10.800 0.007 6.551 0.006 3.813 0.010 44.04
L156B 11.196 0.006 10.800 0.007 6.551 0.006 3.813 0.010 44.04
L170B 11.019 0.006 10.326 0.006 5.627 0.005 2.163 0.006 44.25
L207A 11.431 0.007 11.075 0.007 7.303 0.008 4.907 0.025 43.70
L207B 11.410 0.006 11.143 0.007 7.284 0.008 4.909 0.018 43.68

Notes. The 3.4 μm, 4.6 μm, 12 μm, and 22 μm Vega magnitudes of galaxies and log values of their 12 μm luminosity, mapped by WISE.

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