Fig. 17.
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Plot of log values of the 12 μm luminosity, in erg s−1 units, of the galaxies detected by the WISE W3 band versus the log values of the 1.4 GHz luminosity, in W Hz−1 units, observed in the FIRST survey. The red dots are the data points for the galaxies in our sample. The solid blue line shows the linear regression fit to the data, described by L12 μm = 0.36L1.4 GHz + 35.58.
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