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Fig. 10.


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SFR as a function of IR luminosity for the galaxies of the final sample obtained from the UV-submm SED fitting. Circles are galaxies from the final COSMOS sample, the red ones are galaxies confirmed from their spectra. Diamonds indicate galaxies for which IR data are available and well fitted. The dark purple dashed line shows the Kennicutt & Evans (2012) relation for normal star-forming galaxies.

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