Sub-arcsecond LOFAR imaging of 12 bright sub-millimetre galaxies shows their SED-derived star formation rates are overestimated by a median factor of about five due to companion galaxies and AGN radio emission.
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Sub-arcsecond-resolution LOFAR observations of bright sub-millimetre galaxies in the North Ecliptic Pole field
Sub-arcsecond LOFAR imaging of 12 bright sub-millimetre galaxies shows their SED-derived star formation rates are overestimated by a median factor of about five due to companion galaxies and AGN radio emission.