New ALMA data on z>5 radio-loud quasars show synchrotron emission contributes roughly 10% to near 100% of the observed 1 mm continuum in at least four hosts, so dust-based star formation and gas masses for such objects must be treated with caution.
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The host galaxies of radio-loud quasars at z>5 with ALMA
New ALMA data on z>5 radio-loud quasars show synchrotron emission contributes roughly 10% to near 100% of the observed 1 mm continuum in at least four hosts, so dust-based star formation and gas masses for such objects must be treated with caution.