SKA AA4's broad-band radio coverage, applied to mock galaxy samples, improves star-formation-rate estimates and is forecast to constrain the cosmic star formation history out to z~5-8.
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Tracing cosmic star formation history through radio continuum spectral energy distribution and non-thermal emission
SKA AA4's broad-band radio coverage, applied to mock galaxy samples, improves star-formation-rate estimates and is forecast to constrain the cosmic star formation history out to z~5-8.