Rest-frame radio SEDs of 160 COSMOS starbursts at z=1.5-3.5 show flatter synchrotron spectra with star formation, and a variable spectral index makes the IR-radio correlation redshift-invariant.
For a uniform field with a constant inclination i with respect to the sky plane ( i = 0 ◦ is the face-on view), c3 = [cos(i)](1+αnt)
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The Radio Spectral Energy Distribution and Star Formation Calibration in MIGHTEE-COSMOS Highly Star-Forming Galaxies at 1.5 < z < 3.5
Rest-frame radio SEDs of 160 COSMOS starbursts at z=1.5-3.5 show flatter synchrotron spectra with star formation, and a variable spectral index makes the IR-radio correlation redshift-invariant.