The production rate of right-handed neutrinos from a Standard Model plasma ata temperature above a hundred GeV is evaluated up to NLO in Standard Modelcouplings. The results apply in the so-called relativistic regime, referringparametrically to a mass M ~ pi T, generalizing thereby previous NLO resultswhich only apply in the non-relativistic regime M >> pi T. The non-relativisticexpansion is observed to converge for M > 15 T, but the smallness of any loopcorrections allows it to be used in practice already for M > 4 T. In the latterregime any non-covariant dependence of the differential rate on the spatialmomentum is shown to be mild. The loop expansion breaks down in theultrarelativistic regime M << pi T, but after a simple mass resummation itnevertheless extrapolates reasonably well towards a result obtained previouslythrough complete LPM resummation, apparently confirming a strong enhancement ofthe rate at high temperatures (which facilitates chemical equilibration). Whencombined with other ingredients the results may help to improve upon theaccuracy of leptogenesis computations operating above the electroweak scale.