  Farr and Mandel reanalyse our data, finding initial-mass-function slopes for
high mass stars in 30 Doradus that agree with our results. However, their
reanalysis appears to underpredict the observed number of massive stars. Their
technique results in more precise slopes than in our work, strengthening our
conclusion that there is an excess of massive stars above
$30\,\mathrm{M}_\odot$ in 30 Doradus.
