The CDF of stellar mass (left panel) and sSFR (right panel) for sGRBs (orange; B. O’Connor et al. 2020; W.-f. Fong et al. 2022; A. E. Nugent et al. 2022), LGRBs (gray; K. M. Svensson et al. 2010; D. A. Perley et al. 2013; F. Y. Wang & Z. G. Dai 2014; S. D. Vergani et al. 2015; Y. Niino et al. 2017), sGRBEEs (dark orange; B. O’Connor et al. 2020; W.-f. Fong et al. 2022; A. E. Nugent et al. 2022), sGRB-KNe (blue), and LGRB-KNe (magenta) with a redshift cut at z  <  0.6. The dashed line shows the GRB-KN host sample as a whole.