Host galaxy characteristics of TeV GRBs presented along with other well-studied lGRBs (shown with cyan circles) and sGRBs (shown using orange circles) to determine if TeV-detected GRBs require unique environments. Top panel: Distribution of host galaxy mass plotted against SFR, with the top X-axis and right side Y-axis representing the histogram of mass and SFR, respectively. The dashed black line represents an sSFR of 1 Gyr⁻¹ Bottom panel: Distribution of host galaxy mass as a function of sSFR, with the top X-axis and right side Y-axis representing the histogram of mass and sSFR, respectively. In these histograms, the vertical red lines show the position of GRB 221009A. The position of GRB 221009A is marked using red diamonds in both figures.