“…We use the new, sharp bounds on the first two of these norms from [39], quoted here as Theorem 2.1, and the sharp bounds on the third of these norms from [ [44]: the mesh thresholds for quasi-optimality in Theorem 1.10 are sharper than the corresponding ones in [44], and the results are valid for a wider class of obstacles. This sharpening is due to the new, sharp bounds on L 2 (∂Ω) → H 1 (∂Ω) norms of S k , D k , and D k from [39], and the widening of the class of obstacles is due to the bound on (A k,η ) −1 L 2 (∂Ω)→L 2 (∂Ω) for nontrapping obstacles from [9,Theorem 1.13]. In more detail: Theorem 1.4 of [44] is the analogue of our Theorem 1.10 except that the former is only valid when Ω is star-shaped with respect to a ball and C 2,α and the mesh threshold is hk (d+1)/2 ≤ C. Comparing this result to Theorem 1.10 we see that we've sharpened the threshold in the d = 3 case, expanded the class of obstacles to nontrapping ones, and added the additional results (b) and (c).…”