Wang et al. (2009) diagrams comparing the Si IIλλ5972, 6355 pEW and Doppler velocity (v(Si II)_abs) measurements from near maximum spectra of the Carnegie Supernova Project sample (Morrell et al. 2024; Ashall et al. 2021). Measurements made from the two nearest to maximum light spectra of ASASSN-20jq are plotted as purple points, as well as those inferred from nearly a dozen peculiar SNe Ia with commonalities with SN 2002es. Branch types are same as in Fig. 12. The vertical line separates normal and high-velocity SNe Ia as defined by Wang et al. (2009).