Nebular phase spectroscopic comparisons of our simulated spectra at 45 d post r-band peak and the observed Ca-rich transients SN 2021gno (Jacobson-Galán et al. 2022; Ertini et al. 2023), SN 2022oqm (Yadavalli et al. 2024), SN 2019ehk (Jacobson-Galán et al. 2020b; Nakaoka et al. 2021), and SN PTF12bho (Lunnan et al. 2017) at similar epochs. The epochs of the observations are relative to the Sloan r-band or Bessel R-band peak. For reference, the dashed grey line is plotted between the rest wavelengths of the key [Ca II] 7291, 7324 Å lines, the Fe I emission feature predicted by the simulation is highlighted in grey, and the location of the [O I] 6300, 6364 Å feature commonly observed for Ca-rich transients is highlighted in green.