Estimated local density rate comparison between XT1- and XT2-like objects (derived in this work) and the merger rate of neutron star and BH systems (${\rho }_0^{\mathrm{BHNS}}={130}_{-69}^{+112}$ Gpc⁻³ yr⁻¹; Abbott et al. 2021a), the merger rate of BNS systems (${\rho }_0^{\mathrm{BNS}}={320}_{-240}^{+490}$ Gpc⁻³ yr⁻¹; Abbott et al. 2021b), jetted WD-IMBH TDEs (ρ₀^IMBH = 1.8 − 10 Gpc⁻³ yr⁻¹; Malyali et al. 2019; Tanikawa et al. 2022), LL-LGRBs (ρ_{0, LL − LGRBs} = 150 yr⁻¹ Gpc⁻³, corrected by f_b⁻¹ = 1 − 14; Liang et al. 2007; Zhang 2018), LGRBs (ρ_0, LGRBs = 0.75 yr⁻¹ Gpc⁻³, corrected by f_b⁻¹ = 50 − 500; Wanderman & Piran 2010; Palmerio & Daigne 2021) and SGRBs (ρ_0, SGRBs = 1.75 yr⁻¹ Gpc⁻³, corrected by f_b⁻¹ = 25 − 110; Guetta & Piran 2005; Wanderman & Piran 2015).