Relation between black hole mass and the host galaxy stellar mass. Our low-redshift LRD analogues are shown as red stars. For comparison, we include high-redshift LRDs from JWST surveys and other low-redshift LRDs. The established local scaling relations for active galaxies from Reines & Volonteri (2015) and inactive galaxies from Greene et al. (2020) are shown as colored dashed lines. The black dashed lines represent different ratios of black hole mass to total stellar mass (M_BH/M_★ = 0.1, 0.01, and 0.001). The arrows and open markers show the effect of increasing the stellar mass of the high-redshift LRDs by a factor of 10.