Scatter plots for the low-mass bin (log M_*C = 10.160–10.405) halos probing correlations between the number of satellite galaxies per halo (N_sats), M_*, M_*C, M_200c, M_gas, M_cg, M_bh (all in log M_⊙), and SFR (in M_⊙ yr⁻¹). The 25th (Satellite-poor), 50th, and 75th (Satellite-rich) quartiles are shown as aqua, blue, and teal points, respectively. Histograms for the satellite-poor and satellite-rich quartiles for corresponding halo attributes are also shown in the form of blue and orange bars, respectively.