We performed simulations of the HLVK detector network configuration for the upcoming O5 observing run, estimating the expected gravitational-wave (GW) detection rates using a signal-to-noise ratio (S/N) threshold of 8. The simulated compact-binary population is drawn from the GWTC-4 Broken Power Law + Two Gaussian Peaks (BP2P) population model, ensuring consistency with the latest observational constraints on compact-object mass, spin, and merger-rate distributions. The statistics folder contains summary statistics for both the O4 and projected O5 observing scenarios, enabling direct comparisons of detection rates, source classifications, and population properties between current and anticipated detector sensitivities. Events are classified according to component masses using a standard threshold: neutron stars (NS) are defined as having masses < 3 M⊙, while black holes (BH) are defined as having masses ≥ 3 M⊙. These simulations build on previous observing-scenario studies, including the O4HL, O4HLV, and O5a/O5b/O5c sensitivity projections.