The DebrisWatch II preprint (arXiv:2605.27516, May 2026) reprocesses 2.54 m Isaac Newton Telescope observations of geosynchronous orbit using blind stacking and refined astrometric calibration, recovering 25 additional tracklets and extending sensitivity by one magnitude. Methodology relied on single-frame detection followed by post-hoc stacking on a dataset whose size is not quantified in the abstract, with contemporaneous 36 cm astrograph images used only for benchmarking; limitations include the absence of peer review, short-arc orbit solutions that remain preliminary, and photometric variability measurements drawn from objects near the noise floor. These findings matter because GPS, weather, and communications satellites operate in this narrow orbital band where even sub-meter fragments can trigger costly avoidance maneuvers. Earlier surveys such as the 2019 ESA DISCOS catalog updates and the 2023 NASA ODPO high-altitude population models already flagged that optically faint debris constitutes the dominant untracked fraction, yet neither incorporated the high-cadence light-curve analysis showing rapid tumbling among faint fragments that the INT reanalysis now highlights. The original coverage underplayed how commercial-off-the-shelf systems could contribute to routine monitoring if calibrated to sub-arcsecond levels, a capability that could close the coverage-sensitivity trade-off ESA has cited as the chief barrier to persistent GSO surveillance. By connecting the new 25 detections to documented 2024 conjunction alerts involving Intelsat and SES satellites, the scale of risk becomes concrete: each undetected tumbling fragment multiplies the probability of cascading collisions that would degrade services millions depend on daily.